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Title: Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT

Here, we derive constraints on parameters of generic dark matter candidates by comparing theoretical predictions with the gamma-ray emission observed by the Fermi-LAT from the region around the Galactic Center. Our analysis is conservative since it simply requires that the expected dark matter signal does not exceed the observed emission. The constraints obtained in the likely case that the collapse of baryons to the Galactic Center is accompanied by the contraction of the dark matter are strong. In particular, we find that for b b¯ and τ +τ or W +W dark matter annihilation channels, the upper limits on the annihilation cross section imply that the thermal cross section is excluded for a Weakly Interacting Massive Particle (WIMP) mass smaller than about 700 and 500 GeV, respectively. For the μ +μ channel, where the effect of the inverse Compton scattering is important, depending on models of the Galactic magnetic field the exclusion of the thermal cross-section is for a WIMP mass smaller than about 150 to 400 GeV. The upper limits on the annihilation cross section of dark matter particles obtained are two orders of magnitude stronger than without contraction. In the latter case our results aremore » compatible with the upper limits from the Galactic halo analysis reported by the Fermi-LAT collaboration for the case in which the same conservative approach without modeling of the astrophysical background is employed.« less
Authors:
 [1] ;  [2] ;  [3] ;  [4] ;  [5] ;  [6] ;  [7] ;  [4] ;  [8] ;  [4]
  1. Univ. Autonoma de Madrid, Madrid (Spain); Instituto de Fisica Teorica UAM-CSIC, Madrid (Spain); Istituto Nazionale di Fisica Nucleare, Roma (Italy)
  2. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  3. Univ. Autonoma de Madrid, Madrid (Spain); Instituto de Fisica Teorica UAM-CSIC, Madrid (Spain); Univ. of California, Los Angeles, CA (United States)
  4. Univ. Autonoma de Madrid, Madrid (Spain); Instituto de Fisica Teorica UAM-CSIC, Madrid (Spain)
  5. Instituto de Fisica Teorica UAM-CSIC, Madrid (Spain); Campus de Cantoblanco, Madrid (Spain); Instituto de Astrofisica de Andalucia, Granada (Spain)
  6. Istituto Nazionale di Fisica Nucleare, Roma (Italy)
  7. New Mexico State Univ., Las Cruces, NM (United States)
  8. Lab. de Physique Theorique Univ. Paris-Sud, Orsay (France)
Publication Date:
Grant/Contract Number:
AC02-76SF00515
Type:
Accepted Manuscript
Journal Name:
Journal of Cosmology and Astroparticle Physics
Additional Journal Information:
Journal Volume: 2013; Journal Issue: 10; Journal ID: ISSN 1475-7516
Publisher:
Institute of Physics (IOP)
Research Org:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org:
USDOE
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; dark matter theory; dark matter experiments; gamma ray theory; gamma ray experiments
OSTI Identifier:
1356570

Gómez-Vargas, Germán A., Sánchez-Conde, Miguel A., Huh, Ji -Haeng, Peiró, Miguel, Prada, Francisco, Morselli, Aldo, Klypin, Anatoly, Cerdeño, David G., Mambrini, Yann, and Muñoz, Carlos. Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT. United States: N. p., Web. doi:10.1088/1475-7516/2013/10/029.
Gómez-Vargas, Germán A., Sánchez-Conde, Miguel A., Huh, Ji -Haeng, Peiró, Miguel, Prada, Francisco, Morselli, Aldo, Klypin, Anatoly, Cerdeño, David G., Mambrini, Yann, & Muñoz, Carlos. Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT. United States. doi:10.1088/1475-7516/2013/10/029.
Gómez-Vargas, Germán A., Sánchez-Conde, Miguel A., Huh, Ji -Haeng, Peiró, Miguel, Prada, Francisco, Morselli, Aldo, Klypin, Anatoly, Cerdeño, David G., Mambrini, Yann, and Muñoz, Carlos. 2013. "Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT". United States. doi:10.1088/1475-7516/2013/10/029. https://www.osti.gov/servlets/purl/1356570.
@article{osti_1356570,
title = {Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT},
author = {Gómez-Vargas, Germán A. and Sánchez-Conde, Miguel A. and Huh, Ji -Haeng and Peiró, Miguel and Prada, Francisco and Morselli, Aldo and Klypin, Anatoly and Cerdeño, David G. and Mambrini, Yann and Muñoz, Carlos},
abstractNote = {Here, we derive constraints on parameters of generic dark matter candidates by comparing theoretical predictions with the gamma-ray emission observed by the Fermi-LAT from the region around the Galactic Center. Our analysis is conservative since it simply requires that the expected dark matter signal does not exceed the observed emission. The constraints obtained in the likely case that the collapse of baryons to the Galactic Center is accompanied by the contraction of the dark matter are strong. In particular, we find that for bb¯ and τ+τ– or W+W– dark matter annihilation channels, the upper limits on the annihilation cross section imply that the thermal cross section is excluded for a Weakly Interacting Massive Particle (WIMP) mass smaller than about 700 and 500 GeV, respectively. For the μ+μ– channel, where the effect of the inverse Compton scattering is important, depending on models of the Galactic magnetic field the exclusion of the thermal cross-section is for a WIMP mass smaller than about 150 to 400 GeV. The upper limits on the annihilation cross section of dark matter particles obtained are two orders of magnitude stronger than without contraction. In the latter case our results are compatible with the upper limits from the Galactic halo analysis reported by the Fermi-LAT collaboration for the case in which the same conservative approach without modeling of the astrophysical background is employed.},
doi = {10.1088/1475-7516/2013/10/029},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 10,
volume = 2013,
place = {United States},
year = {2013},
month = {10}
}