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		<id>https://www.evknowledge.org/ekb/index.php?action=history&amp;feed=atom&amp;title=TFNR_-_Cosmic_objects_and_bodies</id>
		<title>TFNR - Cosmic objects and bodies - Revision history</title>
		<link rel="self" type="application/atom+xml" href="https://www.evknowledge.org/ekb/index.php?action=history&amp;feed=atom&amp;title=TFNR_-_Cosmic_objects_and_bodies"/>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;action=history"/>
		<updated>2026-10-22T20:39:03Z</updated>
		<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15930&amp;oldid=prev</id>
		<title>Paolo: /* Evolution */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15930&amp;oldid=prev"/>
				<updated>2026-01-17T17:39:36Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Evolution&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 17:39, 17 January 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L210&quot; &gt;Line 210:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 210:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We have seen how these enigmatic objects form—typically by the collapse of massive stars—and how they structure themselves, with all the different parts that make up their internal and external parts. We've explored how they grow—through the incorporation of Matter: gas, dust, stars, or even other black holes through mergers—and how they interact with the galaxy that hosts them, with intragalactic materials and objects, with compact bodies such as neutron stars, and with other BHs through (gravitational attraction, accretion, mergers, jets and radiation).&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We have seen how these enigmatic objects form—typically by the collapse of massive stars—and how they structure themselves, with all the different parts that make up their internal and external parts. We've explored how they grow—through the incorporation of Matter: gas, dust, stars, or even other black holes through mergers—and how they interact with the galaxy that hosts them, with intragalactic materials and objects, with compact bodies such as neutron stars, and with other BHs through (gravitational attraction, accretion, mergers, jets and radiation).&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The evolution of black holes is a dynamic process''' that unfolds over cosmic time scales, shaping galaxies and influencing the structure of the Universe. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Let’s &lt;/del&gt;now examine some aspects of their possible evolutionary paths.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The evolution of black holes is a dynamic process''' that unfolds over cosmic time scales, shaping galaxies and influencing the structure of the Universe. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Let's &lt;/ins&gt;now examine some aspects of their possible evolutionary paths.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We cannot exclude the possibility that a stellar black hole—especially one with a relatively low Mass, that has not undergone significant accretion or fusion events—'''might wander undisturbed for eternity within its host galaxy, or even in extragalactic space''' (ejected due to dynamic gravitational interactions with very massive objects), without participating in the growth dynamics through fusion with other BHs.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We cannot exclude the possibility that a stellar black hole—especially one with a relatively low Mass, that has not undergone significant accretion or fusion events—'''might wander undisturbed for eternity within its host galaxy, or even in extragalactic space''' (ejected due to dynamic gravitational interactions with very massive objects), without participating in the growth dynamics through fusion with other BHs.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15929&amp;oldid=prev</id>
		<title>Paolo: /* Evolution */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15929&amp;oldid=prev"/>
				<updated>2026-01-17T17:38:48Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Evolution&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 17:38, 17 January 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L208&quot; &gt;Line 208:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 208:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Let's '''review some of the concepts expressed in this section''' to complete the overview of the formation and evolution of black holes.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Let's '''review some of the concepts expressed in this section''' to complete the overview of the formation and evolution of black holes.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We have seen how these enigmatic objects form—typically by the collapse of massive stars—and how they structure themselves, with all the different parts that make up their internal and external parts. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;We’ve &lt;/del&gt;explored how they grow—through the incorporation of Matter: gas, dust, stars, or even other black holes through mergers—and how they interact with the galaxy that hosts them, with intragalactic materials and objects, with compact bodies such as neutron stars, and with other BHs through (gravitational attraction, accretion, mergers, jets and radiation).&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We have seen how these enigmatic objects form—typically by the collapse of massive stars—and how they structure themselves, with all the different parts that make up their internal and external parts. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;We've &lt;/ins&gt;explored how they grow—through the incorporation of Matter: gas, dust, stars, or even other black holes through mergers—and how they interact with the galaxy that hosts them, with intragalactic materials and objects, with compact bodies such as neutron stars, and with other BHs through (gravitational attraction, accretion, mergers, jets and radiation).&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The evolution of black holes is a dynamic process''' that unfolds over cosmic time scales, shaping galaxies and influencing the structure of the Universe. Let’s now examine some aspects of their possible evolutionary paths.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The evolution of black holes is a dynamic process''' that unfolds over cosmic time scales, shaping galaxies and influencing the structure of the Universe. Let’s now examine some aspects of their possible evolutionary paths.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15928&amp;oldid=prev</id>
		<title>Paolo: /* Structure */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15928&amp;oldid=prev"/>
