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Science & Technology
Black holes are portals to the 1st dimension
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<blockquote data-quote="Wind7" data-source="post: 235101" data-attributes="member: 6388"><p><h3><em><strong><span style="color: rgb(247, 218, 100)">Neutron Star</span></strong></em></h3><p><strong><em><span style="color: rgb(247, 218, 100)">"For a sufficiently massive star, an iron core is formed and still the gravitational collapse has enough energy to heat it up to a high enough temperature to either fuse or fission iron. Either in the aftermath of a supernova or in just a collapsing massive star, the energy gets high enough to break down the iron into alpha particles and other smaller units, and still the pressure continues to build. When it reaches the threshold of energy necessary to force the combining of electrons and protons to form neutrons, the <strong><em><strong><em><a href="http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/whdwar.html#c3" target="_blank">electron degeneracy</a></em></strong></em></strong> limit has been passed and the collapse continues until it is stopped by <a href="http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/pulsar.html#c3" target="_blank">neutron degeneracy</a>. At this point it appears that the collapse will stop for stars with mass less than two or three solar masses, and the resulting collection of neutrons is called a neutron star. The periodic emitters called <a href="http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/pulsar.html#c2" target="_blank">pulsars</a> are thought to be neutron stars."</span></em></strong></p><p></p><p>Source;</p><p></p><p>[URL unfurl="true"]http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/pulsar.html#:~:text=Neutron%20Star,either%20fuse%20or%20fission%20iron.[/URL]</p><p></p><p></p><p>Jay Pasachoff</p><p></p><p>[URL unfurl="true"]https://www.google.com/search?gs_ssp=eJzj4tTP1TewNDQuzjBg9OIsSCxOTM7IT0sDAEVjBrY&q=pasachoff&rlz=1C1CHBF_enUS914US914&oq=Pasachoff&aqs=chrome.1.0i355i512j46i512j0i512j0i30l4j0i5i30l3.4010j0j7&sourceid=chrome&ie=UTF-8[/URL]</p></blockquote><p></p>
[QUOTE="Wind7, post: 235101, member: 6388"] [HEADING=2][I][B][COLOR=rgb(247, 218, 100)]Neutron Star[/COLOR][/B][/I][/HEADING] [B][I][COLOR=rgb(247, 218, 100)]"For a sufficiently massive star, an iron core is formed and still the gravitational collapse has enough energy to heat it up to a high enough temperature to either fuse or fission iron. Either in the aftermath of a supernova or in just a collapsing massive star, the energy gets high enough to break down the iron into alpha particles and other smaller units, and still the pressure continues to build. When it reaches the threshold of energy necessary to force the combining of electrons and protons to form neutrons, the [B][I][B][I][URL='http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/whdwar.html#c3']electron degeneracy[/URL][/I][/B][/I][/B] limit has been passed and the collapse continues until it is stopped by [URL='http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/pulsar.html#c3']neutron degeneracy[/URL]. At this point it appears that the collapse will stop for stars with mass less than two or three solar masses, and the resulting collection of neutrons is called a neutron star. The periodic emitters called [URL='http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/pulsar.html#c2']pulsars[/URL] are thought to be neutron stars."[/COLOR][/I][/B] Source; [URL unfurl="true"]http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/pulsar.html#:~:text=Neutron%20Star,either%20fuse%20or%20fission%20iron.[/URL] Jay Pasachoff [URL unfurl="true"]https://www.google.com/search?gs_ssp=eJzj4tTP1TewNDQuzjBg9OIsSCxOTM7IT0sDAEVjBrY&q=pasachoff&rlz=1C1CHBF_enUS914US914&oq=Pasachoff&aqs=chrome.1.0i355i512j46i512j0i512j0i30l4j0i5i30l3.4010j0j7&sourceid=chrome&ie=UTF-8[/URL] [/QUOTE]
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