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SN 1987A Gamma-Ray Limits on the Conversion of Pseudoscalars

J. W. Brockway·E. D. Carlson·G. G. Raffelt
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Abstract

Pseudoscalar particles $ϕ$ usually couple electromagnetically by an interaction of the form $\frc14 g ϕF {\widetilde F}$, 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 $γ$-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 $g^{-1}>1{\times}10^{11}\,\rm GeV$, assuming the pseudoscalar is massless. This is an improvement over other astrophysical limits of a factor of about 2.5.

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J. W. Brockway, E. D. Carlson, G. G. Raffelt. 1996-05-31. SN 1987A Gamma-Ray Limits on the Conversion of Pseudoscalars. https://doi.org/10.1016/0370-2693(96)00778-2

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