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001     455158
005     20250716150118.0
024 7 _ |a 10.1088/1475-7516/2021/01/057
|2 doi
024 7 _ |a Acharyya:2020sbj
|2 INSPIRETeX
024 7 _ |a inspire:1809729
|2 inspire
024 7 _ |a 1475-7508
|2 ISSN
024 7 _ |a 1475-7516
|2 ISSN
024 7 _ |a arXiv:2007.16129
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2021-00966
|2 datacite_doi
024 7 _ |a altmetric:87045279
|2 altmetric
024 7 _ |a WOS:000620675000057
|2 WOS
024 7 _ |2 openalex
|a openalex:W3127784318
037 _ _ |a PUBDB-2021-00966
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2007.16129
|2 arXiv
100 1 _ |a Acharyya, A.
|b 0
245 _ _ |a Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
260 _ _ |a London
|c 2021
|b IOP
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1613472934_30362
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
520 _ _ |a We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray signal from pair-annihilating dark matter particles in the region around the Galactic centre. We find that CTA will open a new window of discovery potential, significantly extending the range of robustly testable models given a standard cuspy profile of the dark matter density distribution. Importantly, even for a cored profile, the projected sensitivity of CTA will be sufficient to probe various well-motivated models of thermally produced dark matter at the TeV scale. This is due to CTA's unprecedented sensitivity, angular and energy resolutions, and the planned observational strategy. The survey of the inner Galaxy will cover a much larger region than corresponding previous observational campaigns with imaging atmospheric Cherenkov telescopes. CTA will map with unprecedented precision the large-scale diffuse emission in high-energy gamma rays, constituting a background for dark matter searches for which we adopt state-of-the-art models based on current data. Throughout our analysis, we use up-to-date event reconstruction Monte Carlo tools developed by the CTA consortium, and pay special attention to quantifying the level of instrumental systematic uncertainties, as well as background template systematic errors, required to probe thermally produced dark matter at these energies.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|x 0
|f POF IV
588 _ _ |a Dataset connected to CrossRef, INSPIRE
650 _ 7 |a scale: TeV
|2 INSPIRE
650 _ 7 |a dark matter: density
|2 INSPIRE
650 _ 7 |a dark matter: heavy
|2 INSPIRE
650 _ 7 |a dark matter: annihilation
|2 INSPIRE
650 _ 7 |a Cherenkov counter: atmosphere
|2 INSPIRE
650 _ 7 |a Cherenkov Telescope Array
|2 INSPIRE
650 _ 7 |a sensitivity
|2 INSPIRE
650 _ 7 |a galaxy
|2 INSPIRE
650 _ 7 |a track data analysis
|2 INSPIRE
650 _ 7 |a cross section: thermal
|2 INSPIRE
650 _ 7 |a energy: flux
|2 INSPIRE
650 _ 7 |a cosmic background radiation
|2 INSPIRE
650 _ 7 |a correlation
|2 INSPIRE
650 _ 7 |a charged particle: relativistic
|2 INSPIRE
650 _ 7 |a spatial distribution
|2 INSPIRE
650 _ 7 |a p: cosmic radiation
|2 INSPIRE
650 _ 7 |a noise
|2 INSPIRE
650 _ 7 |a supersymmetry
|2 INSPIRE
650 _ 7 |a benchmark
|2 INSPIRE
650 _ 7 |a WIMP
|2 INSPIRE
650 _ 7 |a MAGIC
|2 INSPIRE
650 _ 7 |a HESS
|2 INSPIRE
650 _ 7 |a AGN
|2 INSPIRE
650 _ 7 |a VERITAS
|2 INSPIRE
650 _ 7 |a gamma ray
|2 INSPIRE
650 _ 7 |a satellite
|2 INSPIRE
650 _ 7 |a GLAST
|2 INSPIRE
650 _ 7 |a radiation: Cherenkov
|2 INSPIRE
650 _ 7 |a energy resolution
|2 INSPIRE
650 _ 7 |a Monte Carlo
|2 INSPIRE
650 _ 7 |a imaging
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)CTA-20150101
|5 EXP:(DE-H253)CTA-20150101
|e Cherenkov Telescope Array
|x 0
700 1 _ |a Adam, R.
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700 1 _ |a Adams, C.
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700 1 _ |a Agudo, I.
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700 1 _ |a Aguirre-Santaella, A.
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700 1 _ |a Alfaro, R.
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700 1 _ |a Alfaro, J.
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700 1 _ |a Alispach, C.
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700 1 _ |a Aloisio, R.
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700 1 _ |a Alves Batista, R.
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700 1 _ |a Amati, L.
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700 1 _ |a Ambrosi, G.
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700 1 _ |a Angüner, E. O.
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700 1 _ |a Antonelli, L. A.
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700 1 _ |a Aramo, C.
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700 1 _ |a Araudo, A.
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700 1 _ |a Armstrong, T.
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700 1 _ |a Arqueros, F.
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700 1 _ |a Asano, K.
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700 1 _ |a Balazs, C.
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700 1 _ |a Baquero Larriva, A.
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700 1 _ |a Barres de Almeida, U.
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700 1 _ |a Barrio, J. A.
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700 1 _ |a Berge, D.
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700 1 _ |a Berti, A.
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700 1 _ |a Beshley, V.
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700 1 _ |a Bregeon, J.
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700 1 _ |a Brill, A.
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700 1 _ |a Bringmann, Torsten
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|e Corresponding author
700 1 _ |a Brown, A. M.
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700 1 _ |a Chen, A.
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700 1 _ |a De Martino, D.
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700 1 _ |a de Souza, V.
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700 1 _ |a Ebr, J.
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700 1 _ |a Eckner, Christopher
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|e Corresponding author
700 1 _ |a Edwards, T. D. P.
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700 1 _ |a Ekoume, T. R. N.
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700 1 _ |a Fegan, S.
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700 1 _ |a Feng, Q.
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700 1 _ |a Ferrand, G.
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700 1 _ |a Gent, A.
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700 1 _ |a Ghalumyan, A.
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700 1 _ |a Gianotti, F.
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700 1 _ |a Giavitto, Gianluca
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700 1 _ |a Giglietto, N.
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700 1 _ |a Giuliani, A.
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700 1 _ |a Glicenstein, J.
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700 1 _ |a Goldoni, P.
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700 1 _ |a González, M. M.
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700 1 _ |a Gourgouliatos, K.
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700 1 _ |a Granot, J.
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700 1 _ |a Grasso, D.
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700 1 _ |a Green, J.
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700 1 _ |a Gueta, O.
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700 1 _ |a Gunji, S.
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700 1 _ |a Hassan Collado, Tarek
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700 1 _ |a Heller, M.
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700 1 _ |a Humensky, T. B.
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700 1 _ |a Iarlori, M.
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700 1 _ |a Inada, T.
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700 1 _ |a Iori, M.
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700 1 _ |a Janecek, P.
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700 1 _ |a Leone, F.
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700 1 _ |a Mazin, D.
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Marc 21