Essential Ingredients in Core-collapse Supernovae
Abstract
Marking the inevitable death of a massive star, and the birth of a neutron star or black hole, core-collapse supernovae bring together physics at a wide range in spatial scales, from kilometer-sized hydrodynamic motions (eventually growing to gigameter scale) down to femtometer scale nuclear reactions. Carrying 10$$^{44}$$ joules of kinetic energy and a rich-mix of newly synthesized atomic nuclei, core-collapse supernovae are the preeminent foundries of the nuclear species which make up ourselves and our solar system. We will discuss our emerging understanding of the convectively unstable, neutrino-driven explosion mechanism, based on increasingly realistic neutrino-radiation hydrodynamic simulations that include progressively better nuclear and particle physics. Recent multi-dimensional models with spectral neutrino transport from several research groups, which slowly develop successful explosions for a range of progenitors, have motivated changes in our understanding of the neutrino reheating mechanism. In a similar fashion, improvements in nuclear physics, most notably explorations of weak interactions on nuclei and the nuclear equation of state, continue to refine our understanding of how supernovae explode. Recent progress on both the macroscopic and microscopic effects that affect core-collapse supernovae are discussed.
- Authors:
-
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); Univ. of Tennessee, Knoxville, TN (United States)
- Univ. of Tennessee, Knoxville, TN (United States)
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); Univ. of Tennessee, Knoxville, TN (United States)
- Univ. of Tennessee, Knoxville, TN (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
- Florida Atlantic Univ., Boca Raton, FL (United States)
- North Carolina State Univ., Raleigh, NC (United States)
- Publication Date:
- Research Org.:
- Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1195798
- Grant/Contract Number:
- AC05-00OR22725
- Resource Type:
- Accepted Manuscript
- Journal Name:
- AIP Advances
- Additional Journal Information:
- Journal Volume: 4; Journal Issue: 4; Journal ID: ISSN 2158-3226
- Publisher:
- American Institute of Physics (AIP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Hix, William Raphael, Lentz, E. J., Endeve, Eirik, Baird, Mark L., Chertkow, Merek A., Harris, James A., Messer, Bronson, Mezzacappa, Anthony, Bruenn, S. W., and Blondin, J. M. Essential Ingredients in Core-collapse Supernovae. United States: N. p., 2014.
Web. doi:10.1063/1.4870009.
Hix, William Raphael, Lentz, E. J., Endeve, Eirik, Baird, Mark L., Chertkow, Merek A., Harris, James A., Messer, Bronson, Mezzacappa, Anthony, Bruenn, S. W., & Blondin, J. M. Essential Ingredients in Core-collapse Supernovae. United States. https://doi.org/10.1063/1.4870009
Hix, William Raphael, Lentz, E. J., Endeve, Eirik, Baird, Mark L., Chertkow, Merek A., Harris, James A., Messer, Bronson, Mezzacappa, Anthony, Bruenn, S. W., and Blondin, J. M. Thu .
"Essential Ingredients in Core-collapse Supernovae". United States. https://doi.org/10.1063/1.4870009. https://www.osti.gov/servlets/purl/1195798.
@article{osti_1195798,
title = {Essential Ingredients in Core-collapse Supernovae},
author = {Hix, William Raphael and Lentz, E. J. and Endeve, Eirik and Baird, Mark L. and Chertkow, Merek A. and Harris, James A. and Messer, Bronson and Mezzacappa, Anthony and Bruenn, S. W. and Blondin, J. M.},
abstractNote = {Marking the inevitable death of a massive star, and the birth of a neutron star or black hole, core-collapse supernovae bring together physics at a wide range in spatial scales, from kilometer-sized hydrodynamic motions (eventually growing to gigameter scale) down to femtometer scale nuclear reactions. Carrying 10$^{44}$ joules of kinetic energy and a rich-mix of newly synthesized atomic nuclei, core-collapse supernovae are the preeminent foundries of the nuclear species which make up ourselves and our solar system. We will discuss our emerging understanding of the convectively unstable, neutrino-driven explosion mechanism, based on increasingly realistic neutrino-radiation hydrodynamic simulations that include progressively better nuclear and particle physics. Recent multi-dimensional models with spectral neutrino transport from several research groups, which slowly develop successful explosions for a range of progenitors, have motivated changes in our understanding of the neutrino reheating mechanism. In a similar fashion, improvements in nuclear physics, most notably explorations of weak interactions on nuclei and the nuclear equation of state, continue to refine our understanding of how supernovae explode. Recent progress on both the macroscopic and microscopic effects that affect core-collapse supernovae are discussed.},
doi = {10.1063/1.4870009},
journal = {AIP Advances},
number = 4,
volume = 4,
place = {United States},
year = {Thu Mar 27 00:00:00 EDT 2014},
month = {Thu Mar 27 00:00:00 EDT 2014}
}
Web of Science
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