From supernovae to neutron stars

Suwa Yudai

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From supernovae to neutron stars

机译：从超新星到中子星

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Gravitationalcollapse,bounce,andexplosionofanironcoreofan11.2a€‰Ma??stararesimulatedbytwo-dimensionalneutrino-radiationhydrodynamiccode.Theexplosionisdrivenbytheneutrinoheatingaidedbymulti-dimensionalhydrodynamiceffectssuchasconvection.Followingtheexplosionphase,wecontinuethesimulationfocusingonthethermalevolutionoftheprotoneutronstaruptoa??a€‰70??swhenthecrustoftheneutronstarisformed,usingone-dimensionalsimulation.Wefindthatthecrustformsatahigh-densityregion(????a????1014a€‰g??cma?’3)anditproceedsfrominsidetooutside.Thisisthefirstself-consistentsimulationthatsuccessfullyfollowsfromthecollapsephasetotheprotoneutronstarcoolingphasebasedonmulti-dimensionalhydrodynamicsimulation.

机译：Gravitationalcollapse，反弹，andexplosionofanironcoreofan11.2a€‰马?? stararesimulatedbytwo-dimensionalneutrino-radiationhydrodynamiccode.Theexplosionisdrivenbytheneutrinoheatingaidedbymulti-dimensionalhydrodynamiceffectssuchasconvection.Followingtheexplosionphase，wecontinuethesimulationfocusingonthethermalevolutionoftheprotoneutronstaruptoa ??一个€‰70 ?? swhenthecrustoftheneutronstarisformed，usingone-dimensionalsimulation.Wefindthatthecrustformsatahigh-densityregion（????的ΔΣ “ 1014a g g·cma”（3）并从内到外进行。这是第一个自洽的模拟，它成功地遵循了基于多维流体动力学模拟从塌陷阶段到质子核星冷却阶段的崩溃阶段。

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《PASJ: Publications of the Astronomical Society of Japan》 |2014年第2期|共页
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Suwa Yudai;
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1. Simulating Pasta Phases by Molecular Dynamics and Cold AtomsFormation in Supernovae and Superfluid Neutrons in Neutron Stars [J] . Gentaro WATANABE Progress of Theoretical Physics. Supplement . 2010,第186期

机译：通过分子动力学和冷原子在中子星中超新星和超流体中子中模拟面相的过程
2. Deeply bound dibaryon is incompatible with neutron stars and supernovae [J] . Samuel D. McDermott, Sanjay Reddy, Srimoyee Sen Physical review, D . 2019,第3期

机译：深度结合的重子与中子星和超新星不相容
3. Akmal-Pandharipande-Ravenhall equation of state for simulations of supernovae, neutron stars, and binary mergers [J] . Schneider A. S., Constantinou C., Muccioli B., Physical review, C . 2019,第2期

机译：Akmal-Pandharipande-Ravenhall Supernovae，中子恒星和二元兼并模拟的状态
4. Equations of State for Neutron Stars and Core-collapse Supernovae [C] . Micaela Oertel, Constan?a Providência International Symposium on Origin of Matter and Evolution of Galaxies . 2018

机译：中子恒星和核心塌陷超新星的方程
5. Topics in the Physics of Supernovae and Neutron Stars. [D] . Abbar, Sajad. 2016

机译：超新星和中子星物理中的主题。
6. Bridging the gap: from massive stars to supernovae [O] . Justyn R. Maund, Paul A. Crowther, Hans-Thomas Janka, -1

机译：缩小差距：从大质量恒星到超新星
7. Simulating pasta phases by molecular dynamics and cold atoms --- Formation in supernovae and superfluid neutrons in neutron stars [O] . Watanabe, Gentaro 2011

机译：通过分子动力学和冷原子模拟面食阶段--- 中子星中超新星和超流体中子的形成
8. Neutron Star Formation in Theoretical Supernovae. Low Mass Stars and White Dwarfs [R] . Nomoto, K. 1986

机译：理论超新星中的中子星形成。低质量恒星和白矮星

From supernovae to neutron stars

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