Effective -factor of the Galactic Center for velocity-dependent dark matter annihilation
- Johns Hopkins Univ., Baltimore, MD (United States); UH High Energy Physics Group
- Univ. of Hawaii, Honolulu, HI (United States)
- Texas A & M Univ., College Station, TX (United States)
Here, we introduce the effective -factors for the Milky Way for scenarios in which dark matter annihilation is -wave or -wave suppressed. We find that the velocity suppression of dark matter annihilation can have a sizable effect on the morphology of a potential dark matter annihilation signal in the Galactic Center. The gamma-ray flux from the innermost region of the Galactic Center is in particular suppressed. We discover that for dark matter density profiles with steep inner slopes, the morphology of the inner Galaxy gamma-ray emission in -wave models can be made similar to the morphology in standard -wave models. This similarity may suggest that model discrimination between wave and wave is challenging, e.g., when fitting the Galactic Center excess. However, we show that it is difficult to simultaneously match - and -wave morphologies at both large and small angular scales. The -factors we calculate may be implemented with astrophysical foreground models to self-consistently determine the morphology of the excess with velocity-suppressed dark matter annihilation.
- Research Organization:
- Texas A & M Univ., College Station, TX (United States); Univ. of Hawaii, Honolulu, HI (United States)
- Sponsoring Organization:
- National Science Foundation (NSF); USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- Grant/Contract Number:
- SC0010504; SC0010813
- OSTI ID:
- 1598042
- Journal Information:
- Physical Review D, Journal Name: Physical Review D Journal Issue: 6 Vol. 98; ISSN PRVDAQ; ISSN 2470-0010
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Strong constraints on light dark matter interpretation of the EDGES signal
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journal | November 2018 |
Two-integral distribution functions in axisymmetric galaxies: Implications for dark matter searches
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journal | February 2019 |
| Two-integral distribution functions in axisymmetric galaxies: implications for dark matter searches | text | January 2018 |
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