Linear growth index of matter perturbations in Rastall gravity
From MaRDI portal
Publication:2281073
DOI10.1016/J.PHYSLETB.2019.134796zbMath1427.83070arXiv1907.09221OpenAlexW2963171787WikidataQ127439616 ScholiaQ127439616MaRDI QIDQ2281073
Jibitesh Dutta, Wompherdeiki Khyllep
Publication date: 19 December 2019
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1907.09221
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (5)
Lemaître-Tolman-Bondi static universe in Rastall-like gravity ⋮ Effects of Rastall parameter on perturbation of dark sectors of the Universe ⋮ Thick brane in Rastall gravity ⋮ Qualitative study of a model with Rastall gravity ⋮ Ultralight DM bosons with an axion-like potential: scale-dependent constraints revisited
Cites Work
- Unnamed Item
- Unnamed Item
- Rastall gravity is equivalent to Einstein gravity
- Lorentzian causality theory
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Black hole solutions surrounded by perfect fluid in Rastall theory
- Impact of the Rastall parameter on perfect fluid spheres
- Generalization of the Einstein Theory
- PERTURBATIVE ANALYSIS OF GENERALIZED EINSTEIN THEORIES
- MODIFIED GR AND HELIUM NUCLEOSYNTHESIS
- Quantized Fields and Particle Creation in Expanding Universes. I
- The confrontation between general relativity and experiment
This page was built for publication: Linear growth index of matter perturbations in Rastall gravity