The DOI matches its Crossref record; 12 of the 12 references it cites were found in a registry or an index.
Weakly interacting massive particles and neutron stars
Abstract
Neutron stars are used to set constraints on the characteristics of weakly interacting massive particles (WIMP's) suggested as dark-matter candidates. Some special classes of WIMP's are ruled out because they would be trapped in neutron stars, concentrate towards the star center, and become self-gravitating. This results in the formation of a mini black hole that consumes the neutron star, transforming it into a black hole, on a time scale shorter than observed ages of neutron stars in various astrophysical systems.
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Citations
Cites
Black Holes, White Dwarfs, and Neutron Stars: The Physics of Compact Objects
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Bondi, S. H. (1974) · Journal of the Franklin Institute · doi:10.1016/0016-0032(74)90062-3 · Cited by 2,797
Formation of galaxies and large-scale structure with cold dark matter
Blumenthal, G. R., Faber, S. M., Primack, J. R., & Rees, M. J. (1984) · Nature · doi:10.1038/311517a0 · Cited by 1,629
Detectability of certain dark-matter candidates
Goodman, M. W., & Witten, E. (1985) · Physical Review D · doi:10.1103/physrevd.31.3059 · Cited by 1,286
Existence and Nature of Dark Matter in the Universe
Trimble, V. (1987) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.25.090187.002233 · Cited by 776
Capture by the sun of a galactic population of weakly interacting, massive particles
Press, W. H., & Spergel, D. N. (1985) · The Astrophysical Journal · doi:10.1086/163485 · Cited by 498
Accretion-driven stellar X-ray sources
Lewin, W. H. G., & van den Heuvel, E. P. J. (1983) · Medical Entomology and Zoology · Cited by 485
The collisionless damping of density fluctuations in an expanding universe
Bond, J. R., & Szalay, A. S. (1983) · The Astrophysical Journal · doi:10.1086/161460 · Cited by 381
A Microscopic Interpretation of Neutron Star Structure
Arnett, W. D., & Bowers, R. L. (1977) · The Astrophysical Journal Supplement Series · doi:10.1086/190434 · Cited by 315
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Evolution of close neutron star binaries
Clark, J. P. A., & Eardley, D. M. (1977) · The Astrophysical Journal · doi:10.1086/155360 · Cited by 180
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Cited by
Particle dark matter: evidence, candidates and constraints
Bertone, G., Hooper, D., & Silk, J. (2005) · Physics Reports · doi:10.1016/j.physrep.2004.08.031 · Cited by 4,979
Testing the nature of dark compact objects: a status report
Cardoso, V., & Pani, P. (2019) · Living Reviews in Relativity · doi:10.1007/s41114-019-0020-4 · Cited by 956
Black holes, gravitational waves and fundamental physics: a roadmap
Askar, A., Belczynski, C., Bertone, G., Bon, E., Blas, D., Brito, R., Bulik, T., Burrage, C., Byrnes, C. T., Caprini, C., et al. (2019) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ab0587 · Cited by 744
REVIEW OF ASYMMETRIC DARK MATTER
PETRAKI, K., & VOLKAS, R. R. (2013) · International Journal of Modern Physics A · doi:10.1142/s0217751x13300287 · Cited by 488
Can neutron stars constrain dark matter?
Kouvaris, C., & Tinyakov, P. (2010) · Physical Review D · doi:10.1103/physrevd.82.063531 · Cited by 270
Metadata
- Authors
- Goldman, I., & Nussinov, S.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1989-11-15
- Volume
- 40
- Issue
- 10
- Pages
- 3221-3230
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2091474967
- Cited by
- 320
- References
- 12
- FWCI
- 1.00
- Type
- journal article
- Language
- en
- Open access
- closed
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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.
