Isothermal spheres in general relativity and Horava-type gravity
arXiv:2010.00173 · doi:10.1103/PhysRevD.103.064058
Abstract
We construct a toy model for isothermal spheres in Horava gravity, which includes Einstein's gravity if a parameter is appropriately chosen. The equations for the isothermal spheres are derived from the partition function of the gravitating particle system. We confirm that the Newtonian limit of the system coincides with the model of the well-known isothermal sphere. The stability of the isothermal sphere is found to be sensitive to the energy density at the center of the sphere.
17 pages, 12 figures. v5; almost matches the published version
References in corpus (13)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Quantum Gravity at a Lifshitz Point
- Membranes at Quantum Criticality
- Stellar structure models in modified theories of gravity: lessons and challenges
- MOND-like Fractional Laplacian Theory
- On the Kuzmin model in fractional Newtonian gravity
- Minimally Modified Gravity fitting Planck data better than CDM
- Minimally modified gravity with an auxiliary constraint: a Hamiltonian construction
- Newtonian Fractional-Dimension Gravity and Rotationally Supported Galaxies
- Newtonian Fractional-Dimension Gravity and MOND
- Newtonian Fractional-Dimension Gravity and Disk Galaxies
- Caloric curves of classical self-gravitating systems in general relativity
- Gradient modification of Newtonian gravity