Neutrino-pair bremsstrahlung from nucleon-nucleon scattering

Li, Yi; Liou, M. K.; Schreiber, W. M.; Gibson, B. F.

doi:10.1103/PhysRevC.92.015504

Title: Neutrino-pair bremsstrahlung from nucleon-nucleon scattering

Journal Article · Wed Jul 22 00:00:00 EDT 2015 · Physical Review C, Nuclear Physics

DOI:https://doi.org/10.1103/PhysRevC.92.015504· OSTI ID:1239534

Li, Yi ^[1]; Liou, M. K. ^[2]; Schreiber, W. M. ^[3]; Gibson, B. F. ^[4]

Guangxi University, Guangxi (China). College of Physics and Technology
City Univ. (CUNY), NY (United States).
City Univ. (CUNY), NY (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

Background: Neutrino-pair bremsstrahlung processes from nucleon-nucleon scattering ΝΝνν¯ (nnvv¯, ppvv¯, and npvv¯) have recently attracted attention in studies of neutrino emission in neutron stars, because of the implications for the neutron star cooling. The calculated ΝΝνν¯ emissivities within the neutron star environment are relatively insensitive to the two-nucleon dynamical model used in the calculations, but differ significantly from those obtained using an OPE model. Purpose: To investigate the free ΝΝνν¯ cross sections using a realistic nucleon-nucleon scattering amplitude, comparing the relative sizes of the cross sections for the three processes nnvv¯, ppvv¯, and npvv¯.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: AC52-06NA25396; DEAC52-06NA25396

OSTI ID:: 1239534

Alternate ID(s):: OSTI ID: 1201003

Report Number(s):: LA-UR-15-24792; PRVCAN

Journal Information:: Physical Review C, Nuclear Physics, Vol. 92, Issue 1; ISSN 0556-2813

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 3 works

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