Pseudoscalar Conversion and Gamma-Rays from Supernovae
Astrophysics
2007-05-23 v1 High Energy Physics - Phenomenology
Abstract
A light pseudoscalar coupled to two photons would be copiously emitted by the core of a supernova and part of this flux would be converted to gamma-rays by the galactic magnetic field. Measurements on the SN1987A gamma-ray flux by the Gamma-Ray Spectrometer on the Solar Maximum Mission satellite imply stringents bounds on such process. The improved generation of satellite-borne detectors, like EGRET or the projegeneration of satellite-borne detectors, like EGRET or the project GLAST, could be able to detect a pseudoscalar-to-photon signal from a nearby supernova.
Cite
@article{arxiv.astro-ph/9704056,
title = {Pseudoscalar Conversion and Gamma-Rays from Supernovae},
author = {Eduard Masso},
journal= {arXiv preprint arXiv:astro-ph/9704056},
year = {2007}
}
Comments
3 pages, latex, 1 figure. Talk at XXXIInd Rencontres de Moriond, ``Very High Energy Phenomena in the Universe'', Les Arcs, France (1997)