Condensate of Massive Graviton and Dark Matter
arXiv:1707.05003 · doi:10.1103/PhysRevD.97.044002
Abstract
We study coherently oscillating massive gravitons in the ghost-free bigravity theory. This coherent field can be interpreted as a condensate of the massive gravitons. We first define the effective energy-momentum tensor of the coherent massive gravitons in a curved spacetime. We then study the background dynamics of the universe and the cosmic structure formation including the effects of the coherent massive gravitons. We find that the condensate of the massive graviton behaves as a dark matter component of the universe. From the geometrical point of view the condensate is regarded as a spacetime anisotropy. Hence, in our scenario, dark matter is originated from the tiny deformation of the spacetime. We also discuss a production of the spacetime anisotropy and find that the extragalactic magnetic field of a primordial origin can yield a sufficient amount for dark matter.
25 pages, 3 figures; v2: minor improvements, references added, published version
References in corpus (20)
- The Confrontation between General Relativity and Experiment
- Resummation of Massive Gravity
- Ultralight scalars as cosmological dark matter
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Bose-Einstein Condensation of Dark Matter Axions
- Interacting Spin-2 Fields
- Lower limit on the strength and filling factor of extragalactic magnetic fields
- Theory of cosmological perturbations in an anisotropic universe
- Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality
- Review of short-range gravity experiments in the LHC era
- On couplings to matter in massive (bi-)gravity
- Ghosts & Matter Couplings in Massive (bi-&multi-)Gravity
- Heavy spin-2 Dark Matter
- Viable cosmology in bimetric theory
- FRW Cosmological Perturbations in Massive Bigravity
- Appearance of Boulware-Deser ghost in bigravity with doubly coupled matter
- Quantum corrections in massive bigravity and new effective composite metrics
- Dark matter in ghost-free bigravity theory: From a galaxy scale to the universe
- Perturbations of ultralight vector field dark matter
- Vainshtein mechanism in massive gravity nonlinear sigma models
Cited by in corpus (26)
- Black holes, gravitational waves and fundamental physics: a roadmap
- The EDGES 21 cm Anomaly and Properties of Dark Matter
- Pulsar timing residual induced by ultralight tensor dark matter
- Higher Spin Dark Matter
- Pulsar timing residual induced by ultralight vector dark matter
- Vector Fuzzy Dark Matter, Fifth Forces, and Binary Pulsars
- On-shell effective theory for higher-spin dark matter
- Pulsar timing array constraints on spin-2 ULDM
- Gravitational wave probes of particle dark matter: a review
- Spin-2 dark matter from anisotropic Universe in bigravity
- Cosmological Perturbation Theory in Metric-Affine Gravity
- Binary Pulsars as probes for Spin-2 Ultralight Dark Matter
- Searching for spin-2 ULDM with gravitational waves interferometers
- Massive Graviton Geons
- Constraining ultralight dark matter using the Fermi-LAT pulsar timing array
- Massive spin-2 field in arbitrary spacetimes -- the detailed derivation
- Massive graviton dark matter with environment dependent mass: A natural explanation of the dark matter-baryon ratio
- Towards A Direct Detection of the Spin of Dark Matter
- Non-linearly ghost-free higher curvature gravity
- Angular correlation and deformed Hellings-Downs curve from spin-2 ultralight dark matter
- Massive graviton dark matter searches with long-baseline atom interferometers
- The imprint of ultralight vector fields on gravitational wave propagation
- Probing Spin-2 Ultralight Dark Matter with Space-based Gravitational Wave Detectors in the mHz Regime
- Completing the dark matter solutions in degenerate Kaluza-Klein theory
- Signature of polarized ultralight vector dark matter in pulsar timing arrays
- Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons