Sneutrinos from Cygnus X-3?

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Abstract

The possibility that the underground muons arriving from Cygnus X-3 are due to a flux of sneutrinos is analyzed. Crude approximations show that the muons can be due to a resonance production of light charged gauginos produced in sneutrino-electron collisions. © 1986 Springer-Verlag.
Original languageEnglish
Pages (from-to)401-403
JournalZeitschrift für Physik C Particles and Fields
Volume32
Issue number3
DOIs
Publication statusPublished - 1 Sep 1986

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    Pascual, R. (1986). Sneutrinos from Cygnus X-3? Zeitschrift für Physik C Particles and Fields, 32(3), 401-403. https://doi.org/10.1007/BF01551837