Dark energy survivals in massive gravity after GW170817: SO(3) invariant
From MaRDI portal
Publication:5021809
DOI10.1088/1475-7516/2018/01/044OpenAlexW2962904356MaRDI QIDQ5021809
Lavinia Heisenberg, Shinji Tsujikawa
Publication date: 14 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1711.09430
Related Items (4)
Wave operators, torsion, and Weitzenböck identities ⋮ Novel screening with two bodies: summing the ladder in disformal scalar-tensor theories ⋮ Non-trivial gravitational waves and structure formation phenomenology from dark energy ⋮ Cosmic structures and gravitational waves in ghost-free scalar-tensor theories of gravity
Cites Work
- Cosmic acceleration from abelian symmetry breaking
- Massive gravity: a general analysis
- Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
- Lorentz-violating massive gauge and gravitational fields
- Derivative self-interactions for a massive vector field
- Republication of: The dynamics of general relativity
- Variational aspects of relativistic field theories, with application to perfect fluids
- Cosmology in doubly coupled massive gravity: constraints from SNIa, BAO and CMB
- FRW cosmology in ghost free massive gravity from bigravity
- A new type of isotropic cosmological models without singularity
- Cosmology in rotation-invariant massive gravity with non-trivial fiducial metric
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- Cosmological solutions of massive gravity on de Sitter
- DYNAMICS OF DARK ENERGY
- CMB scale dependent non-Gaussianity from massive gravity during inflation
- On couplings to matter in massive (bi-)gravity
- Quantum corrections in massive bigravity and new effective composite metrics
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Non-local massive gravity
This page was built for publication: Dark energy survivals in massive gravity after GW170817: SO(3) invariant
