Joint Model-independent Constraints on the Post-Newtonian Parameter and Cosmic Curvature from Galaxy-scale Strong Lensing, SNe Ia, BAO, and Cosmic Chronometers

arXiv:2609.29377 · gr-qc, astro-ph.CO · Submitted 2026-09-24 · Read on arXiv

gr-qc, astro-ph.CO

Submitted: 2026-09-24

Updated: 2026-09-24

Terminology

Velocity Dispersion — 16× in this paper · explained in 2 episodes
Degeneracy — 15× in this paper · explained in 3 episodes
Aperture — 11× in this paper · explained in 1 episode
Calibration — 8× in this paper · explained in 7 episodes
Gravitational Lensing — 7× in this paper · explained in 2 episodes
Anisotropy — 4× in this paper · explained in 3 episodes
Consistency — 4× in this paper · explained in 3 episodes
Chebyshev Polynomials — 3× in this paper · explained in 2 episodes
Clustering — 3× in this paper · explained in 2 episodes
Accuracy — 2× in this paper · explained in 1 episode
Aperture Correction — 2× in this paper · explained in 1 episode
Benchmark — 2× in this paper · explained in 2 episodes
Systematic Bias — 2× in this paper · explained in 3 episodes
Core — 1× in this paper · explained in 2 episodes
Matter Power Spectrum — 1× in this paper · explained in 2 episodes
Metallicity — 1× in this paper · explained in 3 episodes
Model-Agnostic — 1× in this paper · explained in 2 episodes
Population Synthesis — 1× in this paper · explained in 2 episodes
Regularization — 1× in this paper · explained in 3 episodes
Robustness — 1× in this paper · explained in 5 episodes

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