Neutrino Synchrotron Radiation. II: Application to Neutron Stars

Details Neutrino Synchrotron Radiation. II: Application to Neutron Stars Neutrino Synchrotron Radiation. II: Application to Neutron Stars

Sep 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...8..448c&link_type=abstract

Astrophysics and Space Science, Volume 8, Issue 3, pp.448-456

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

The neutrino luminosity of several models of neutron stars has been computed according to the photon-neutrino coupling theory and compared with that of the current-current coupling theory. It is shown that the NSR process alone should have cooled the core of the neutron star created in a supernova explosion in 1954 A.D. to a temperature around 2×109 K according to the photon-neutrino coupling theory. The emission power of the star is greater than the emission power of the X-ray source discovered in the Crab Nebula; so the source may be interpreted as the thermal radiation of the star according to the photon-neutrino coupling theory.

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