Splashback in galaxy clusters as a probe of cosmic expansion and gravity
From MaRDI portal
Publication:5023704
DOI10.1088/1475-7516/2018/11/033OpenAlexW3102759997MaRDI QIDQ5023704
Susmita Adhikari, Jeremy Sakstein, Bhuvnesh Jain, Baojiu Li, Neal Dalal
Publication date: 24 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1806.04302
Related Items (2)
Relation between the turnaround radius and virial mass in f(R) model ⋮ The effect of finite halo size on the clustering of neutral hydrogen
Uses Software
Cites Work
- Unnamed Item
- Cosmological tests of gravity
- Challenges to self-acceleration in modified gravity from gravitational waves and large-scale structure
- Tests of chameleon gravity
- Constraining chameleon models with cosmology
- Relativistic stars in beyond Horndeski theories
- Manifestly Local Theory of Vacuum Energy Sequestering
- DYNAMICS OF DARK ENERGY
- Testing the Vainshtein mechanism using stars and galaxies
- Superfluids and the cosmological constant problem
- Turnaround radius in f(R) model
- Ghosts in the self-accelerating universe
- Brownian Motion, Dynamical Friction, and Stellar Dynamics
- The confrontation between general relativity and experiment
- 4D gravity on a brane in 5D Minkowski space
This page was built for publication: Splashback in galaxy clusters as a probe of cosmic expansion and gravity