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Pasta nuklir - Riwayat revisi
2026-09-16T00:17:18Z
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<p>Presentation V4: sitasi, referensi, Math, Wikimedia Commons, dan atribusi</p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Revisi sebelumnya</td>
<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revisi per 26 Agustus 2026 09.23</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1">Baris 1:</td>
<td colspan="2" class="diff-lineno">Baris 1:</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;">Dalam bidang </del>[[<del style="font-weight: bold; text-decoration: none;">astrofisika]] dan [[fisika nuklir]</del>]<del style="font-weight: bold; text-decoration: none;">, '''pasta nuklir''' adalah jenis [[materi degenerat</del>]<del style="font-weight: bold; text-decoration: none;">] teoretis yang diduga terbentuk di dalam kerak [[bintang neutron]]. Jika keberadaannya benar, pasta nuklir diyakini sebagai material terkuat di alam semesta.</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>[[<ins style="font-weight: bold; text-decoration: none;">File:Neutron_star_cross_section.svg|thumb|right|280px|Neutron star cross section</ins>]]</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;">Di antara permukaan bintang neutron dan </del>[[<del style="font-weight: bold; text-decoration: none;">plasma kuark–gluon</del>]] <del style="font-weight: bold; text-decoration: none;">di intinya, pada kerapatan materi sekitar 10<sup>14</sup>&nbsp;g/cm<sup>3</sup>, </del>[[<del style="font-weight: bold; text-decoration: none;">gaya </del>nuklir]] <del style="font-weight: bold; text-decoration: none;">dan </del>[[<del style="font-weight: bold; text-decoration: none;">tolakan Coulomb</del>]] <del style="font-weight: bold; text-decoration: none;">memiliki besaran </del>yang <del style="font-weight: bold; text-decoration: none;">sebanding. Persaingan antara kedua gaya ini memunculkan berbagai struktur kompleks yang tersusun atas </del>[[neutron]] <del style="font-weight: bold; text-decoration: none;">dan </del>[<del style="font-weight: bold; text-decoration: none;">[proton]</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><ins style="font-weight: bold; text-decoration: none;">Dalam bidang </ins>[[<ins style="font-weight: bold; text-decoration: none;">astrofisika</ins>]] <ins style="font-weight: bold; text-decoration: none;">dan </ins>[[<ins style="font-weight: bold; text-decoration: none;">fisika </ins>nuklir]]<ins style="font-weight: bold; text-decoration: none;">, '''pasta nuklir''' adalah jenis </ins>[[<ins style="font-weight: bold; text-decoration: none;">materi degenerat</ins>]] <ins style="font-weight: bold; text-decoration: none;">teoretis </ins>yang <ins style="font-weight: bold; text-decoration: none;">diduga terbentuk di dalam kerak </ins>[[<ins style="font-weight: bold; text-decoration: none;">bintang </ins>neutron]]<ins style="font-weight: bold; text-decoration: none;">. Jika keberadaannya benar, pasta nuklir diyakini sebagai material terkuat di alam semesta.<ref>M. E. Caplan. </ins>[<ins style="font-weight: bold; text-decoration: none;">https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.121.132701 Elasticity of Nuclear Pasta</ins>]. <ins style="font-weight: bold; text-decoration: none;">''Physical Review Letters''. 24 September 2018. Vol. 121 (13). doi:10.1103/PhysRevLett.121.132701.</ref> </ins></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;">Para astrofisikawan menamai struktur-struktur </del>ini <del style="font-weight: bold; text-decoration: none;">sebagai ''pasta nuklir'' karena bentuk geometrinya menyerupai </del>berbagai <del style="font-weight: bold; text-decoration: none;">jenis </del>[[<del style="font-weight: bold; text-decoration: none;">pasta</del>]] <del style="font-weight: bold; text-decoration: none;">Italia, seperti lembaran, tabung, atau spiral</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><ins style="font-weight: bold; text-decoration: none;">Di antara permukaan bintang neutron dan [[plasma kuark–gluon]] di intinya, pada kerapatan materi sekitar 10<sup>14</sup>&nbsp;g/cm<sup>3</sup>, [[gaya nuklir]] dan [[tolakan Coulomb]] memiliki besaran yang sebanding. Persaingan antara kedua gaya </ins>ini <ins style="font-weight: bold; text-decoration: none;">memunculkan </ins>berbagai <ins style="font-weight: bold; text-decoration: none;">struktur kompleks yang tersusun atas </ins>[[<ins style="font-weight: bold; text-decoration: none;">neutron]] dan [[proton</ins>]]. <ins style="font-weight: bold; text-decoration: none;"> </ins></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;">==Referensi==</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><ins style="font-weight: bold; text-decoration: none;">Para astrofisikawan menamai struktur-struktur ini sebagai ''pasta nuklir'' karena bentuk geometrinya menyerupai berbagai jenis [[pasta]] Italia, seperti lembaran, tabung, atau spiral.<ref>José A. Pons. ''Too much "pasta" for pulsars to spin down''. ''Nature Physics''. 2013. Vol. 9 (7). hlm. 431–434. doi:10.1038/nphys2640.</ref><ref>David Reagan. [http://racinfo.indiana.edu/research/scholarly-highlights/articles/nuclear-pasta.php Visualizations of Nuclear Pasta]. Advanced Visualization Lab, Research Technologies, Indiana University.</ref></ins></div></td></tr>
