Predicted intensity of gamma rays from photonium

Details Predicted intensity of gamma rays from photonium Predicted intensity of gamma rays from photonium

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994zphya.349..189r&link_type=abstract

Zeitschrift für Physik A Hadrons and Nuclei, Volume 349, Issue 2, pp.189-193

Physics

95.35.+D, 98.70.Sa, 95.30.Dr

Scientific paper

We have shown in a previous paper that stable electron-positron resonances (“photonium”) can account for the dark matter in the universe. In this paper we show that photonium in the galaxy will be dissociated by cosmic rays. We predict the intensity of the resulting 511 keV gamma rays as a test of the model. We find that the predictions exceed observations from the galactic center for model where the photonium has a similar distribution to the baryons. The predicted intensity is consistent with observations if the photonium is distributed in a large halo.

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