Effects of the neutrino electromagnetic form factors on the neutrino and antineutrino mean free paths in dense matter
arXiv:nucl-th/0608080 · doi:10.1016/j.nuclphysa.2006.10.034
Abstract
We have studied the effects of the nucleon weak magnetism and the neutrino electromagnetic properties on the neutrino and antineutrino mean free paths for all types of neutrinos. In the calculation, we consider matters with and without neutrino trapping as the target. We have found that the difference between the two mean free paths depends not only on the neutrino energy, but also on the matter density as well as matter constituents. Compared to the nucleon weak magnetism, the neutrino electromagnetic properties are found to have negligible effects on this difference.
arXiv comment6 pages, 4 figures, Talk given at the 5th International Conference on Perspectives in Hadronic Physics, Trieste, Italy, 22-26 May 2006
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Cited by in corpus (5)
- Impact of medium modification of the nucleon weak and electromagnetic form factors on the neutrino mean free path in dense matter
- Neutrino propagation in the neutron star with uncertainties from nuclear, hadron, and particle physics
- Antineutrino Opacity in Neutron Stars in the Models Constrained by Recent Terrestrial Experiments and Astrophysical Observations
- From Pauli Principle to Hypernucleus, Neutron Star, and Econophysics
- Neutrino mean free path in neutron stars in the presence of hyperons