Self-interacting dark matter in cosmology: accurate numerical implementation and observational constraints
DOI10.1088/1475-7516/2022/02/024zbMath1487.83078arXiv2108.02657OpenAlexW3191918602MaRDI QIDQ5063496
Rafael Yunis, Carlos R. Argüelles, Diana López Nacir, Claudia G. Scóccola, Gastón L. Giordano
Publication date: 21 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2108.02657
cosmological perturbation theorydark matter theoryparticle physics-cosmology connectionLyman alpha forest
Relativistic cosmology (83F05) Nuclear physics (81V35) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Perturbations in context of PDEs (35B20) Dark matter and dark energy (83C56)
Cites Work
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- Dark matter self-interactions and small scale structure
- Accuracy and Stability of Numerical Algorithms
- The cosmological evolution of self-interacting dark matter
- Boltzmann hierarchies for self-interacting warm dark matter scenarios
- Kinetic Theory in the Expanding Universe
- On observables in a dark matter-clustering quintessence system
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