				<updated>2026-01-17T17:37:32Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Structure&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 17:37, 17 January 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L122&quot; &gt;Line 122:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 122:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;**'''Innermost Stable Circular Orbit''' (ISCO) - The ISCO is the smallest orbit in which a Particle can stably revolve around a black hole without spiraling inward. It plays a crucial role in the dynamics of black hole accretion disks, marking the inner edge where matter can orbit before inevitably falling into the event horizon.&amp;lt;br&amp;gt;For a non-rotating (Schwarzschild) black hole, the ISCO lies at a fixed radial distance. However, its position varies depending on the black hole's rotation (or non-rotation) and the direction of orbital motion. If the orbiting particle moves in the same direction as the black hole's spin, the ISCO shifts closer to the event horizon; if it moves in the opposite direction, the ISCO lies farther out.&amp;lt;br&amp;gt;The ISCO influences both the physics of accretion and the gravitational wave signals emitted by spiraling objects. Within the framework of this work, we can say that the ISCO is the analogue, for Vortex InfoStructures, of what the Photon Sphere is for Waves. Vortex InfoStructures possess Mass—even if minimal, as in the case of neutrinos—and inertia, and can reach velocities that approach the limit of propagation for Causality / Action / Information. This causes the ISCO to be positioned slightly farther out than the Photon Sphere.&amp;lt;br&amp;gt;Here too, the level of Perturbation (rate of Time flow) and the directionality of Translation (direction and intensity of gravitational attraction) are decisive.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;**'''Innermost Stable Circular Orbit''' (ISCO) - The ISCO is the smallest orbit in which a Particle can stably revolve around a black hole without spiraling inward. It plays a crucial role in the dynamics of black hole accretion disks, marking the inner edge where matter can orbit before inevitably falling into the event horizon.&amp;lt;br&amp;gt;For a non-rotating (Schwarzschild) black hole, the ISCO lies at a fixed radial distance. However, its position varies depending on the black hole's rotation (or non-rotation) and the direction of orbital motion. If the orbiting particle moves in the same direction as the black hole's spin, the ISCO shifts closer to the event horizon; if it moves in the opposite direction, the ISCO lies farther out.&amp;lt;br&amp;gt;The ISCO influences both the physics of accretion and the gravitational wave signals emitted by spiraling objects. Within the framework of this work, we can say that the ISCO is the analogue, for Vortex InfoStructures, of what the Photon Sphere is for Waves. Vortex InfoStructures possess Mass—even if minimal, as in the case of neutrinos—and inertia, and can reach velocities that approach the limit of propagation for Causality / Action / Information. This causes the ISCO to be positioned slightly farther out than the Photon Sphere.&amp;lt;br&amp;gt;Here too, the level of Perturbation (rate of Time flow) and the directionality of Translation (direction and intensity of gravitational attraction) are decisive.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;**'''Accretion Disk''' (if present) - Although not part of the black hole itself, this is a surrounding disk of superheated Matter spiraling inward, emitting intense radiation before crossing the event horizon. It consists of Ordinary (visible) Matter in the form of Particles of various types—including &amp;quot;exotic&amp;quot; ones formed under extreme energetic conditions (temperature, collisions, etc.)—ionized atoms, electrons, gas, dust, and fragments of stellar objects torn apart by gravitational forces.&amp;lt;br&amp;gt;Here too, the slowing of Time associated with the Perturbation gradient, and the Translation orientation toward the center of Mass of the BH (gravitational attraction), cause this Matter to spiral inward until it crosses the event horizon. Part of the Energy—kinetic, thermal, electromagnetic, nuclear—and part of the Mass of this rotating Matter escapes, emitted in the form of Dark and Ordinary Waves (Gravitational Waves and Electromagnetic Waves, respectively).&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;**'''Accretion Disk''' (if present) - Although not part of the black hole itself, this is a surrounding disk of superheated Matter spiraling inward, emitting intense radiation before crossing the event horizon. It consists of Ordinary (visible) Matter in the form of Particles of various types—including &amp;quot;exotic&amp;quot; ones formed under extreme energetic conditions (temperature, collisions, etc.)—ionized atoms, electrons, gas, dust, and fragments of stellar objects torn apart by gravitational forces.&amp;lt;br&amp;gt;Here too, the slowing of Time associated with the Perturbation gradient, and the Translation orientation toward the center of Mass of the BH (gravitational attraction), cause this Matter to spiral inward until it crosses the event horizon. Part of the Energy—kinetic, thermal, electromagnetic, nuclear—and part of the Mass of this rotating Matter escapes, emitted in the form of Dark and Ordinary Waves (Gravitational Waves and Electromagnetic Waves, respectively).&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;**'''Relativistic Jets''' - These are powerful streams of ionized Matter ejected from the vicinity of black holes at speeds approaching that of light. Jets are commonly associated with active galactic nuclei (AGN), quasars, and radio galaxies, where supermassive black holes drive extreme astrophysical processes.&amp;lt;br&amp;gt;Astrophysics explains that intense gravitational forces and magnetic fields heat the Matter to extreme temperatures, which accumulates in the accretion disk awaiting infall. Magnetic fields within the disk play a key role in jet formation. Twisted and tangled magnetic field lines near the black hole can channel plasma outward, emitting jets along the black &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;hole’s &lt;/del&gt;rotation axis.&amp;lt;br&amp;gt;In rotating black holes, the relativistic frame-dragging effect further influences jet formation and acceleration, producing speeds near the speed of light. Some jets extend millions of light-years into intergalactic space, shaping their environment, influencing galaxy formation, redistributing Energy and Matter, and regulating star formation by heating interstellar gas. Jets emit radiation across the electromagnetic spectrum, including radio waves, X-rays, and gamma rays.&amp;lt;br&amp;gt;What can we add to this conventional picture? First, we can hypothesize that the magnetic fields relevant to jet formation are not only those generated within the accretion disk by rotation and ionization. Let us recall what was previously illustrated: the main body of a black hole consists of a super-Particle, endowed with Mass, extrinsic linear and angular Motion, Charge (Chirality), and Spin—defined by the orientation of the axis of intrinsic rotation (which may coincide with the axis of extrinsic rotation).