On Neutrino Emission From Dense Matter Containing Meson Condensates
arXiv:nucl-th/9502004 · doi:10.1103/PhysRevD.52.3739
Abstract
We consider the rate at which energy is emitted by neutrinos from the dense interior of neutron stars containing a Bose condensate of pions or kaons. The rates obtained are larger, by a factor of 2, than those found earlier, and are consistent with those found for the direct Urca processes.
RevTeX, 10 pages
Cited by in corpus (10)
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- Kaon Condensates, Nuclear Symmetry Energy and Cooling of Neutron Stars
- Rapid cooling of magnetized neutron stars
- Fast Cooling of Neutron Stars: Superfluidity vs. Heating and Accreted Envelope
- Nonequilibrium Weak Processes in Kaon Condensation I --- Reaction rate for the thermal kaon process ---
- Constraining the Right Handed Interactions from Pion Condensate Matter