Symplectic gauge fields and dark matter

J. Asorey, M. Asorey, and D. García-Álvarez
Phys. Rev. D 92, 103517 – Published 23 November 2015

Abstract

The dynamics of symplectic gauge fields provides a consistent framework for fundamental interactions based on spin-3 gauge fields. One remarkable property is that symplectic gauge fields only have minimal couplings with gravitational fields and not with any other field of the Standard Model. Interactions with ordinary matter and radiation can only arise from radiative corrections. In spite of the gauge nature of symplectic fields they acquire a mass by the Coleman-Weinberg mechanism which generates Higgs-like mass terms where the gravitational field is playing the role of a Higgs field. Massive symplectic gauge fields weakly interacting with ordinary matter are natural candidates for the dark matter component of the Universe.

  • Received 9 September 2015

DOI:https://doi.org/10.1103/PhysRevD.92.103517

© 2015 American Physical Society

Authors & Affiliations

J. Asorey

  • Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA

M. Asorey

  • Departamento de Fí sica Teórica, Facultad de Ciencias, Universidad de Zaragoza, 50009 Zaragoza, Spain

D. García-Álvarez

  • Departamento de Análisis Económico Facultad de Economía y Empresa, Universidad de Zaragoza, 50005 Zaragoza, Spain

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Issue

Vol. 92, Iss. 10 — 15 November 2015

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