&amp;lt;br&amp;gt;It is precisely this Spin, which reorients the Spins of all the event-points of the Elementary Field in the internal and external regions that momentarily support the BH, that transforms the BH into an immense magnet. Due to its extremely rapid extrinsic rotation and the frame-dragging effect, the BH shapes the magnetic field lines (derived from Spin) into complex, spiral, and focused structures directed toward and out of its poles.&amp;lt;br&amp;gt;These structures—partly chaotic, turbulent, and spiraling—form a natural particle accelerator, capable of projecting Matter across vast distances at extremely high speeds and energy levels. Interactions within the jets, and with the interstellar medium and galactic magnetic field lines, produce significant energetic effects, including strong emissions of Electromagnetic Waves spanning the entire spectrum.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;**'''Relativistic Jets''' - These are powerful streams of ionized Matter ejected from the vicinity of black holes at speeds approaching that of light. Jets are commonly associated with active galactic nuclei (AGN), quasars, and radio galaxies, where supermassive black holes drive extreme astrophysical processes.&amp;lt;br&amp;gt;Astrophysics explains that intense gravitational forces and magnetic fields heat the Matter to extreme temperatures, which accumulates in the accretion disk awaiting infall. Magnetic fields within the disk play a key role in jet formation. Twisted and tangled magnetic field lines near the black hole can channel plasma outward, emitting jets along the black &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;hole's &lt;/ins&gt;rotation axis.&amp;lt;br&amp;gt;In rotating black holes, the relativistic frame-dragging effect further influences jet formation and acceleration, producing speeds near the speed of light. Some jets extend millions of light-years into intergalactic space, shaping their environment, influencing galaxy formation, redistributing Energy and Matter, and regulating star formation by heating interstellar gas. Jets emit radiation across the electromagnetic spectrum, including radio waves, X-rays, and gamma rays.&amp;lt;br&amp;gt;What can we add to this conventional picture? First, we can hypothesize that the magnetic fields relevant to jet formation are not only those generated within the accretion disk by rotation and ionization. Let us recall what was previously illustrated: the main body of a black hole consists of a super-Particle, endowed with Mass, extrinsic linear and angular Motion, Charge (Chirality), and Spin—defined by the orientation of the axis of intrinsic rotation (which may coincide with the axis of extrinsic rotation).&amp;lt;br&amp;gt;It is precisely this Spin, which reorients the Spins of all the event-points of the Elementary Field in the internal and external regions that momentarily support the BH, that transforms the BH into an immense magnet. Due to its extremely rapid extrinsic rotation and the frame-dragging effect, the BH shapes the magnetic field lines (derived from Spin) into complex, spiral, and focused structures directed toward and out of its poles.&amp;lt;br&amp;gt;These structures—partly chaotic, turbulent, and spiraling—form a natural particle accelerator, capable of projecting Matter across vast distances at extremely high speeds and energy levels. Interactions within the jets, and with the interstellar medium and galactic magnetic field lines, produce significant energetic effects, including strong emissions of Electromagnetic Waves spanning the entire spectrum.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== Formation ====&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== Formation ====&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15875&amp;oldid=prev</id>
		<title>Paolo: /* In conclusion */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15875&amp;oldid=prev"/>
				<updated>2026-01-15T17:32:55Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;In conclusion&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 17:32, 15 January 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L228&quot; &gt;Line 228:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 228:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== In conclusion ====&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== In conclusion ====&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;This is '''a very broad topic'''. Here, we have only scratched the surface. Much deeper investigation would be necessary to fully grasp the complexity and richness of the subject. But I hope the essence of what &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;I’ve &lt;/del&gt;expressed regarding some aspects of these enigmatic and frightening objects is clear. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;This is '''a very broad topic'''. Here, we have only scratched the surface. Much deeper investigation would be necessary to fully grasp the complexity and richness of the subject. But I hope the essence of what &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;I've &lt;/ins&gt;expressed regarding some aspects of these enigmatic and frightening objects is clear. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''In extreme summary''', for me:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''In extreme summary''', for me:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15874&amp;oldid=prev</id>
		<title>Paolo: /* Formation */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15874&amp;oldid=prev"/>
				<updated>2026-01-15T17:32:28Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Formation&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 17:32, 15 January 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L130&quot; &gt;Line 130:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 130:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''We exclude the hypothesis of primordial black hole''' formation in the early Universe through density fluctuations shortly after the Big Bang. No Big Bang, no primordial black holes!&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''We exclude the hypothesis of primordial black hole''' formation in the early Universe through density fluctuations shortly after the Big Bang. No Big Bang, no primordial black holes!&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The most plausible hypothesis''', especially within the framework proposed here regarding the formation of the Universe and its constituent objects and structures, is that of '''stellar collapse''': an extreme gravitational implosion typically occurring at the end of a massive &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;star’s &lt;/del&gt;life cycle. When such a star exhausts its nuclear fuel, it can no longer resist gravitational forces. Its core collapses under its own weight, triggering a '''supernova explosion''' that ejects the outer layers. If the remaining core is sufficiently massive (around 2.