The potential role of spatial dimension in the neutrino-driving mechanism of core-collapse supernova explosions

被引:2
作者
Burrows, Adam [1 ]
Nordhaus, Jason [1 ]
Almgren, Ann [2 ]
Bell, John [2 ]
机构
[1] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[2] Univ Calif Berkeley, Lawrence Berkeley Lab, Computat Res Div, Berkeley, CA 94720 USA
关键词
Hydrodynamics; supernovae; General; stars; Interiors; neutrinos; HYDRODYNAMICS;
D O I
10.1016/j.cpc.2010.10.014
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
We have hydrodynamically explored the dependence on spatial dimension of the viability of the neutrino heating mechanism of core-collapse supernova explosions and find that the tendency to explode is a monotonically increasing function of dimension. Moreover, we find that the delay to explosion for a given neutrino luminosity is always shorter in 3D than 2D, sometimes by many hundreds of milliseconds. The magnitude of this dimensional effect is much larger than the purported magnitude of a variety of other effects sometimes invoked to bridge the gap between the current ambiguous and uncertain theoretical situation and the fact of robust supernova explosions in Nature. Our finding, facilitated by access to state-of-the-art codes and large computers, may be an important step towards unraveling one of the most problematic puzzles in stellar astrophysics. (C) 2010 Elsevier By. All rights reserved.
引用
收藏
页码:1764 / 1766
页数:3
相关论文
共 50 条
[41]   Simulations of Core-collapse Supernovae in Spatial Axisymmetry with Full Boltzmann Neutrino Transport [J].
Nagakura, Hiroki ;
Iwakami, Wakana ;
Furusawa, Shun ;
Okawa, Hirotada ;
Harada, Akira ;
Sumiyoshi, Kohsuke ;
Yamada, Shoichi ;
Matsufuru, Hideo ;
Imakura, Akira .
ASTROPHYSICAL JOURNAL, 2018, 854 (02)
[42]   Neutrino driven explosions aided by axion cooling in multidimensional simulations of core-collapse supernovae [J].
Betranhandy, Aurore ;
O'Connor, Evan .
PHYSICAL REVIEW D, 2022, 106 (06)
[43]   TWO-DIMENSIONAL CORE-COLLAPSE SUPERNOVA SIMULATIONS WITH THE ISOTROPIC DIFFUSION SOURCE APPROXIMATION FOR NEUTRINO TRANSPORT [J].
Pan, Kuo-Chuan ;
Liebendoerfer, Matthias ;
Hempel, Matthias ;
Thielemann, Friedrich-Karl .
ASTROPHYSICAL JOURNAL, 2016, 817 (01)
[44]   Learning from core-collapse supernova remnants on the explosion mechanism [J].
Soker, Noam .
NEW ASTRONOMY, 2025, 121
[45]   THREE-DIMENSIONAL HYDRODYNAMIC CORE-COLLAPSE SUPERNOVA SIMULATIONS FOR AN 11.2 M⊙ STAR WITH SPECTRAL NEUTRINO TRANSPORT [J].
Takiwaki, Tomoya ;
Kotake, Kei ;
Suwa, Yudai .
ASTROPHYSICAL JOURNAL, 2012, 749 (02)
[46]   Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare r-process Site [J].
Fischer, Tobias ;
Wu, Meng-Ru ;
Wehmeyer, Benjamin ;
Bastian, Niels-Uwe F. ;
Martinez-Pinedo, Gabriel ;
Thielemann, Friedrich-Karl .
ASTROPHYSICAL JOURNAL, 2020, 894 (01)
[47]   FAILURE OF A NEUTRINO-DRIVEN EXPLOSION AFTER CORE-COLLAPSE MAY LEAD TO A THERMONUCLEAR SUPERNOVA [J].
Kushnir, Doron ;
Katz, Boaz .
ASTROPHYSICAL JOURNAL, 2015, 811 (02)
[48]   Correlated Signatures of Gravitational-wave and Neutrino Emission in Threedimensional General-relativistic Core-collapse Supernova Simulations [J].
Kuroda, Takami ;
Kotake, Kei ;
Hayama, Kazuhiro ;
Takiwaki, Tomoya .
ASTROPHYSICAL JOURNAL, 2017, 851 (01)
[49]   Future neutrino observations of nearby pre-supernova stars before core-collapse [J].
Odrzywolek, A. ;
Misiaszek, M. ;
Kutschera, M. .
NNN06: NEXT GENERATION NUCLEON DECAY AND NEUTRINO DETECTORS 2006, 2007, 944 :109-118
[50]   Convection- and SASI-driven flows in parametrized models of core-collapse supernova explosions [J].
Endeve, E. ;
Cardall, C. Y. ;
Budiardja, R. D. ;
Mezzacappa, A. .
PHYSICA SCRIPTA, 2016, 91 (02)