Unidentified gamma-ray sources as targets for indirect dark matter detection with the Fermi -Large Area Telescope
Abstract
We report that one of the predictions of the ΛCDM cosmological framework is the hierarchical formation of structure, giving rise to dark matter (DM) halos and subhalos. When the latter are massive enough they retain gas (i.e., baryons) and become visible. This is the case of the dwarf satellite galaxies in the Milky Way (MW) . Below a certain mass, halos may not accumulate significant amounts of baryons and remain completely dark. However, if DM particles are Weakly Interacting Massive Particles (WIMPs), we expect them to annihilate in subhalos, producing gamma rays which can be detected with the Fermi satellite. Using the three most recent point-source Fermi Large Area Telescope (LAT) catalogs (3FGL, 2FHL and 3FHL), we search for DM subhalo candidates among the unidentified sources, i.e., sources with no firm association to a known astrophysical object. We apply several selection criteria based on the expected properties of the DM-induced emission from subhalos, which allow us to significantly reduce the list of potential candidates. Then, by characterizing the minimum detection flux of the instrument and comparing our sample to predictions from the Via Lactea II (VL-II) N-body cosmological simulation, we place conservative and robust constraints on the $$\langle$$σ v$$\rangle$$-mDM parameter space. For annihilation via the τ+τ- channel, we put an upper limit of 4 × 10-26 (5 × 10-25) cm3s-1 for a mass of 10 (100) GeV . A critical improvement over previous treatments is the repopulation we made to include low-mass subhalos below the VL\nobreakdash-II mass resolution. Finally, with more advanced subhalo candidate filtering the sensitivity reach of our method can potentially improve these constraints by a factor 3 (2) for τ+τ- (b$$\bar{b}$$) channel.
- Authors:
-
- Universidad Autónoma de Madrid (Spain)
- Universidad Complutense de Madrid (Spain)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); The Catholic Univ. of America, Washington, DC (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland Baltimore County (UMBC), Baltimore, MD (United States)
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1546970
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2019; Journal Issue: 07; Journal ID: ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Coronado-Blázquez, Javier, Sánchez-Conde, Miguel A., Domínguez, Alberto, Aguirre-Santaella, Alejandra, Mauro, Mattia Di, Mirabal, Néstor, Nieto, Daniel, and Charles, Eric. Unidentified gamma-ray sources as targets for indirect dark matter detection with the Fermi -Large Area Telescope. United States: N. p., 2019.
Web. doi:10.1088/1475-7516/2019/07/020.
Coronado-Blázquez, Javier, Sánchez-Conde, Miguel A., Domínguez, Alberto, Aguirre-Santaella, Alejandra, Mauro, Mattia Di, Mirabal, Néstor, Nieto, Daniel, & Charles, Eric. Unidentified gamma-ray sources as targets for indirect dark matter detection with the Fermi -Large Area Telescope. United States. https://doi.org/10.1088/1475-7516/2019/07/020
Coronado-Blázquez, Javier, Sánchez-Conde, Miguel A., Domínguez, Alberto, Aguirre-Santaella, Alejandra, Mauro, Mattia Di, Mirabal, Néstor, Nieto, Daniel, and Charles, Eric. Fri .
"Unidentified gamma-ray sources as targets for indirect dark matter detection with the Fermi -Large Area Telescope". United States. https://doi.org/10.1088/1475-7516/2019/07/020. https://www.osti.gov/servlets/purl/1546970.