&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;7–3 &lt;/del&gt;solar masses), it continues collapsing, forming a '''stellar-mass black hole'''. But, as stated above, '''no singularity'''.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The most plausible hypothesis''', especially within the framework proposed here regarding the formation of the Universe and its constituent objects and structures, is that of '''stellar collapse''': an extreme gravitational implosion typically occurring at the end of a massive &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;star's &lt;/ins&gt;life cycle. When such a star exhausts its nuclear fuel, it can no longer resist gravitational forces. Its core collapses under its own weight, triggering a '''supernova explosion''' that ejects the outer layers. If the remaining core is sufficiently massive (around 2.&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;7-3 &lt;/ins&gt;solar masses), it continues collapsing, forming a '''stellar-mass black hole'''. But, as stated above, '''no singularity'''.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Black holes of greater mass may form through the '''collapse of more massive stars''' or via the '''progressive aggregation of matter''' by a black hole already formed through stellar collapse. Even more massive black holes likely emerge through the '''incorporation of stellar objects, mergers with neutron stars, or other black holes'''.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Black holes of greater mass may form through the '''collapse of more massive stars''' or via the '''progressive aggregation of matter''' by a black hole already formed through stellar collapse. Even more massive black holes likely emerge through the '''incorporation of stellar objects, mergers with neutron stars, or other black holes'''.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L136&quot; &gt;Line 136:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 136:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The general structure of a galaxy''', with its dark (invisible) and ordinary (visible) components, can be configured as an immense '''gravitational well''', attracting matter toward its center of Mass, which presumably coincides with its center / axis of rotation. As if the galactic nucleus were the hub of a colossal wheel—a '''gigantic Vortex''' whose shape, Mass profile, and specific dynamics draw Matter inward, facilitating successive fusions of massive objects into increasingly larger black holes. These very massive objects, barring interactions that eject them, will tend to fall toward the galactic interior, where a central black hole resides and continues to grow through the collapse of gas, dust, stars, and—of course—other black holes, even very massive ones.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''The general structure of a galaxy''', with its dark (invisible) and ordinary (visible) components, can be configured as an immense '''gravitational well''', attracting matter toward its center of Mass, which presumably coincides with its center / axis of rotation. As if the galactic nucleus were the hub of a colossal wheel—a '''gigantic Vortex''' whose shape, Mass profile, and specific dynamics draw Matter inward, facilitating successive fusions of massive objects into increasingly larger black holes. These very massive objects, barring interactions that eject them, will tend to fall toward the galactic interior, where a central black hole resides and continues to grow through the collapse of gas, dust, stars, and—of course—other black holes, even very massive ones.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''Significant contributions to the formation of supermassive black holes''', such as those found at galactic centers, in active galactic nuclei, quasars, etc., undoubtedly '''arise from galactic interactions and mergers''', especially involving '''dwarf galaxies'''. It is reasonable to assume that the probability of central black hole fusion during a galactic merger is higher when the merger involves a '''satellite dwarf galaxy'''. The trajectory of such a satellite is more likely directed toward the host &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;galaxy’s &lt;/del&gt;center, and the disparity in size and mass increases the likelihood that the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;satellite’s &lt;/del&gt;entire stellar population remains within the host. Simultaneously, the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;satellite’s &lt;/del&gt;central black hole is very likely to approach and merge with the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;host’s &lt;/del&gt;central black hole, which—due to its immense mass—exerts a '''formidable gravitational pull'''.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''Significant contributions to the formation of supermassive black holes''', such as those found at galactic centers, in active galactic nuclei, quasars, etc., undoubtedly '''arise from galactic interactions and mergers''', especially involving '''dwarf galaxies'''. It is reasonable to assume that the probability of central black hole fusion during a galactic merger is higher when the merger involves a '''satellite dwarf galaxy'''. The trajectory of such a satellite is more likely directed toward the host &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;galaxy's &lt;/ins&gt;center, and the disparity in size and mass increases the likelihood that the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;satellite's &lt;/ins&gt;entire stellar population remains within the host. Simultaneously, the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;satellite's &lt;/ins&gt;central black hole is very likely to approach and merge with the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;host's &lt;/ins&gt;central black hole, which—due to its immense mass—exerts a '''formidable gravitational pull'''.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;I do not believe that the formation of supermassive black holes (SMBHs) occurs '''via direct collapse of massive gas clouds'''. An '''intermediate stellar phase is, in my view, the norm'''. A galactic cloud collapses into a star, which exhausts its fuel and collapses into a black hole, initiating a growth trajectory as hypothesized above. In my opinion, gas and dust can feed black holes, but not cause them to form from scratch.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;I do not believe that the formation of supermassive black holes (SMBHs) occurs '''via direct collapse of massive gas clouds'''. An '''intermediate stellar phase is, in my view, the norm'''. A galactic cloud collapses into a star, which exhausts its fuel and collapses into a black hole, initiating a growth trajectory as hypothesized above. In my opinion, gas and dust can feed black holes, but not cause them to form from scratch.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15873&amp;oldid=prev</id>
