The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M ⊙
Abstract
We present a first study of the progenitor star dependence of the three-dimensional (3D) neutrino mechanism of core-collapse supernovae. We employ full 3D general-relativistic multi-group neutrino radiation-hydrodynamics and simulate the postbounce evolutions of progenitors with zero-age main sequence masses of 12, 15, 20, 27, and 40 M⊙. All progenitors, with the exception of the 12 M ⊙ star, experience shock runaway by the end of their simulations. In most cases, a strongly asymmetric explosion will result. We demonstrate three qualitatively distinct evolutions that imply a complex dependence of explosion dynamics on progenitor density structure, neutrino heating, and 3D flow. (1) Progenitors with massive cores, shallow density profiles, and high post-core-bounce accretion rates experience very strong neutrino heating and neutrino-driven turbulent convection, leading to early shock runaway. Accretion continues at a high rate, likely leading to black hole formation. (2) Intermediate progenitors experience neutrino-driven, turbulence-aided explosions triggered by the arrival of density discontinuities at the shock. These occur typically at the silicon/silicon–oxygen shell boundary. (3) Progenitors with small cores and density profiles without strong discontinuities experience shock recession and develop the 3D standing-accretion shock instability (SASI). Shock runaway ensues late, once declining accretion rate, SASI, and neutrino-driven convection create favorable conditions.more »
- Authors:
-
- Kyoto Univ. (Japan); California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Michigan State Univ., East Lansing, MI (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Kyoto Univ. (Japan)
- Univ. of Illinois, Urbana-Champaign, IL (United States)
- Perimeter Inst. for Theoretical Physics, Waterloo, ON (Canada); Univ. of Guelph, ON (Canada); Louisiana State Univ., Baton Rouge, LA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Basic Energy Sciences (BES). Scientific User Facilities Division
- OSTI Identifier:
- 1524172
- Grant/Contract Number:
- AC02-05CH11231; CAREER PHY-1151197; PHY-1404569; OAC-1550514; AST-1333520
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal. Letters (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal. Letters (Online); Journal Volume: 855; Journal Issue: 1; Journal ID: ISSN 2041-8213
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; neutrinos; stars: black holes; stars: neutron; supernovae: general
Citation Formats
Ott, Christian D., Roberts, Luke F., da Silva Schneider, André, Fedrow, Joseph M., Haas, Roland, and Schnetter, Erik. The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M ⊙. United States: N. p., 2018.
Web. doi:10.3847/2041-8213/aaa967.
Ott, Christian D., Roberts, Luke F., da Silva Schneider, André, Fedrow, Joseph M., Haas, Roland, & Schnetter, Erik. The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M ⊙. United States. https://doi.org/10.3847/2041-8213/aaa967
Ott, Christian D., Roberts, Luke F., da Silva Schneider, André, Fedrow, Joseph M., Haas, Roland, and Schnetter, Erik. Mon .
"The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M ⊙". United States. https://doi.org/10.3847/2041-8213/aaa967. https://www.osti.gov/servlets/purl/1524172.
@article{osti_1524172,
title = {The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M ⊙},
author = {Ott, Christian D. and Roberts, Luke F. and da Silva Schneider, André and Fedrow, Joseph M. and Haas, Roland and Schnetter, Erik},
abstractNote = {We present a first study of the progenitor star dependence of the three-dimensional (3D) neutrino mechanism of core-collapse supernovae. We employ full 3D general-relativistic multi-group neutrino radiation-hydrodynamics and simulate the postbounce evolutions of progenitors with zero-age main sequence masses of 12, 15, 20, 27, and 40 M⊙. All progenitors, with the exception of the 12 M ⊙ star, experience shock runaway by the end of their simulations. In most cases, a strongly asymmetric explosion will result. We demonstrate three qualitatively distinct evolutions that imply a complex dependence of explosion dynamics on progenitor density structure, neutrino heating, and 3D flow. (1) Progenitors with massive cores, shallow density profiles, and high post-core-bounce accretion rates experience very strong neutrino heating and neutrino-driven turbulent convection, leading to early shock runaway. Accretion continues at a high rate, likely leading to black hole formation. (2) Intermediate progenitors experience neutrino-driven, turbulence-aided explosions triggered by the arrival of density discontinuities at the shock. These occur typically at the silicon/silicon–oxygen shell boundary. (3) Progenitors with small cores and density profiles without strong discontinuities experience shock recession and develop the 3D standing-accretion shock instability (SASI). Shock runaway ensues late, once declining accretion rate, SASI, and neutrino-driven convection create favorable conditions. These differences in explosion times and dynamics conclude in a non-monotonic relationship between progenitor and compact remnant mass.},
doi = {10.3847/2041-8213/aaa967},
journal = {The Astrophysical Journal. Letters (Online)},
number = 1,
volume = 855,
place = {United States},
year = {2018},
month = {2}
}
Web of Science
Figures / Tables:

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Figures / Tables found in this record: