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Chiral effective field theory calculations of neutrino processes in dense matter
Phys. Rev. C 80, 032802(R) – Published 23 September, 2009
DOI: https://doi.org/10.1103/PhysRevC.80.032802
Abstract
We calculate neutrino processes involving two nucleons at subnuclear densities using chiral effective field theory. Shorter range noncentral forces reduce the neutrino rates significantly compared with the one-pion exchange approximation currently used in supernova simulations. For densities , we find that neutrino rates are well constrained by nuclear interactions and nucleon-nucleon scattering data. As an application, we calculate the mean-square energy transfer in scattering of a neutrino from nucleons and find that collision processes and spin-dependent mean-field effects dominate over the energy transfer due to nucleon recoil.
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