@article{osti_1546970,
title = {Unidentified gamma-ray sources as targets for indirect dark matter detection with the Fermi -Large Area Telescope},
author = {Coronado-Blázquez, Javier and Sánchez-Conde, Miguel A. and Domínguez, Alberto and Aguirre-Santaella, Alejandra and Mauro, Mattia Di and Mirabal, Néstor and Nieto, Daniel and Charles, Eric},
abstractNote = {We report that one of the predictions of the ΛCDM cosmological framework is the hierarchical formation of structure, giving rise to dark matter (DM) halos and subhalos. When the latter are massive enough they retain gas (i.e., baryons) and become visible. This is the case of the dwarf satellite galaxies in the Milky Way (MW) . Below a certain mass, halos may not accumulate significant amounts of baryons and remain completely dark. However, if DM particles are Weakly Interacting Massive Particles (WIMPs), we expect them to annihilate in subhalos, producing gamma rays which can be detected with the Fermi satellite. Using the three most recent point-source Fermi Large Area Telescope (LAT) catalogs (3FGL, 2FHL and 3FHL), we search for DM subhalo candidates among the unidentified sources, i.e., sources with no firm association to a known astrophysical object. We apply several selection criteria based on the expected properties of the DM-induced emission from subhalos, which allow us to significantly reduce the list of potential candidates. Then, by characterizing the minimum detection flux of the instrument and comparing our sample to predictions from the Via Lactea II (VL-II) N-body cosmological simulation, we place conservative and robust constraints on the $\langle$σ v$\rangle$-mDM parameter space. For annihilation via the τ+τ- channel, we put an upper limit of 4 × 10-26 (5 × 10-25) cm3s-1 for a mass of 10 (100) GeV . A critical improvement over previous treatments is the repopulation we made to include low-mass subhalos below the VL\nobreakdash-II mass resolution. Finally, with more advanced subhalo candidate filtering the sensitivity reach of our method can potentially improve these constraints by a factor 3 (2) for τ+τ- (b$\bar{b}$) channel.},
doi = {10.1088/1475-7516/2019/07/020},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 07,
volume = 2019,
place = {United States},
year = {Fri Jul 12 00:00:00 EDT 2019},
month = {Fri Jul 12 00:00:00 EDT 2019}
}
Web of Science
Figures / Tables:
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The second catalog of flaring gamma-ray sources from the Fermi All-sky Variability Analysis
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3FGLzoo. Classifying 3FGL Unassociated Fermi-LAT Gamma-ray Sources by Artificial Neural Networks
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WIMP dark matter candidates and searches - current status and future prospects
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Disruption of Dark Matter Substructure: Fact or Fiction?
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Optical spectroscopic survey of a sample of Unidentified Fermi objects
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- arXiv
Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar
text, January 2018
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- arXiv
Optical Spectroscopic Observations of Gamma-Ray Blazar Candidates. VII. Follow-up Campaign in the Southern Hemisphere
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HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
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Earth-mass dark-matter haloes as the first structures in the early Universe
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What mass are the smallest protohalos?
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Effects of cold dark matter decoupling and pair annihilation on cosmological perturbations
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Observability of Gamma Rays from Dark Matter Neutralino Annihilations in the Milky Way Halo
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Particle Dark Matter: Evidence, Candidates and Constraints
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Optical spectroscopic observations of gamma-ray blazar candidates. VII. Follow-up campaign in the southern hemisphere
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Multi-Wavelength Observations of 3fgl J2039.6–5618: a Candidate Redback Millisecond Pulsar
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Optical Spectroscopic Survey of a Sample of Unidentified Fermi Objects
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Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar
text, January 2018
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Works referencing / citing this record:
Spectral and spatial analysis of the dark matter subhalo candidates among Fermi Large Area Telescope unidentified sources
journal, November 2019
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- Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 11
Gamma-Ray Sensitivity to Dark Matter Subhalo Modelling at High Latitudes
journal, November 2019
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- Galaxies, Vol. 7, Issue 4
Constraints to Dark Matter Annihilation from High-Latitude HAWC Unidentified Sources
journal, December 2019
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Fermi Large Area Telescope Fourth Source Catalog
journal, March 2020
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Fermi Large Area Telescope Fourth Source Catalog
text, January 2020
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- Deutsches Elektronen-Synchrotron, DESY, Hamburg
Spectral and spatial analysis of the dark matter subhalo candidates among Fermi Large Area Telescope unidentified sources
text, January 2019
- Coronado-Blázquez, Javier; Sánchez-Conde, Miguel A.; Di Mauro, Mattia
- arXiv
Constraints to dark matter annihilation from high-latitude HAWC unidentified sources
text, January 2020
- Coronado-Blazquez, Javier; Sanchez-Conde, Miguel A.
- arXiv
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