		<title>Paolo: /* Structure */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=15873&amp;oldid=prev"/>
				<updated>2026-01-15T17:31:34Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Structure&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;a href=&quot;https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;amp;diff=15873&amp;amp;oldid=14252&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14252&amp;oldid=prev</id>
		<title>Paolo: /* In conclusion */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14252&amp;oldid=prev"/>
				<updated>2025-07-17T15:43:29Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;In conclusion&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 15:43, 17 July 2025&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L232&quot; &gt;Line 232:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 232:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''In extreme summary''', for me:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;'''In extreme summary''', for me:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*black holes are '''not just gravitational traps'''—they are '''dynamic, evolving structures that shape the architecture of the Universe'''&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*black holes are '''not just gravitational traps'''—they are '''dynamic, evolving structures that shape the architecture of the Universe'''&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*their &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;interactions—through &lt;/del&gt;accretion, mergers, jets, and field &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;dynamics—are &lt;/del&gt;central to the cosmic narrative&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*their &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''interactions'''—through &lt;/ins&gt;accretion, mergers, jets, and field &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;dynamics—'''are &lt;/ins&gt;central to the cosmic narrative&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*they '''have a structure, including an internal one''', within Ordinary Matter, even if it is very strange and exotic, which makes them up&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*they '''have a structure, including an internal one''', within Ordinary Matter, even if it is very strange and exotic, which makes them up&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''their core can be represented as a super-particle'''&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''their core can be represented as a super-particle'''&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14251&amp;oldid=prev</id>
		<title>Paolo: /* In conclusion */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14251&amp;oldid=prev"/>
				<updated>2025-07-17T15:43:07Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;In conclusion&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 15:43, 17 July 2025&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L228&quot; &gt;Line 228:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 228:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== In conclusion ====&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== In conclusion ====&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;This is a very broad topic. Here, we have only scratched the surface. Much deeper investigation would be necessary. But I hope the essence of what &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;I said &lt;/del&gt;regarding some aspects of these enigmatic and frightening objects is clear. In extreme summary, for me:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;This is &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;a very broad topic&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;. Here, we have only scratched the surface. Much deeper investigation would be necessary &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;to fully grasp the complexity and richness of the subject&lt;/ins&gt;. But I hope the essence of what &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;I’ve expressed &lt;/ins&gt;regarding some aspects of these enigmatic and frightening objects is clear. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;black holes &lt;/del&gt;have a structure, including an internal one''', within Ordinary Matter, even if it is very strange and exotic, which makes them up&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;In extreme summary&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;, for me:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;black holes are '''not just gravitational traps'''—they are '''dynamic, evolving structures that shape the architecture of the Universe'''&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;*their interactions—through accretion, mergers, jets, and field dynamics—are central to the cosmic narrative&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;*they &lt;/ins&gt;'''have a structure, including an internal one''', within Ordinary Matter, even if it is very strange and exotic, which makes them up&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''their core can be represented as a super-particle'''&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''their core can be represented as a super-particle'''&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''no singularity''' (which, in this model, as stated, cannot exist)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''no singularity''' (which, in this model, as stated, cannot exist)&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14250&amp;oldid=prev</id>
		<title>Paolo: /* In conclusion */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14250&amp;oldid=prev"/>
				<updated>2025-07-17T15:38:33Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;In conclusion&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;col class='diff-marker' /&gt;
				&lt;col class='diff-content' /&gt;
