Latest Research in Galaxies: Formation, Evolution, Phenomena

Top Research Topics in Galaxies: Formation, Evolution, Phenomena

• Cosmology and Gravitation Theories — 74 papers
• Cosmology and Nongalactic Astrophysics — 48 papers
• General Relativity and Quantum Cosmology — 29 papers
• Galaxies: Formation, Evolution, Phenomena — 26 papers
• High Energy Astrophysical Phenomena — 23 papers
• High Energy Physics - Phenomenology — 17 papers
• Nuclear Theory — 16 papers
• Pulsars and Gravitational Waves Research — 7 papers
• Astrophysical Phenomena and Observations — 6 papers
• Dark Matter and Cosmic Phenomena — 4 papers

Highest-Cited Papers

1. History-Dependent Gravity LXV: Reproducible Code and Data
2. History-Dependent Gravity LXV: Reproducible Code and Data
3. A Deep Inquiry into Galactic SpiralArm Curling Evolution
4. Late-time varying-speed-of-light test of the DESI DR2 geometrical preference
5. Is Dark Matter Really Matter?
6. Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii
7. On the Possibility of a Strong First-Order Phase Transition in Neutron Stars
8. Two Barriers to the MOND Acceleration Coefficient: the de Sitter-Unruh Balance Is Orbital-Invariant at a0 = 2 c H_Lambda, and Rotation-Curve Determinations of a0 Are Definition-Limited at 30%
9. A Tale of Two Couplings: Bayesian Selection in the Interacting Dark Sector
10. Two Barriers to the MOND Acceleration Coefficient: the de Sitter-Unruh Balance Is Orbital-Invariant at a0 = 2 c H_Lambda, and Rotation-Curve Determinations of a0 Are Definition-Limited at 30%
11. Two Barriers to the MOND Acceleration Coefficient: the de Sitter-Unruh Balance Is Orbital-Invariant at a0 = 2 c H_Lambda, and Rotation-Curve Determinations of a0 Are Definition-Limited at 30%
12. Two Barriers to the MOND Acceleration Coefficient: the de Sitter-Unruh Balance Is Orbital-Invariant at a0 = 2 c H_Lambda, and Rotation-Curve Determinations of a0 Are Definition-Limited at 30%
13. Cluster Mass from the Non Linear Superposition of Galactic Scalar Fields
14. Two Barriers to the MOND Acceleration Coefficient: the de Sitter-Unruh Balance Is Orbital-Invariant at a0 = 2 c H_Lambda, and Rotation-Curve Determinations of a0 Are Definition-Limited at 30%
15. Cluster Mass from the Non Linear Superposition of Galactic Scalar Fields
16. Does strange meson condensation reduce the moment of inertia of massive proto neutron stars? insights at S = 1 and YL = 0.4
17. From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State
18. Universal Relations for Elastic Hybrid Stars and Quark Stars
19. Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity
20. Systematic study of the morphology and length of slow stable hybrid star branches