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- W2140174380 abstract "We study the emission of neutrinos, resulting from the scattering of electrons off magnetic flux tubes (fluxoids) in the neutron star cores with superfluid (superconducting) pro- tons. In the absence of proton superfluidity (T Tcp), this pro- cess transforms into the well known electron synchrotron emis- sionofneutrinopairsinalocallyuniformmagneticeldB,with the neutrino energy loss rate Q proportional to B 2 T 5 . For tem- peratures T not much below Tcp, the synchrotron regime (Q / T 5 ) persists and the emissivity Q can be amplied by several ordersofmagnitudeduetotheappearanceofthefluxoidsandas- sociated enhancement of the eld within them. For lowerT, the synchrotron regime transforms into the bremsstrahlung regime (Q / T 6 ) similar to the ordinary neutrino-pair bremsstrahlung of electrons which scatter off atomic nuclei. We calculate Q numerically and represent our results through a suitable ana- lytic t. In addition, we estimate the emissivities of two other neutrino-production mechanisms which are usually neglected { neutrino-pair bremsstrahlung processes due to electron-proton and electron-electron collisions. We show that the electron- fluxoid and electron-electron scattering can provide the main neutrino production mechanisms in the neutron star cores with highly superfluid protons and neutrons at T 10 13 G." @default.
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- W2140174380 date "1997-09-01" @default.
- W2140174380 modified "2023-09-23" @default.
- W2140174380 title "NEUTRINO PAIR EMISSION DUE TO SCATTERING OF ELECTRONS OFF FLUXOIDS IN SUPERFLUID NEUTRON STAR CORES" @default.
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