A Strong Cosmologically Coupled Mass Growth Solution in Linearized General Relativity
gr-qc, astro-ph.CO
Submitted: 2026-09-29
Updated: 2026-09-29
Terminology
Sources
- Implications of Symmetry and Pressure in Friedmann Cosmology. I. Formalism
- Cosmological term as a source of mass
- Stable gravastars - an alternative to black holes?
- Smooth transitions from Schwarzschild vacuum to de Sitter space
- Gravastars must have anisotropic pressures
- Stable dark energy stars
- Surface Tension and Negative Pressure Interior of a Non-Singular `Black Hole'
- Gravitational Aether and the thermodynamic solution to the cosmological constant problem
- Stellar Black Holes and the Origin of Cosmic Acceleration
- A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
- Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energy
- The assembly of supermassive black holes at $z<1$ in early-type galaxies from scaling relations
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0
- Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape
- Positive neutrino masses with DESI DR2 via matter conversion to dark energy
- The CMB optical depth constrains the duration of reionization
- Rapid late-time reionization: constraints and cosmological implications
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