Neutrino Reactions in Strong Magnetic Field

Details Neutrino Reactions in Strong Magnetic Field Neutrino Reactions in Strong Magnetic Field

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..28..145c&link_type=abstract

Astrophysics and Space Science, Volume 28, Issue 1, pp.145-161

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

We present the energy losses due to several neutrinos processes: (1) synchrotron neutrinos, (2) pair annihilation neutrinos, (3) plasmon neutrinos, and (4) photoneutrinos in the presence of a superstrong magnetic field. Numerical results are tabulated and illustrated for several values of densities and temperatures. In the low density regime (ϱ≲107 g cm-3) the presence of a magnetic field decreases the luminosity, whereas the opposite is true at higher densities. This last effect is however almost entirely due to the existence of a new process the synchrotron neutrinos that disappear whenH→0. Even though the overall effect can only be quantitatively ascertain after a complete cooling computation is performed, one should however expect a much lower temperature for neutron star surface than the one computed in theH=0 case.

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