Latest Research in Astrophysics of Galaxies
15 research papers · 2026 median publication year
Top Research Topics in Astrophysics of Galaxies
- Cosmology and Gravitation Theories — 7 papers
- Cosmology and Nongalactic Astrophysics — 4 papers
- Astrophysics of Galaxies — 2 papers
- Pulsars and Gravitational Waves Research — 1 papers
- History and Developments in Astronomy — 1 papers
Highest-Cited Papers
- MIsCORE–RIUD: Paper VIII Horizon Formation, Relaxation, and the GR-Side Mechanism
- Peering Beyond the Veil of Last Scattering: A View of the Universe with CMB Spectral Distortions
- Time‑Accumulated Vacuum Cosmology v3.6 Unified Proper‑Time Tracking Model for Evolving Dark Energy ρ₍vac₎(x) = ρ₀ [1 + k Φ(x)/c²]
- Time‑Accumulated Vacuum Cosmology v3.6 Unified Proper‑Time Tracking Model for Evolving Dark Energy ρ₍vac₎(x) = ρ₀ [1 + k Φ(x)/c²]
- Time‑Accumulated Vacuum Cosmology v3.6 Unified Proper‑Time Tracking Model for Evolving Dark Energy ρ₍vac₎(x) = ρ₀ [1 + k Φ(x)/c²]
- Time‑Accumulated Vacuum Cosmology v3.6 Unified Proper‑Time Tracking Model for Evolving Dark Energy ρ₍vac₎(x) = ρ₀ [1 + k Φ(x)/c²]
- Initial clustering of primordial black holes: A general formulation for arbitrary local non-Gaussianity
- Predictive Anticipations regarding the Nancy Grace Roman Space Telescope
- Fractional Bose-Einstein Condensate Dark Matter Cores: Numerical GPP Solutions and SPARC Rotation Curves
- Real Panthen+SH0ES, DESI BAO and f sigma8 Observational Test of Cosmological Special and General Relativity(CSTR/CGR):MCMC Analysis with Full Covariance and Second-Order (HX/c)^2 Corrections
- Consistency between cosmological and standard siren observations in evolving dark energy
- The exponential growth of infinitesimal perturbations in the long-term evolution of simulated galaxies
- QBRT: A Predictive Theory of Dark Energy and the Cosmological Constant
- A normalization-independent estimate of the evolution index of the radial-acceleration scale
- Constraining Gravitational Waves from Superconducting Cosmic Strings with the Dark Ages $21$-cm Signal