Quantum Field Theory Of Cosmological Perturbations Induced By Ultralight Dark Matter
Tomislav Prokopec, Marco Vecchioni
hep-th, astro-ph.CO, gr-qc
Submitted: 2026-07-29
Comments: 97 pages, 1 figure, 9 Feynman diagrams
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
- The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope
- Planck 2018 results. V. CMB power spectra and likelihoods
- Planck 2018 results. X. Constraints on inflation
- Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck III: Combined cosmological constraints
- Planck 2018 results. VI. Cosmological parameters
- Ultra-Light Dark Matter
- Ultralight scalars as cosmological dark matter
- Primordial Black Holes as Dark Matter Candidates
- Gravitational Wave Resonance in Ultra-Light Dark Matter Halos
- Parametric resonance of gravitational waves in general scalar-tensor theories
- Gravitational-Wave Propagation Through the Axiverse
- Scalar field dark matter in hybrid approach
- Kinetic theory and classical limit for real scalar quantum field in curved space-time
- Field-theoretic approach to large-scale structure formation
- Oscillating gravitational potential due to ultralight axion: linear theory
- Stamps of state on structure: Probing the state of ultralight dark matter via its density fluctuations
- One-loop tensor power spectrum from an excited scalar field during inflation
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