The DOI matches its Crossref record; 16 of the 16 references it cites were found in a registry or an index.
Dark-matter spike at the galactic center?
Open accessAbstract
The past growth of the central black hole (BH) might have enhanced the density of cold dark matter halo particles at the galactic center. We compute this effect in realistic growth models of the present $(2\ensuremath{-}3)\ifmmode\times\else\texttimes\fi{}{10}^{6}{M}_{\ensuremath{\bigodot}}$ BH from a low-mass seed BH, with special attention to dynamical modeling in a realistic galaxy environment with merger and orbital decay of a seed BH formed generally outside the exact center of the halo. An intriguing ``very-dense spike'' of dark matter has been claimed in models of Gondolo and Silk with a density high enough to contradict with experimental upper bounds of neutralino annihilation radiation. This ``spike'' disappears completely or is greatly weakened when we include important dynamical processes neglected in their idealized or restrictive picture with cold particles surrounding an at-the-center zero-seed adiabatically growing BH. For the seed BH to spiral in and settle to the center within a Hubble time by dynamical friction, the seed mass must be at least a significant fraction of the present BH. Any subsequent at-the-center growth of the BH and steepening of the central Keplerian potential well can squeeze the halo density distribution only mildly, whether the squeezing happens adiabatically or instantaneously.
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Citations
Cites
The Structure of Cold Dark Matter Halos
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Self-citationNon-baryonic dark matter: observational evidence and detection methods
Bergström, L. (2000) · Reports on Progress in Physics · doi:10.1088/0034-4885/63/5/2r3 · Cited by 904
Resolving the Structure of Cold Dark Matter Halos
Moore, B., Governato, F., Quinn, T., Stadel, J., & Lake, G. (1998) · The Astrophysical Journal · doi:10.1086/311333 · Cited by 898
Dark Matter Annihilation at the Galactic Center
Gondolo, P., & Silk, J. (1999) · Physical Review Letters · doi:10.1103/physrevlett.83.1719 · Cited by 777
Ghez, A. M., Klein, B. L., Morris, M., & Becklin, E. E. (1998) · The Astrophysical Journal · doi:10.1086/306528 · Cited by 769
Analytical models for galactic nuclei
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Self-citationObservations of stellar proper motions near the Galactic Centre
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Rates of tidal disruption of stars by massive central black holes
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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
Ghez, A. M., Salim, S., Weinberg, N. N., Lu, J. R., Do, T., Dunn, J. K., Matthews, K., Morris, M. R., Yelda, S., Becklin, E. E., et al. (2008) · The Astrophysical Journal · doi:10.1086/592738 · Cited by 1,577
Stellar Orbits around the Galactic Center Black Hole
Ghez, A. M., Salim, S., Hornstein, S. D., Tanner, A., Lu, J. R., Morris, M., Becklin, E. E., & Duchene, G. (2005) · The Astrophysical Journal · doi:10.1086/427175 · Cited by 802
Astrophysics with the Laser Interferometer Space Antenna
Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., Bartos, I., Bavera, S. S., Bellovary, J., Berry, C. P. L., et al. (2023) · Living Reviews in Relativity · doi:10.1007/s41114-022-00041-y · Cited by 609
Hui, L. (2021) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-120920-010024 · Cited by 373
Metadata
- Authors
- Ullio, P., Zhao, H., & Kamionkowski, M.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2001-07-20
- Volume
- 64
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2099693814
- Cited by
- 324
- References
- 16
- FWCI
- 9.12
- Type
- journal article
- Language
- en
- Open access
- bronze
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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