A new monte carlo method for time-dependent neutrino radiation transport

Ernazar Abdikamalov, Adam Burrows, Christian D. Ott, Frank Löffler, Evan O'Connor, Joshua C. Dolence, Erik Schnetter

Research output: Contribution to journalArticle

46 Citations (Scopus)

Abstract

Monte Carlo approaches to radiation transport have several attractive properties such as simplicity of implementation, high accuracy, and good parallel scaling. Moreover, Monte Carlo methods can handle complicated geometries and are relatively easy to extend to multiple spatial dimensions, which makes them potentially interesting in modeling complex multi-dimensional astrophysical phenomena such as core-collapse supernovae. The aim of this paper is to explore Monte Carlo methods for modeling neutrino transport in core-collapse supernovae. We generalize the Implicit Monte Carlo photon transport scheme of Fleck & Cummings and gray discrete-diffusion scheme of Densmore et al. to energy-, time-, and velocity-dependent neutrino transport. Using our 1D spherically-symmetric implementation, we show that, similar to the photon transport case, the implicit scheme enables significantly larger timesteps compared with explicit time discretization, without sacrificing accuracy, while the discrete-diffusion method leads to significant speed-ups at high optical depth. Our results suggest that a combination of spectral, velocity-dependent, Implicit Monte Carlo and discrete-diffusion Monte Carlo methods represents a robust approach for use in neutrino transport calculations in core-collapse supernovae. Our velocity-dependent scheme can easily be adapted to photon transport.

Original languageEnglish
Article number111
JournalAstrophysical Journal
Volume755
Issue number2
DOIs
Publication statusPublished - Aug 20 2012
Externally publishedYes

Fingerprint

radiation transport
Monte Carlo method
neutrinos
supernovae
photons
optical thickness
optical depth
modeling
astrophysics
scaling
geometry
radiation
method
energy

Keywords

  • hydrodynamics
  • neutrinos
  • radiative transfer
  • stars: evolution
  • stars: neutron
  • supernovae: general

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Abdikamalov, E., Burrows, A., Ott, C. D., Löffler, F., O'Connor, E., Dolence, J. C., & Schnetter, E. (2012). A new monte carlo method for time-dependent neutrino radiation transport. Astrophysical Journal, 755(2), [111]. https://doi.org/10.1088/0004-637X/755/2/111

A new monte carlo method for time-dependent neutrino radiation transport. / Abdikamalov, Ernazar; Burrows, Adam; Ott, Christian D.; Löffler, Frank; O'Connor, Evan; Dolence, Joshua C.; Schnetter, Erik.

In: Astrophysical Journal, Vol. 755, No. 2, 111, 20.08.2012.

Research output: Contribution to journalArticle

Abdikamalov, E, Burrows, A, Ott, CD, Löffler, F, O'Connor, E, Dolence, JC & Schnetter, E 2012, 'A new monte carlo method for time-dependent neutrino radiation transport', Astrophysical Journal, vol. 755, no. 2, 111. https://doi.org/10.1088/0004-637X/755/2/111
Abdikamalov, Ernazar ; Burrows, Adam ; Ott, Christian D. ; Löffler, Frank ; O'Connor, Evan ; Dolence, Joshua C. ; Schnetter, Erik. / A new monte carlo method for time-dependent neutrino radiation transport. In: Astrophysical Journal. 2012 ; Vol. 755, No. 2.
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