				&lt;tr style='vertical-align: top;'&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 15:38, 17 July 2025&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L231&quot; &gt;Line 231:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 231:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''black holes have a structure, including an internal one''', within Ordinary Matter, even if it is very strange and exotic, which makes them up&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''black holes have a structure, including an internal one''', within Ordinary Matter, even if it is very strange and exotic, which makes them up&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''their core can be represented as a super-particle'''&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''their core can be represented as a super-particle'''&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;cannot host a &lt;/del&gt;singularity''' (which, in this model, as stated, cannot exist)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;no &lt;/ins&gt;singularity''' (which, in this model, as stated, cannot exist)&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''no primordial black holes''' exist (there was no Big Bang, and the only way black holes can form and evolve is through collapse and accretion&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*'''no primordial black holes''' exist (there was no Big Bang, and the only way black holes can form and evolve is through collapse and accretion&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;#160; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;#160; &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{Template:PaperPages1}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{Template:PaperPages1}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

	<entry>
		<id>https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14249&amp;oldid=prev</id>
		<title>Paolo: /* Evolution */</title>
		<link rel="alternate" type="text/html" href="https://www.evknowledge.org/ekb/index.php?title=TFNR_-_Cosmic_objects_and_bodies&amp;diff=14249&amp;oldid=prev"/>
				<updated>2025-07-17T15:37:58Z</updated>
		
		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Evolution&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class='diff diff-contentalign-left'&gt;
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				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='2' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 15:37, 17 July 2025&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;L206&quot; &gt;Line 206:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 206:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== Evolution ====&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== Evolution ====&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Let's review some of the concepts expressed in this section to complete the overview of the formation and evolution of black holes.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Let's &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;review some of the concepts expressed in this section&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;''' &lt;/ins&gt;to complete the overview of the formation and evolution of black holes.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We have seen how these enigmatic objects &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;form (typically &lt;/del&gt;by the collapse of massive &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;stars) and &lt;/del&gt;structure themselves &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;(&lt;/del&gt;with all the different parts that make up &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;the &lt;/del&gt;internal and external &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;structures), &lt;/del&gt;how they &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;grow (&lt;/del&gt;incorporation of &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;matter&lt;/del&gt;: gas, dust, stars or even other black holes&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;), &lt;/del&gt;how they interact with the galaxy that hosts them, with intragalactic materials and objects, with compact &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;objects &lt;/del&gt;such as neutron stars and &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;the black holes themselves &lt;/del&gt;(gravitational attraction, accretion, mergers, jets and radiation).&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We have seen how these enigmatic objects &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;form—typically &lt;/ins&gt;by the collapse of massive &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;stars—and how they &lt;/ins&gt;structure themselves&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;with all the different parts that make up &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;their &lt;/ins&gt;internal and external &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;parts. We’ve explored &lt;/ins&gt;how they &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;grow—through the &lt;/ins&gt;incorporation of &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Matter&lt;/ins&gt;: gas, dust, stars&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;or even other black holes &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;through mergers—and &lt;/ins&gt;how they interact with the galaxy that hosts them, with intragalactic materials and objects, with compact &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;bodies &lt;/ins&gt;such as neutron stars&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;and &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;with other BHs through &lt;/ins&gt;(gravitational attraction, accretion, mergers, jets and radiation).&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The evolution of black holes is a dynamic process that &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;develops on &lt;/del&gt;cosmic time scales, shaping galaxies and influencing the structure of the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;universe&lt;/del&gt;. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Let's &lt;/del&gt;now &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;look at &lt;/del&gt;some aspects of their possible evolutionary &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;path&lt;/del&gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;The evolution of black holes is a dynamic process&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;''' &lt;/ins&gt;that &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;unfolds over &lt;/ins&gt;cosmic time scales, shaping galaxies and influencing the structure of the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Universe&lt;/ins&gt;. