Journal Article/Contribution to a conference proceedings

PUBDB-2023-05449

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Indirect Dark-Matter Searches in VHE Gamma Rays with Legacy VERITAS Dwarf Spheroidal Observations

Tak, D. (Corresponding author)DESY* ; VERITAS Collaboration (Collaboration author)

2023
SISSA Trieste

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Please use a persistent id in citations: doi:10.22323/1.417.0197  doi:10.3204/PUBDB-2023-05449

Abstract: In the current cosmological theory, the existence and contribution of dark matter (DM) is inevitable. The weakly interacting massive particle (WIMP), expected mass in the range of tens of GeV to tens of TeV, is a DM candidate which can annihilate and/or decay into secondary particles, sequentially producing very-high-energy gamma rays (VHE; above 100 GeV). The Very Energetic Radiation Imaging Telescope Array System (VERITAS; sensitive to 100 GeV to 30 TeV gamma rays) is a ground-based VHE telescope array and can look for or detect gamma-ray signatures resulting from the annihilation of WIMPs. Since dwarf spheroidal galaxies (dSphs) are DM-rich regions, they are one of the best targets for studying indirect DM annihilation signatures. Compared to the previous DM search in dSphs, we significantly extend the observational dataset and improve our method of constraining the WIMP annihilation cross section by considering the dSph angular extension.

Keyword(s): gamma ray, VHE ; WIMP, annihilation ; detector, imaging ; dark matter, annihilation ; cross section, annihilation ; GeV ; VERITAS ; TeV ; signature ; galaxy

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Contributing Institute(s):

1. VERITAS (Z_VER)

Research Program(s):

1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)

Experiment(s):

1. Very Energetic Radiation Imaging Telescope Array System

Appears in the scientific report 2023

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Database coverage:
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