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<tr><td colspan="2" class="diff-side-deleted"></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><ins style="font-weight: bold; text-decoration: none;">== Referensi ==</ins></div></td></tr>
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<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 colspan="2" class="diff-side-deleted"></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><ins style="font-weight: bold; text-decoration: none;">== Sumber dan atribusi ==</ins></div></td></tr>
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<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;">Sumber </del>dan <del style="font-weight: bold; text-decoration: none;">atribusi ==</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><ins style="font-weight: bold; text-decoration: none;">Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title</ins>=<ins style="font-weight: bold; text-decoration: none;">Pasta+nuklir&oldid</ins>=<ins style="font-weight: bold; text-decoration: none;">29331664 Wikipedia bahasa Indonesia], revisi 29331664 (2026-06-09T22:09:54Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi-BerbagiSerupa (CC BY-SA). Gambar pada artikel ini bersumber dari Wikimedia Commons </ins>dan <ins style="font-weight: bold; text-decoration: none;">mengikuti ketentuan lisensi masing-masing berkas. Mohon gunakan konten dan media secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.</ins></div></td></tr>
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<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;">Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Pasta+nuklir&oldid=29331664 Wikipedia bahasa Indonesia], revisi 29331664 (2026</del>-<del style="font-weight: bold; text-decoration: none;">06</del>-<del style="font-weight: bold; text-decoration: none;">09T22:09:54Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi</del>-<del style="font-weight: bold; text-decoration: none;">BerbagiSerupa (CC BY</del>-<del style="font-weight: bold; text-decoration: none;">SA). Mohon gunakan konten ini secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.</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><ins style="font-weight: bold; text-decoration: none;"><!</ins>-- <ins style="font-weight: bold; text-decoration: none;">WIKI_UNISSULA_PRESENTATION_V4 </ins>--<ins style="font-weight: bold; text-decoration: none;">></ins></div></td></tr>
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Maintenance script: Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 29331664; atribusi sumber disertakan.
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<p>Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 29331664; atribusi sumber disertakan.</p>
<p><b>Halaman baru</b></p><div>Dalam bidang [[astrofisika]] dan [[fisika nuklir]], '''pasta nuklir''' adalah jenis [[materi degenerat]] teoretis yang diduga terbentuk di dalam kerak [[bintang neutron]]. Jika keberadaannya benar, pasta nuklir diyakini sebagai material terkuat di alam semesta.<br />
<br />
Di antara permukaan bintang neutron dan [[plasma kuark–gluon]] di intinya, pada kerapatan materi sekitar 10<sup>14</sup>&nbsp;g/cm<sup>3</sup>, [[gaya nuklir]] dan [[tolakan Coulomb]] memiliki besaran yang sebanding. Persaingan antara kedua gaya ini memunculkan berbagai struktur kompleks yang tersusun atas [[neutron]] dan [[proton]].<br />
<br />
Para astrofisikawan menamai struktur-struktur ini sebagai ''pasta nuklir'' karena bentuk geometrinya menyerupai berbagai jenis [[pasta]] Italia, seperti lembaran, tabung, atau spiral.<br />
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==Referensi==<br />
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== Sumber dan atribusi ==<br />
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Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Pasta+nuklir&oldid=29331664 Wikipedia bahasa Indonesia], revisi 29331664 (2026-06-09T22:09:54Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi-BerbagiSerupa (CC BY-SA). Mohon gunakan konten ini secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.</div>
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