The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
Self-interacting dark matter
Open accessAbstract
A new type of dark matter is considered. As with cold dark matter, when the dark matter is nonrelativistic, it does not couple to the electron-photon plasma, so its entropy per comoving volume is fixed. The new feature is that there is a cosmological era where number-changing reactions keep the dark matter in chemical equilibrium so that the chemical potential vanishes. This has several interesting consequences: during this era the dark matter cannibalizes its rest mass to keep warm, its temperature dropping only logarithmically with scale. We have done a general study of such self-interacting dark matter to identify the interesting ranges for its mass, coupling, and entropy. There are two consequences of this scheme which are particularly noteworthy. The unusual evolution of energy density and density perturbations allows for the possibility of decreasing the predicted anisotropies in the cosmic microwave background by a factor of 2 or more. This dark matter allows a completely new scheme for processing density perturbations. The theory introduces a new cosmological mass scale: the Jeans mass when the number-changing processes decouple. Perturbations on this supercluster scale are the first to go nonlinear.
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Citations
Cites
Halo Properties in Cosmological Simulations of Self‐interacting Cold Dark Matter
Dave, R., Spergel, D. N., Steinhardt, P. J., & Wandelt, B. D. (2001) · The Astrophysical Journal · doi:10.1086/318417 · Cited by 389
Weakly Self-interacting Dark Matter and the Structure of Dark Halos
Yoshida, N., Springel, V., White, S. D. M., & Tormen, G. (2000) · The Astrophysical Journal · doi:10.1086/317306 · Cited by 281
van den Bosch, F. C., Robertson, B. E., Dalcanton, J. J., & de Blok, W. J. G. (2000) · The Astronomical Journal · doi:10.1086/301315 · Cited by 248
A Test of the Collisional Dark Matter Hypothesis from Cluster Lensing
Miralda‐Escude, J. (2002) · The Astrophysical Journal · doi:10.1086/324138 · Cited by 203
The Structure and Evolution of Weakly Self-interacting Cold Dark Matter Halos
Burkert, A. (2000) · The Astrophysical Journal · doi:10.1086/312674 · Cited by 182
A Quantitative Study of Interacting Dark Matter in Halos
Kochanek, C. S., & White, M. J. (2000) · The Astrophysical Journal · doi:10.1086/317149 · Cited by 148
Collisional dark matter and the structure of dark halos
Yoshida, N., Springel, V, White, S. D. M., et al. (2000) · CERN Document Server (European Organization for Nuclear Research) · Cited by 59
Galactic halos of self-interacting dark matterPreprint
Hannestad, S. (1999) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/9912558 · Cited by 36
Cited by
Harko, T., Lobo, F. S. N., Nojiri, S., & Odintsov, S. D. (2011) · Physical Review D · doi:10.1103/physrevd.84.024020 · Cited by 2,772
Observational Evidence for Self-Interacting Cold Dark Matter
Spergel, D. N., & Steinhardt, P. J. (2000) · Physical Review Letters · doi:10.1103/physrevlett.84.3760 · Cited by 2,097
In the realm of the Hubble tension—a review of solutions *
Di Valentino, E., Mena, O., Pan, S., Visinelli, L., Yang, W., Melchiorri, A., Mota, D. F., Riess, A. G., & Silk, J. (2021) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ac086d · Cited by 2,065
Dark matter self-interactions and small scale structure
Tulin, S., & Yu, H.-B. (2018) · Physics Reports · doi:10.1016/j.physrep.2017.11.004 · Cited by 1,111
Structure Formation with Generalized Dark Matter
Hu, W. (1998) · The Astrophysical Journal · doi:10.1086/306274 · Cited by 420
Metadata
- Authors
- Carlson, E. D., Machacek, M. E., & Hall, L. J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1992-10
- Volume
- 398
- Pages
- 43
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2004949601
- Cited by
- 458
- References
- 8
- FWCI
- 0.54
- Type
- journal article
- Language
- en
- Open access
- green
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.