On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code

Harada, Akira; Nagakura, Hiroki; Iwakami, Wakana; Okawa, Hirotada; Furusawa, Shun; Matsufuru, Hideo; Sumiyoshi, Kohsuke; Yamada, Shoichi

doi:10.3847/1538-4357/ab0203

On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code

Journal Article · Sun Feb 24 23:00:00 EST 2019 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/ab0203· OSTI ID:1612911

Harada, Akira ^[1]; ^[2]; ^[3]; Okawa, Hirotada ^[3]; Furusawa, Shun ^[4]; Matsufuru, Hideo ^[5]; ^[6]; ^[7]

Univ. of Tokyo (Japan); DOE/OSTI
Princeton Univ., NJ (United States); California Inst. of Technology (CalTech), Pasadena, CA (United States)
Kyoto Univ. (Japan); Waseda Univ., Tokyo (Japan)
RIKEN, Saitama (Japan). Interdisciplinary Theoretical and Mathematical Sciences Program (iTHEMS)
High Energy Accelerator Research Organization, Ibaraki (Japan)
Numazu College of Technology (Japan)
Waseda Univ., Tokyo (Japan)

With the Boltzmann-radiation-hydrodynamics code, which we have developed to solve numerically the Boltzmann equations for neutrino transfer, the Newtonian hydrodynamics equations, and the Newtonian self-gravity simultaneously and consistently, in this work we simulate the collapse of a rotating core of the progenitor with a zero-age- main-sequence mass of 11.2 M_⊙ and a shellular rotation of $$1\,\mathrm{rad}\,{{\rm{s}}}^{-1}$$ at the center. We pay particular attention in this paper to the neutrino distribution in phase space, which is affected by the rotation. By solving the Boltzmann equations directly, we can assess the rotation-induced distortion of the angular distribution in momentum space, which gives rise to the rotational component of the neutrino flux. We compare the Eddington tensors calculated both from the raw data and from the M1-closure approximation. We demonstrate that the Eddington tensor is determined by complicated interplays of the fluid velocity and the neutrino interactions and that the M1-closure, which assumes that the Eddington factor is determined by the flux factor, fails to fully capture this aspect, especially in the vicinity of the shock. We find that the error in the Eddington factor reaches ~20% in our simulation. This is due not to the resolution but to the different dependence of the Eddington and flux factors on the angular profile of the neutrino distribution function, and hence modification to the closure relation is needed.

View Accepted Manuscript (DOE)

Research Organization:: Univ. of California, Oakland, CA (United States)

Sponsoring Organization:: Ministry of Education, Culture, Sports, Science and Technology (MEXT); Japan Society for the Promotion of Science (JSPS); National Science Foundation (NSF); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR) (SC-21). Scientific Discovery through Advanced Computing (SciDAC)

Grant/Contract Number:: SC0018297

OSTI ID:: 1612911

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 872; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Electron capture rates on nuclei and implications for stellar core collapse Langanke, K.; Martinez-Pinedo, G.; Sampaio, J. M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0302459	text	January 2003
A simple parameterization of the consequences of deleptonization for simulations of stellar core collapse Liebendoerfer, M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0504072	text	January 2005
Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state Sumiyoshi, K.; Yamada, S.; Suzuki, H. arXiv https://doi.org/10.48550/arxiv.astro-ph/0506620	text	January 2005
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
Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae Kotake, Kei; Sato, Katsuhiko; Takahashi, Keitaro arXiv https://doi.org/10.48550/arxiv.astro-ph/0509456	text	January 2005
GW170817: Observation of gravitational waves from a binary neutron star inspiral Abbott, B. P.; Abbott, R.; Abbott, T. D. American Physical Society https://doi.org/10.5167/uzh-147231	text	January 2017
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
Global comparison of core-collapse supernova simulations in spherical symmetry O'Connor, Evan; Bollig, Robert; Burrows, Adam IOP Publishing https://doi.org/10.5451/unibas-ep69143	text	January 2018

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Fast neutrino flavor conversion modes in multidimensional core-collapse supernova models: The role of the asymmetric neutrino distributions Abbar, Sajad; Duan, Huaiyu; Sumiyoshi, Kohsuke Physical Review D, Vol. 101, Issue 4 https://doi.org/10.1103/physrevd.101.043016	journal	February 2020
Long-term simulations of multi-dimensional core-collapse supernovae: Implications for neutron star kicks Nakamura, Ko; Takiwaki, Tomoya; Kotake, Kei Publications of the Astronomical Society of Japan, Vol. 71, Issue 5 https://doi.org/10.1093/pasj/psz080	journal	August 2019
Multimessenger asteroseismology of core-collapse supernovae Westernacher-Schneider, John Ryan; O’Connor, Evan; O’Sullivan, Erin Physical Review D, Vol. 100, Issue 12 https://doi.org/10.1103/physrevd.100.123009	journal	December 2019
Three-dimensional Boltzmann-hydro Code for Core-collapse in Massive Stars. III. A New Method for Momentum Feedback from Neutrino to Matter Nagakura, Hiroki; Sumiyoshi, Kohsuke; Yamada, Shoichi The Astrophysical Journal, Vol. 878, Issue 2 https://doi.org/10.3847/1538-4357/ab2189	journal	June 2019
One-, Two-, and Three-dimensional Simulations of Oxygen-shell Burning Just before the Core Collapse of Massive Stars Yoshida, Takashi; Takiwaki, Tomoya; Kotake, Kei The Astrophysical Journal, Vol. 881, Issue 1 https://doi.org/10.3847/1538-4357/ab2b9d	journal	August 2019
Fast-pairwise Collective Neutrino Oscillations Associated with Asymmetric Neutrino Emissions in Core-collapse Supernovae Nagakura, Hiroki; Morinaga, Taiki; Kato, Chinami The Astrophysical Journal, Vol. 886, Issue 2 https://doi.org/10.3847/1538-4357/ab4cf2	journal	November 2019
One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars Yoshida, Takashi; Takiwaki, Tomoya; Kotake, Kei arXiv https://doi.org/10.48550/arxiv.1903.07811	text	January 2019
Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks Nakamura, Ko; Takiwaki, Tomoya; Kotake, Kei arXiv https://doi.org/10.48550/arxiv.1904.08088	text	January 2019

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