The impact of different neutrino transport methods on multidimensional core-collapse supernova simulations

Pan, Kuo-Chuan; Mattes, Carlos; O’Connor, Evan P.; Couch, Sean M.; Perego, Albino; Arcones, Almudena

doi:10.1088/1361-6471/aaed51

Title: The impact of different neutrino transport methods on multidimensional core-collapse supernova simulations

Journal Article · 21 November 2018 · Journal of Physics. G, Nuclear and Particle Physics

DOI: https://doi.org/10.1088/1361-6471/aaed51 · OSTI ID:1612344

^[1]; Mattes, Carlos ^[2];

^[3]; Couch, Sean M. ^[4]; Perego, Albino ^[5]; Arcones, Almudena ^[6]

Michigan State Univ., East Lansing, MI (United States); National Tsing Hua Univ., Hsinchu (Taiwan); DOE/OSTI
Darmstadt Univ. of Technology (Germany)
Stockholm Univ. (Sweden)
Michigan State Univ., East Lansing, MI (United States)
Istituto Nazionale di Fisica Nucleare (INFN), Parma (Italy); Univ. degli Studi di Milano-Bicocca (Italy)
Darmstadt Univ. of Technology (Germany); GSI-Darmstadt (Germany)

Neutrinos play a crucial role in the core-collapse supernova (CCSN) explosion mechanism. The requirement of accurately calculating the transport of neutrinos makes simulations of the CCSN mechanism extremely challenging and computationally expensive. Historically, this stiff challenge has been met by making approximations to the full transport equation. In this work, we compare CCSN simulations in one- and two-dimensions with three approximate neutrino transport schemes, each implemented in the FLASH simulation framework. We compare a two-moment M1 scheme with an analytic closure (M1), the isotropic diffusion source approximation (IDSA), and the advanced spectral leakage method. We identify and discuss the advantages and disadvantages of each scheme. For each approximate transport scheme, we use identical grid setups, hydrodynamics, and gravity solvers to investigate the transport effects on supernova shock dynamics and neutrino quantities. We find that the transport scheme has a small effect on the evolution of protoneutron star (PNS) radius, PNS mass, and the mass accretion rate. The neutrino luminosities, mean energies, and shock radii have a ~10%–20% quantitative difference but the overall qualitative trends are fairly consistent between all three approximations. We find larger differences in the gain region properties, including the gain region mass and the net heating rate in the gain region, as well as the strength of PNS convection in the core. We investigate the progenitor, nuclear equation of state, and stochastic perturbation dependence of our simulations and find similar magnitudes of impact on key quantities. We also compare the computational expense of the various approximations.

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Research Organization:: Michigan State University, East Lansing, MI (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0015904; SC0017955

OSTI ID:: 1612344

Journal Information:: Journal of Physics. G, Nuclear and Particle Physics, Journal Name: Journal of Physics. G, Nuclear and Particle Physics Journal Issue: 1 Vol. 46; ISSN 0954-3899

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae O'Connor, Evan; Couch, Sean arXiv https://doi.org/10.48550/arxiv.1807.07579	text	January 2018
An Adaptive Grid, Implicit Code for Spherically Symmetric, General Relativistic Hydrodynamics in Comoving Coordinates Liebendoerfer, Matthias; Rosswog, Stephan; Thielemann, Friedrich-Karl arXiv https://doi.org/10.48550/arxiv.astro-ph/0106539	text	January 2001
High Resolution Calculations of Merging Neutron Stars II: Neutrino Emission Rosswog, S.; Liebendoerfer, M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0302301	text	January 2003
Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star Buras, R.; Rampp, M.; Janka, H. -Th. arXiv https://doi.org/10.48550/arxiv.astro-ph/0507135	text	January 2005
Supernova Neutrino Opacity from Nucleon-Nucleon Bremsstrahlung and Related Processes Hannestad, Steen; Raffelt, Georg arXiv https://doi.org/10.48550/arxiv.astro-ph/9711132	text	January 1997
An Advanced Leakage Scheme for Neutrino Treatment in Astrophysical Simulations Perego, A.; Cabezón, R. M.; Käppeli, R. IOP Publishing https://doi.org/10.5451/unibas-ep53879	text	January 2016
A New Gravitational-wave Signature from Standing Accretion Shock Instability in Supernovae Kuroda, Takami; Kotake, Kei; Takiwaki, Tomoya American Astronomical Society https://doi.org/10.5451/unibas-ep53880	text	January 2016

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Searching for fast neutrino flavor conversion modes in core-collapse supernova simulations Abbar, Sajad Journal of Cosmology and Astroparticle Physics, Vol. 2020, Issue 05 https://doi.org/10.1088/1475-7516/2020/05/027	journal	May 2020
A multidimensional implementation of the Advanced Spectral neutrino Leakage scheme Gizzi, D.; O’Connor, E.; Rosswog, S. Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 3 https://doi.org/10.1093/mnras/stz2911	journal	October 2019
A multi-dimensional implementation of the Advanced Spectral neutrino Leakage scheme Gizzi, Davide; O'Connor, Evan; Rosswog, Stephan arXiv https://doi.org/10.48550/arxiv.1906.11494	text	January 2019

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