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Let’s &lt;/ins&gt;now &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;examine &lt;/ins&gt;some aspects of their possible evolutionary &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;paths&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We cannot exclude that a stellar black &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;hole (especially &lt;/del&gt;one with a &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;not too high mass&lt;/del&gt;, &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;a black hole &lt;/del&gt;that has not undergone &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;some &lt;/del&gt;accretion &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;by &lt;/del&gt;fusion&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, or in any case few events of this type) can &lt;/del&gt;wander undisturbed for eternity &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;in the &lt;/del&gt;galaxy &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;that hosts it &lt;/del&gt;or even in extragalactic space (&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;ejection &lt;/del&gt;due to dynamic &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;effects of &lt;/del&gt;gravitational &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;interaction &lt;/del&gt;with very massive objects) without &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;interacting with &lt;/del&gt;the growth dynamics &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;by &lt;/del&gt;fusion &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;of &lt;/del&gt;other &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;black holes&lt;/del&gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;We cannot exclude &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;the possibility &lt;/ins&gt;that a stellar black &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;hole—especially &lt;/ins&gt;one with a &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;relatively low Mass&lt;/ins&gt;, that has not undergone &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;significant &lt;/ins&gt;accretion &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;or &lt;/ins&gt;fusion &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;events—'''might &lt;/ins&gt;wander undisturbed for eternity &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;within its host &lt;/ins&gt;galaxy&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;or even in extragalactic space&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;''' &lt;/ins&gt;(&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;ejected &lt;/ins&gt;due to dynamic gravitational &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;interactions &lt;/ins&gt;with very massive objects)&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;without &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;participating in &lt;/ins&gt;the growth dynamics &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;through &lt;/ins&gt;fusion &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;with &lt;/ins&gt;other &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;BHs&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;But &lt;/del&gt;it is more reasonable to &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;think &lt;/del&gt;that the strong gravitational attraction of these &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;objects, increasingly greater &lt;/del&gt;as their &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;mass increases, brings &lt;/del&gt;them &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;towards &lt;/del&gt;increasingly crowded galactic regions, multiplying the probability of &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;incurring &lt;/del&gt;mergers with other BHs. In general, the more massive the object, the greater its tendency to escape local dynamics&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, to &lt;/del&gt;follow a long-term &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;trend &lt;/del&gt;that leads it &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;to get closer and &lt;/del&gt;closer to the galactic center, where a supermassive black hole &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;is waiting &lt;/del&gt;to &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;swallow it, after &lt;/del&gt;a gravitational dance that &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;can &lt;/del&gt;be &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;very long &lt;/del&gt;but &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;with an &lt;/del&gt;inexorable &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;outcome &lt;/del&gt;(except &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;for &lt;/del&gt;rare cases of gravitational kick &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;that can throw &lt;/del&gt;the approaching &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;black hole &lt;/del&gt;into &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;the &lt;/del&gt;deep &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;cosmos&lt;/del&gt;).&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;However, &lt;/ins&gt;it is more reasonable to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;assume &lt;/ins&gt;that the strong gravitational attraction of these &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;objects—growing stronger &lt;/ins&gt;as their &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Mass increases—draws &lt;/ins&gt;them &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;toward &lt;/ins&gt;increasingly crowded galactic regions, multiplying the probability of &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;encountering &lt;/ins&gt;mergers with other BHs. In general, the more massive the object, the greater its tendency to escape local dynamics &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;and &lt;/ins&gt;follow &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;a long-term &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;trajectory &lt;/ins&gt;that leads it &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;ever &lt;/ins&gt;closer to the galactic center&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;, where a supermassive black hole &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;(SMBH) awaits &lt;/ins&gt;to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;absorb it—after &lt;/ins&gt;a gravitational dance that &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;may &lt;/ins&gt;be &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;prolonged &lt;/ins&gt;but &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;ultimately &lt;/ins&gt;inexorable (except &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;in &lt;/ins&gt;rare cases of gravitational kick&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, which may hurl &lt;/ins&gt;the approaching &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;BH &lt;/ins&gt;into deep &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;space&lt;/ins&gt;).&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;As for SMBHs, in their evolution we certainly find the formation of accretion disks, which generate intense radiation and sometimes produce quasars, among the brightest objects in the universe. And again, the active participation in the interaction dynamics in the merger between galaxies, perhaps without then encountering a merger with the SMBH of the other galaxy, but still greatly influencing the outcome of the galactic merger. Let us also remember phenomena such as the emission of powerful gravitational waves and the evolution of spin (due to accretion and mergers), which can influence their ability to generate relativistic jets, high-speed particle flows and electromagnetic radiation.