Generalized Kompaneets formalism for inelastic neutrino-nucleon scattering in supernova simulations

Tianshu Wang, Adam Burrows

Research output: Contribution to journalArticlepeer-review

5 Scopus citations


Based on the Kompaneets approximation, we develop a robust methodology to calculate spectral redistribution via inelastic neutrino-nucleon scattering in the context of core-collapse supernova simulations. The resulting equations conserve lepton number to machine precision and scale linearly, not quadratically, with number of energy groups. The formalism also provides an elegant means to derive the rate of energy transfer to matter which, as it must, automatically goes to zero when the neutrino radiation field is in thermal equilibrium. Furthermore, we derive the next higher order in µ/mc2 correction to the neutrino Kompaneets equation. Unlike other Kompaneets schema, ours also generalizes to the case of anisotropic angular distributions, while retaining the conservative form that is a hallmark of the classical Kompaneets equation. Our formalism enables immediate incorporation into supernova codes that follow the spectral angular moments of the neutrino radiation fields.

Original languageEnglish (US)
Article number023017
JournalPhysical Review D
Issue number2
StatePublished - Jul 15 2020

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics


Dive into the research topics of 'Generalized Kompaneets formalism for inelastic neutrino-nucleon scattering in supernova simulations'. Together they form a unique fingerprint.

Cite this