Axion flux from nascent neutron stars

Details Axion flux from nascent neutron stars Axion flux from nascent neutron stars

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phlb..203..469h&link_type=abstract

Physics Letters B, Volume 203, Issue 4, p. 469-473.

Physics

36

Scientific paper

The emission rate of the invisible axion due to electron-related processes is evaluated in detail at high temperatures (T~20 MeV) and at high densities (ρ~1014g cm-3), relevant to the supernova explosion. If one properly treats relativistic kinematics, no useful bound on the Peccei-Quinn symmetry breaking scale (fA) is obtained from SN1987A, contrary to the recent argument by others. A brief comment on the bound from the neutron-neutron axion bremsstrahlung process is also made.

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