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Title: Heavy spin-2 Dark Matter

Abstract

We provide further details on a recent proposal addressing the nature of the dark sectors in cosmology and demonstrate that all current observations related to Dark Matter can be explained by the presence of a heavy spin-2 particle. Massive spin-2 fields and their gravitational interactions are uniquely described by ghost-free bimetric theory, which is a minimal and natural extension of General Relativity. In this setup, the largeness of the physical Planck mass is naturally related to extremely weak couplings of the heavy spin-2 field to baryonic matter and therefore explains the absence of signals in experiments dedicated to Dark Matter searches. It also ensures the phenomenological viability of our model as we confirm by comparing it with cosmological and local tests of gravity. At the same time, the spin-2 field possesses standard gravitational interactions and it decays universally into all Standard Model fields but not into massless gravitons. Matching the measured DM abundance together with the requirement of stability constrains the spin-2 mass to be in the 1 to 100 TeV range.

Authors:
 [1];  [2]; ;  [3];  [4];  [5]; ;  [3];  [6]
  1. Laboratoire de Physique Théorique, CNRS, Univ. Paris-Sud, Université Paris-Saclay,91405 Orsay (France)
  2. (France)
  3. National Institute of Chemical Physics and Biophysics,Rävala 10, 10143 Tallinn (Estonia)
  4. (Estonia)
  5. Institut für Theoretische Physik, Eidgenössische Technische Hochschule Zürich,Wolfgang-Pauli-Strasse 27, 8093 Zürich (Switzerland)
  6. UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, GReCO,98bis boulevard Arago, F-75014 Paris (France)
Publication Date:
Sponsoring Org.:
SCOAP3, CERN, Geneva (Switzerland)
OSTI Identifier:
22572149
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2016; Journal Issue: 09; Other Information: PUBLISHER-ID: JCAP09(2016)016; OAI: oai:repo.scoap3.org:17105; cc-by Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BARYONS; BOSONS; COSMOLOGY; COUPLING; GENERAL RELATIVITY THEORY; GRAVITATIONAL INTERACTIONS; GRAVITONS; METRICS; NONLUMINOUS MATTER; STANDARD MODEL; TEV RANGE 10-100

Citation Formats

Babichev, Eugeny, UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, GReCO,98bis boulevard Arago, F-75014 Paris, Marzola, Luca, Raidal, Martti, Laboratory of Theoretical Physics, Institute of Physics, University of Tartu,Ravila 14c, 50411 Tartu, Schmidt-May, Angnis, Urban, Federico, Veermäe, Hardi, and Strauss, Mikael von. Heavy spin-2 Dark Matter. United States: N. p., 2016. Web. doi:10.1088/1475-7516/2016/09/016.
Babichev, Eugeny, UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, GReCO,98bis boulevard Arago, F-75014 Paris, Marzola, Luca, Raidal, Martti, Laboratory of Theoretical Physics, Institute of Physics, University of Tartu,Ravila 14c, 50411 Tartu, Schmidt-May, Angnis, Urban, Federico, Veermäe, Hardi, & Strauss, Mikael von. Heavy spin-2 Dark Matter. United States. doi:10.1088/1475-7516/2016/09/016.
Babichev, Eugeny, UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, GReCO,98bis boulevard Arago, F-75014 Paris, Marzola, Luca, Raidal, Martti, Laboratory of Theoretical Physics, Institute of Physics, University of Tartu,Ravila 14c, 50411 Tartu, Schmidt-May, Angnis, Urban, Federico, Veermäe, Hardi, and Strauss, Mikael von. 2016. "Heavy spin-2 Dark Matter". United States. doi:10.1088/1475-7516/2016/09/016.
@article{osti_22572149,
title = {Heavy spin-2 Dark Matter},
author = {Babichev, Eugeny and UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, GReCO,98bis boulevard Arago, F-75014 Paris and Marzola, Luca and Raidal, Martti and Laboratory of Theoretical Physics, Institute of Physics, University of Tartu,Ravila 14c, 50411 Tartu and Schmidt-May, Angnis and Urban, Federico and Veermäe, Hardi and Strauss, Mikael von},
abstractNote = {We provide further details on a recent proposal addressing the nature of the dark sectors in cosmology and demonstrate that all current observations related to Dark Matter can be explained by the presence of a heavy spin-2 particle. Massive spin-2 fields and their gravitational interactions are uniquely described by ghost-free bimetric theory, which is a minimal and natural extension of General Relativity. In this setup, the largeness of the physical Planck mass is naturally related to extremely weak couplings of the heavy spin-2 field to baryonic matter and therefore explains the absence of signals in experiments dedicated to Dark Matter searches. It also ensures the phenomenological viability of our model as we confirm by comparing it with cosmological and local tests of gravity. At the same time, the spin-2 field possesses standard gravitational interactions and it decays universally into all Standard Model fields but not into massless gravitons. Matching the measured DM abundance together with the requirement of stability constrains the spin-2 mass to be in the 1 to 100 TeV range.},
doi = {10.1088/1475-7516/2016/09/016},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 09,
volume = 2016,
place = {United States},
year = 2016,
month = 9
}
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