The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.
Galactic searches for dark matter
Open accessAbstract
Abstract For nearly a century, more mass has been measured in galaxies than is contained in the luminous stars and gas. Through continual advances in observations and theory, it has become clear that the dark matter in galaxies is not comprised of known astronomical objects or baryonic matter, and that identification of it is certain to reveal a profound connection between astrophysics, cosmology, and fundamental physics. The best explanation for dark matter is that it is in the form of a yet undiscovered particle of nature, with experiments now gaining sensitivity to the most well-motivated particle dark matter candidates. In this article, I review measurements of dark matter in the Milky Way and its satellite galaxies and the status of Galactic searches for particle dark matter using a combination of terrestrial and space-based astroparticle detectors, and large scale astronomical surveys. I review the limits on the dark matter annihilation and scattering cross sections that can be extracted from both astroparticle experiments and astronomical observations, and explore the theoretical implications of these limits. I discuss methods to measure the properties of particle dark matter using future experiments, and conclude by highlighting the exciting potential for dark matter searches during the next decade, and beyond.
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Citations
Cites
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 2×
“Further, it was found that the outer regions of the density profile fall-off more steeply, as r−3, and that this double power law model, the Navarro-Frenk-White (NFW) profile, is nearly universal in halos over a wide range of mass scales (Navarro et al., 1996).”
BackgroundParticle 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
A Catalog of Parameters for Globular Clusters in the Milky Way
Harris, W. E. (1996) · The Astronomical Journal · doi:10.1086/118116 · Cited by 4,500
THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION
Atwood, W. B., Abdo, A. A., Ackermann, M., Althouse, W., Anderson, B., Axelsson, M., Baldini, L., Ballet, J., Band, D. L., Barbiellini, G., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/2/1071 · Cited by 4,198
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
THE OBSERVED PROPERTIES OF DWARF GALAXIES IN AND AROUND THE LOCAL GROUP
McConnachie, A. W. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/144/1/4 · Cited by 1,869
SEGUE: A SPECTROSCOPIC SURVEY OF 240,000 STARS WITH g = 14-20
Yanny, B., Rockosi, C., Newberg, H. J., Knapp, G. R., Adelman-McCarthy, J. K., Alcorn, B., Allam, S., Prieto, C. A., An, D., Anderson, K. S. J., et al. (2009) · The Astronomical Journal · doi:10.1088/0004-6256/137/5/4377 · Cited by 1,162
McMillan, P. J. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18564.x · Cited by 789
Direct Detection of Cold Dark Matter Substructure
Dalal, N., & Kochanek, C. S. (2002) · The Astrophysical Journal · doi:10.1086/340303 · Cited by 610
THE MILKY WAY'S CIRCULAR-VELOCITY CURVE BETWEEN 4 AND 14 kpc FROM APOGEE DATA
Bovy, J., Allende Prieto, C., Beers, T. C., Bizyaev, D., da Costa, L. N., Cunha, K., Ebelke, G. L., Eisenstein, D. J., Frinchaboy, P. M., García Pérez, A. E., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/759/2/131 · Cited by 413
Gravitational detection of a low-mass dark satellite galaxy at cosmological distance
Vegetti, S., Lagattuta, D. J., McKean, J. P., Auger, M. W., Fassnacht, C. D., & Koopmans, L. V. E. (2012) · Nature · doi:10.1038/nature10669 · Cited by 386
THE FERMI HAZE: A GAMMA-RAY COUNTERPART TO THE MICROWAVE HAZE
Dobler, G., Finkbeiner, D. P., Cholis, I., Slatyer, T., & Weiner, N. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/717/2/825 · Cited by 285 · cited 2×
“erized, an interesting morphological structure has come to light in recent analysis of the data. After subtracting out templates for the neutral pion, inverse Compton, and 74 bremsstrahlung emission, Dobler et al. (2010) rst reported a detection of the \Fermi Haze," which extends 50above and below the Galactic pl…”
BackgroundMethodAn Improved Proper-Motion Catalog Combining USNO-B and the Sloan Digital Sky Survey
Munn, J. A., Monet, D. G., Levine, S. E., Canzian, B., Pier, J. R., Harris, H. C., Lupton, R. H., Ivezić, Ž., Hindsley, R. B., Hennessy, G. S., et al. (2004) · The Astronomical Journal · doi:10.1086/383292 · Cited by 251
The missing massive satellites of the Milky Way
Wang, J., Frenk, C. S., Navarro, J. F., Gao, L., & Sawala, T. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21357.x · Cited by 185 · cited 1×
“Specifically, if the Milky Way mass is approximately 1012 M , the number of subhalos with maximum circular velocity & 30 km/s can be made consistent with observations (Wang et al., 2012).”
Broken degeneracies: the rotation curve and velocity anisotropy of the Milky Way halo
Deason, A. J., Belokurov, V., Evans, N. W., & An, J. (2012) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1111/j.1745-3933.2012.01283.x · Cited by 133
Cited by
Small-Scale Challenges to the ΛCDM Paradigm
Bullock, J. S., & Boylan-Kolchin, M. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-091916-055313 · Cited by 1,504
Ackermann, M., Albert, A., Anderson, B., Atwood, W. B., Baldini, L., Barbiellini, G., Bastieri, D., Bechtol, K., Bellazzini, R., Bissaldi, E., et al. (2015) · Physical Review Letters · doi:10.1103/physrevlett.115.231301 · Cited by 1,116
Self-citationBillard, J., Figueroa-Feliciano, E., & Strigari, L. (2014) · Physical Review D · doi:10.1103/physrevd.89.023524 · Cited by 719
Self-citationTaking atom interferometric quantum sensors from the laboratory to real-world applications
Bongs, K., Holynski, M., Vovrosh, J., Bouyer, P., Condon, G., Rasel, E., Schubert, C., Schleich, W. P., & Roura, A. (2019) · Nature Reviews Physics · doi:10.1038/s42254-019-0117-4 · Cited by 382
MAGIC collaboration (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/02/039 · Cited by 308
Metadata
- Authors
- Strigari, L. E.
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2013-10
- Volume
- 531
- Issue
- 1
- Pages
- 1-88
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W1963782091
- Cited by
- 256
- References
- 15
- FWCI
- 12.53
- Type
- journal article
- Language
- en
- Open access
- green
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