Massive mimetic cosmology

Autor: Adam R. Solomon, Yashar Akrami, Valeri Vardanyan
Přispěvatelé: Laboratoire de physique de l'ENS - ENS Paris (LPENS (UMR_8023)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Astrophysique, École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Université Paris Diderot - Paris 7 (UPD7)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Université Paris Diderot - Paris 7 (UPD7)
Jazyk: angličtina
Rok vydání: 2019
Předmět:
High Energy Physics - Theory
Nuclear and High Energy Physics
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
perturbation
gravitation: model
stability: linear
Dark matter
gravitation: effect
FOS: Physical sciences
General Relativity and Quantum Cosmology (gr-qc)
Cosmological constant
Astrophysics::Cosmology and Extragalactic Astrophysics
Curvature
graviton: mass
cosmological constant: negative
01 natural sciences
General Relativity and Quantum Cosmology
Cosmology
dark matter: parametrization
Metric expansion of space
Theoretical physics
High Energy Physics::Theory
cosmological model: parameter space
0103 physical sciences
structure
gravitation: massive
010306 general physics
Physics
010308 nuclear & particles physics
[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]
Graviton
acceleration
ghost
lcsh:QC1-999
graviton: effect
Massive gravity
High Energy Physics - Theory (hep-th)
dark energy: density
curvature
Dark energy
[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
history
mass: gravitation
lcsh:Physics
Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj: Phys.Lett.B
Phys.Lett.B, 2019, 794, pp.135-142. ⟨10.1016/j.physletb.2019.05.045⟩
Physics Letters
Physics Letters B, Vol 794, Iss, Pp 135-142 (2019)
Physics Letters B, 794, 135-142
Physics Letters B
Physics Letters B, Elsevier, 2019, 794, pp.135-142. ⟨10.1016/j.physletb.2019.05.045⟩
ISSN: 0370-2693
DOI: 10.1016/j.physletb.2019.05.045⟩
Popis: We study the first cosmological implications of the mimetic theory of massive gravity recently proposed by Chamseddine and Mukhanov. This is a novel theory of ghost-free massive gravity which additionally contains a mimetic dark matter component. In an echo of other modified gravity theories, there are self-accelerating solutions which contain a ghost instability. In the ghost-free region of parameter space, the effect of the graviton mass on the cosmic expansion history amounts to an effective negative cosmological constant, a radiation component, and a negative curvature term. This allows us to place constraints on the model parameters---the graviton mass and the St\"uckelberg vacuum expectation value---by insisting that the effective radiation and curvature terms be within observational bounds. The late-time acceleration must be accounted for by a separate positive cosmological constant or other dark energy sector. We impose further constraints at the level of perturbations by demanding linear stability. We comment on the possibility of distinguishing this theory from $\Lambda$CDM with current and future large-scale structure surveys.
Comment: 9+1 pages, 1 figure. Version published in PLB
Databáze: OpenAIRE