Evidence for dark matter in the inner Milky Way
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Pre-Gaia analyses of the inner Milky Way rotation curve had established robust evidence for a non-baryonic dark component already at R ≲ R0.
“PreGaia analyses of the inner MW rotation curve had nonetheless established robust evidence for a non-baryonic dark component already at R ≲ R 0 (Iocco et al., 2015), complementing the kinematic and dynamical constraints on the outer halo.”
From The rotation curve of the Milky Way: State of the art, the Keplerian decline debate, and implications for dark matter (2026) · cites this paper as Iocco et al., 2015
Currently, the stellar disc mass of the Galaxy is poorly constrained and thus cannot be used to distinguish between the two models, although most measurements agree better with the lower stellar mass of the contracted NFW halo model.
“Currently, the stellar disc mass of our galaxy is poorly constrained (e.g. see the compilation of stellar profiles in Iocco et al. 2015) and thus cannot be used to distinguish between the two models, although most measurements agree better with the lower stellar mass of the contracted NFW halo model”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Iocco et al. 2015
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Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations
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Probing Dark Matter Subhalos in Galaxy Clusters Using Highly Magnified Stars
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Testing modified Newtonian dynamics in the Milky Way
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galkin: A new compilation of Milky Way rotation curve data
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Bayesian analysis of sneutrino dark matter in the NMSSM with a type-I seesaw mechanism
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An estimate of the DM profile in the Galactic bulge region
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The dark matter component of the Gaia radially anisotropic substructure
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Gravitationally bound Bose condensates with rotation
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The dark matter profile of the milky way: A non-parametric reconstruction
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Which Milky Way masses are consistent with the slightly declining 5–25 kpc rotation curve?
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Testing MOdified Gravity (MOG) theory and dark matter model in Milky Way using the local observables
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The difficulty of measuring the local dark matter density
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A universal constant for dark matter-baryon interplay
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- Authors
- Iocco, F., Pato, M., & Bertone, G.
- Affiliations
- Stockholm University (SE)
- University of Amsterdam (NL)
- Venue
- Nature Physics
- Published
- 2015-02-09
- Volume
- 11
- Issue
- 3
- Pages
- 245-248
- ISSN
- 1745-2473 (ISSN-L)
- 1745-2481
- OpenAlex
- W2007025690
- Cited by
- 192
- References
- 61
- Citations by year
- 2026: 11 · 2025: 20 · 2024: 9 · 2023: 11 · 2022: 11 · 2021: 15 · 2020: 22 · 2019: 15 · 2018: 18 · 2017: 15 · 2016: 31 · 2015: 14
- FWCI
- 13.02
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- Nature Physics (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- UvA-DARE (University of Amsterdam) (publishedVersion)
- Acervo Digital da Universidade Estadual Paulista (Universidade Estadual Paulista) (submittedVersion)
- UNESP Institutional Repository (São Paulo State University) (submittedVersion)
- Data Archiving and Networked Services (DANS) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Wenner-Gren Stiftelserna
- University of California, Santa Barbara
- Kavli Institute for Theoretical Physics, University of California, Santa Barbara
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- dark matter, Milky Way, galaxy rotation curves, baryonic mass distribution, inner Galaxy, solar neighborhood, halo density profiles, dark matter searches
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