• Open Access

Oscillating spin-2 dark matter

Luca Marzola, Martti Raidal, and Federico R. Urban
Phys. Rev. D 97, 024010 – Published 8 January 2018

Abstract

The negative outcomes of laboratory searches, juxtaposed with cosmological observations, may indicate that dark matter has a gravitational origin. We show that coherent oscillations of a massive spin-2 field emerging from bimetric theory can easily account for the observed dark matter abundance. The framework, based on the only known consistent extension of general relativity to interacting spin-2 fields, is testable in precision measurements of the electric charge variation by means of atomic clocks, molecular systems, dedicated resonant mass detectors, as well as gravity interferometers and axionlike-particle experiments. These searches, therefore, provide a new window into the phenomenology of gravity which complements the results of dedicated tests of gravitation. We also present a multimetric extension of the scenario that straightforwardly implements the clockwork mechanism for gravity, explaining the apparent weakness of this force.

  • Received 2 September 2017

DOI:https://doi.org/10.1103/PhysRevD.97.024010

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Luca Marzola, Martti Raidal, and Federico R. Urban

  • Laboratory of High Energy and Computational Physics, NICPB, Rävala puiestee 10, 10143 Tallinn, Estonia

Article Text

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Issue

Vol. 97, Iss. 2 — 15 January 2018

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