https://www.pipedija.com/index.php?action=history&feed=atom&title=Neutron-spheres 2026-07-06T11:26:23Z Šio puslapio versijų istorija projekte MediaWiki 1.37.1 https://www.pipedija.com/index.php?title=Neutron-spheres&diff=91715&oldid=prev 2025-11-17T13:36:06Z

<p></p> <table style="background-color: #fff; color: #202122;" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="lt"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Ankstesnė versija</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">16:36, 17 lapkričio 2025 versija</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l27">27 eilutė:</td> <td colspan="2" class="diff-lineno">27 eilutė:</td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>&lt;br&gt; and therefore have higher-frequency photon emissions.</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>&lt;br&gt; and therefore have higher-frequency photon emissions.</div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr> <tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; 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;"><div><del style="font-weight: bold; text-decoration: none;">.</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; 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;"><div> </div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Kategorija:Astronomy and astrophysics]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>[[Kategorija:Astronomy and astrophysics]]</div></td></tr> <!-- diff cache key pipedija_1_37-mediawiki_:diff::1.12:old-91714:rev-91715 --> </table>

Eengglish https://www.pipedija.com/index.php?title=Neutron-spheres&diff=91714&oldid=prev 2025-11-17T13:35:19Z

<p>Naujas puslapis: A &lt;b&gt;neutron-sphere&lt;/b&gt; is one of two possible types of astral-body &lt;br&gt; which remain after a supernova, and which is formed from the core of the &lt;br&gt; supernova&#039;s star. &lt;br&gt; Neutron-spheres are usually called by the misnomer &quot;<a href="/index.php/Neutron_stars" class="mw-redirect" title="Neutron stars">neutron stars</a>&quot;. &lt;br&gt; The other possible type of astral-body that remains is a <a href="/index.php/Quark-sphere" class="mw-redirect" title="Quark-sphere">quark-sphere</a>, &lt;br&gt; which is usually called by the misnomer &quot;<a href="/index.php/Black_hole" title="Black hole">black hole</a>&quot;. Neutron-spheres are composed largely or entirely of &lt;br&gt; neutron-degenerate matter, whic...</p> <p><b>Naujas puslapis</b></p><div>A &lt;b&gt;neutron-sphere&lt;/b&gt; is one of two possible types of astral-body<br /> &lt;br&gt; which remain after a supernova, and which is formed from the core of the<br /> &lt;br&gt; supernova's star.<br /> &lt;br&gt; Neutron-spheres are usually called by the misnomer &quot;[[neutron stars]]&quot;.<br /> &lt;br&gt; The other possible type of astral-body that remains is a [[quark-sphere]],<br /> &lt;br&gt; which is usually called by the misnomer &quot;[[black hole]]&quot;.<br /> <br /> Neutron-spheres are composed largely or entirely of<br /> &lt;br&gt; neutron-degenerate matter, which means that the neutrons are not<br /> &lt;br&gt; organized into separate nuclei.<br /> &lt;br&gt; Consequently, a neutron-sphere is like a giant atomic nucleus.<br /> <br /> The core of a portion of the neutron-spheres, probably the majority thereof,<br /> &lt;br&gt; is composed not of neutron-degenerate matter, but of quark-degenerate matter,<br /> &lt;br&gt; due to the higher pressure therein.<br /> &lt;br&gt; Quark-degenerate matter is what the quark-spheres are composed of.<br /> &lt;br&gt; The more massiv the neutron-sphere, the larger the fraction of its interior is<br /> &lt;br&gt; composed of quark-degenerate matter.<br /> <br /> At the core of that quark-degenerate matter, where the pressure is highest,<br /> &lt;br&gt; the quark-matter is broken-down into high-energy photons.<br /> &lt;br&gt; The energy of those photons depends upon how much energy is put-into<br /> &lt;br&gt; their predecessor-quarks via the extreme pressure, such that the higher the pressure,<br /> &lt;br&gt; the higher the energy of the photons.<br /> &lt;br&gt; Consequently, those photons range in energy from X-rays to &quot;soft&quot; gamma-rays.<br /> &lt;br&gt; By comparison, quark-spheres have higher core-pressure,<br /> &lt;br&gt; and therefore have higher-frequency photon emissions.<br /> <br /> .<br /> [[Kategorija:Astronomy and astrophysics]]</div>

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