Conservative formulations of general relativistic kinetic theory

Christian Y. Cardall, Anthony Mezzacappa

Research output: Contribution to journalArticlepeer-review

36 Scopus citations

Abstract

Experience with core-collapse supernova simulations shows that accurate accounting of total particle number and 4-momentum can be a challenge for computational radiative transfer. This accurate accounting would be facilitated by the use of particle number and 4-momentum transport equations that allow transparent conversion between volume and surface integrals in both configuration and momentum space. Such conservative formulations of general relativistic kinetic theory in multiple spatial dimensions are presented in this paper, and their relevance to core-collapse supernova simulations is described.

Original languageEnglish
Article number023006
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume68
Issue number2
DOIs
StatePublished - 2003

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