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;As for SMBHs, in their evolution we certainly find the formation of accretion disks, which generate intense radiation and sometimes produce quasars, among the brightest objects in the universe. And again, the active participation in the interaction dynamics in the merger between galaxies, perhaps without then encountering a merger with the SMBH of the other galaxy, but still greatly influencing the outcome of the galactic merger. Let us also remember phenomena such as the emission of powerful gravitational waves and the evolution of spin (due to accretion and mergers), which can influence their ability to generate relativistic jets, high-speed particle flows and electromagnetic radiation.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Regarding the final fate of a black hole, there is much &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;talk of &lt;/del&gt;evaporation, Hawking Radiation, and &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;so on&lt;/del&gt;. After having rejected the possibility that some &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;of them &lt;/del&gt;could originate from primordial black &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;holes (an &lt;/del&gt;impossible hypothesis&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/del&gt;in a Universe without a Big &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Bang), I &lt;/del&gt;would also reject the hypothesis of their disappearance &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;by &lt;/del&gt;evaporation, even if &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;in &lt;/del&gt;an almost infinite time. This supposed phenomenon does not seem plausible to me&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, and in any case, &lt;/del&gt;even if it were possible, I believe its effect would be so modest and diluted over &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;an &lt;/del&gt;immense time that in my opinion it would not significantly influence the dynamics and fates of black &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;holes and &lt;/del&gt;more generally of the Universe. Yes, I &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;understand, &lt;/del&gt;it is a central aspect in the attempt to understand the relationships between Relativity and the quantum world. But I believe that, for this purpose, it will be necessary to &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;find &lt;/del&gt;other more &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;&amp;quot;&lt;/del&gt;concrete&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;&amp;quot; &lt;/del&gt;and &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;&amp;quot;&lt;/del&gt;observable&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;&amp;quot; &lt;/del&gt;phenomena.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;As for SMBHs, '''their evolution certainly includes the formation of accretion disks,''' which generate intense radiation and sometimes produce quasars—among the brightest objects in the Universe. They also play an active role in the interaction dynamics during galactic mergers, even if they do not always merge with the SMBH of the other interacting galaxy. Nevertheless, they significantly influence the outcome of the galactic merger. Let us also recall phenomena such as:&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;*emission of powerful gravitational waves&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;*evolution of Spin and the orientation of its axis (due to accretion and mergers)&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;*generation of relativistic jets—high-speed particle flows and electromagnetic radiation&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;These processes are not only central to the life cycle of black holes but also to the broader architecture and evolution of the cosmos.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;Regarding the final fate of a black hole&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;, there is much &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;discussion about &lt;/ins&gt;evaporation, Hawking Radiation, and &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;related phenomena&lt;/ins&gt;. After having rejected the possibility that some &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;black holes &lt;/ins&gt;could originate from primordial black &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;holes—an &lt;/ins&gt;impossible hypothesis in a Universe without a Big &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Bang—I &lt;/ins&gt;would also reject the hypothesis of their disappearance &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;through &lt;/ins&gt;evaporation, even if &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;occurring over &lt;/ins&gt;an almost infinite time &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;scale&lt;/ins&gt;. This supposed phenomenon does not seem plausible to me&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;. And &lt;/ins&gt;even if it were possible, I believe its effect would be so modest and diluted over &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;such &lt;/ins&gt;immense time &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;spans &lt;/ins&gt;that&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;in my opinion&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;it would not significantly influence the dynamics and fates of black &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;holes—or, &lt;/ins&gt;more generally&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;of the Universe. Yes, I &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;see: &lt;/ins&gt;it is a central aspect in the attempt to understand the relationships between Relativity and the quantum world. But I believe that, &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;for this purpose, it will be necessary to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;identify &lt;/ins&gt;other&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;more concrete and observable phenomena&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;'''&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== In conclusion ====&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==== In conclusion ====&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Paolo</name></author>	</entry>

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