Galactic sparsity and -gravity
arXiv:2008.10463 · doi:10.1142/S0217732320502995
Abstract
The sparsity parameter for clusters of galaxies is obtained in the context of -gravity. It is shown that, the theoretical estimated values are within the reported error limits of the measured data. Thus, in the future the sparsity parameter can serve as an informative new test to detect the discrepancy between General Relativity and -gravity.
arXiv comment6 pages, Mod. Phys. Lett. A (in press)
References in corpus (16)
- Planck 2015 results. XIII. Cosmological parameters
- A Universal Density Profile from Hierarchical Clustering
- Direct Detection of WIMP Dark Matter: Concepts and Status
- The size - virial radius relation of galaxies
- CLASH: The Concentration-Mass Relation of Galaxy Clusters
- Directional axion detection
- The cosmological constant derived via galaxy groups and clusters
- Two fundamental constants of gravity unifying the dark matter and the dark energy
- Messier 81's Planck view vs its halo mapping
- Extended galactic rotational velocity profiles in gravity background
- Planck view of the M82 galaxy
- Cosmological constant as a fundamental constant
- Dark Matter Halo Sparsity of Modified Gravity Scenarios
- Gravity lens critical test for gravity constants and dark sector
- Rotating baryonic dark halos
- On the structure of galactic halos and the microwave temperature maps