Higher spin dark matter

Details Higher spin dark matter Higher spin dark matter

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1241.1192a&link_type=abstract

INVISIBLE UNIVERSE: Proceedings of the Conference. AIP Conference Proceedings, Volume 1241, pp. 1192-1197 (2010).

Other

Dark Matter, Gamma-Ray Sources (Astronomical), Cosmology, Redshift, Dark Matter, Gamma-Ray Sources, Gamma-Ray Bursts, Observational Cosmology, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

We analyze the role of spin three gauge fields as dark matter candidates. The relevant feature of these higher spin fields is that they do not couple directly to Standard Model particles. Their only direct coupling is to the gravitational field which explains the very weak interactions with other fields and enhances their qualities as realistic candidates for dark matter. The mass of these particles is provided by a Higgs-like mechanism with the gravitational field playing the role of Higgs field.

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