Cosmology with a Non-minimally Coupled Dark Matter Fluid II. Cosmological Perturbations

arXiv:2607.00137 · gr-qc, astro-ph.CO · Submitted 2026-06-30 · Read on arXiv

gr-qc, astro-ph.CO

Submitted: 2026-06-30

Updated: 2026-10-01

Comments: 27 pages + references, 5 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Adam — 6× in this paper · explained in 2 episodes
Quantization — 3× in this paper · explained in 12 episodes
Abundance — 2× in this paper · explained in 1 episode
Anisotropy — 2× in this paper · explained in 3 episodes
Clustering — 2× in this paper · explained in 2 episodes
Consistency — 2× in this paper · explained in 3 episodes
Matter Power Spectrum — 2× in this paper · explained in 2 episodes
Alignment — 1× in this paper · explained in 1 episode
Boltzmann Equation — 1× in this paper · explained in 2 episodes
Conservation Laws — 1× in this paper · explained in 3 episodes
Decoupling — 1× in this paper · explained in 2 episodes
Nine-Year Wilkinson Microwave Anisotropy Probe — 1× in this paper
Non-Gaussianity — 1× in this paper · explained in 2 episodes
Robustness — 1× in this paper · explained in 5 episodes
Trace — 1× in this paper · explained in 2 episodes
Weak Lensing — 1× in this paper · explained in 2 episodes

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