Diffusion coefficient of neutrinos in a presupernova star

Details Diffusion coefficient of neutrinos in a presupernova star Diffusion coefficient of neutrinos in a presupernova star

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205..343b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 2, p. 343-353.

Astronomy and Astrophysics

Astrophysics

Chapman-Enskog Theory, Diffusion Coefficient, Elementary Particle Interactions, Neutrinos, Supernovae, Electron Scattering, Gravitational Collapse, Mean Free Path

Scientific paper

The diffusion coefficient of neutrinos in the trapping regime in a presupernova star, where the scattering of neutrinos by nuclei is the dominant effect, is calculated within the framework of relativistic kinetic theory in the lowest order Chapman-Enskog approximation. The screening of the nuclei by ion-ion and electron-electron correlations is also taken into account.

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