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06 October 2024
 
  » arxiv » astro-ph/9605197

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SN 1987A Gamma-Ray Limits on the Conversion of Pseudoscalars
J.W. Brockway ; E.D. Carlson ; G.G. Raffelt ;
Date 31 May 1996
Journal Phys.Lett. B383 (1996) 439-443
AbstractPseudoscalar particles $phi$ usually couple electromagnetically by an interaction of the form $frc14 g phi F {widetilde F}$, allowing them to convert to photons in the presence of magnetic fields. Notably, new low-mass pseudoscalars emitted from supernova (SN) 1987A would have been converted to $gamma$-rays in the intervening magnetic field of the galaxy. Therefore, measurements by the Solar Maximum Mission (SMM) Gamma-Ray Spectrometer (GRS) can limit the inverse coupling constant to $g^{-1}>1{ imes}10^{11}, m GeV$, assuming the pseudoscalar is massless. This is an improvement over other astrophysical limits of a factor of about 2.5.
Source arXiv, astro-ph/9605197
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