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@ARTICLE{Acharyya:455158,
author = {Acharyya, A. and Adam, R. and Adams, C. and Agudo, I. and
Aguirre-Santaella, A. and Alfaro, R. and Alfaro, J. and
Alispach, C. and Aloisio, R. and Alves Batista, R. and
Amati, L. and Ambrosi, G. and Angüner, E. O. and Antonelli,
L. A. and Aramo, C. and Araudo, A. and Armstrong, T. and
Arqueros, F. and Asano, K. and Ascasíbar, Y. and Ashley, M.
and Balazs, C. and Ballester, O. and Baquero Larriva, A. and
Barbosa Martins, Victor and Barkov, M. and Barres de
Almeida, U. and Barrio, J. A. and Bastieri, D. and Becerra,
J. and Beck, G. and Becker Tjus, J. and Benbow, W. and
Benito, M. and Berge, D. and Bernardini, Elisa and
Bernlöhr, K. and Berti, A. and Bertucci, B. and Beshley, V.
and Biasuzzi, B. and Biland, A. and Bissaldi, E. and Biteau,
J. and Blanch, O. and Blazek, J. and Bocchino, F. and
Boisson, C. and Bonneau Arbeletche, L. and Bordas, P. and
Bosnjak, Z. and Bottacini, E. and Bozhilov, V. and Bregeon,
J. and Brill, A. and Bringmann, Torsten and Brown, A. M. and
Brun, P. and Brun, F. and Bruno, P. and Bulgarelli, A. and
Burton, M. and Burtovoi, A. and Buscemi, M. and Cameron, R.
and Capasso, M. and Caproni, A. and Capuzzo-Dolcetta, R. and
Caraveo, P. and Carosi, R. and Carosi, A. and Casanova, S.
and Cascone, E. and Cassol, F. and Catalani, F. and Cauz, D.
and Cerruti, M. and Chadwick, P. and Chaty, S. and Chen, A.
and Chernyakova, M. and Chiaro, G. and Chiavassa, A. and
Chikawa, M. and Chudoba, J. and Çolak, M. and Conforti, V.
and Coniglione, R. and Conte, F. and Contreras, J. L. and
Coronado-Blazquez, J. and Costa, A. and Costantini, H. and
Cotter, G. and Cristofari, P. and D'Aì, A. and D'Ammando,
F. and Damone, L. A. and Daniel, M. K. and Dazzi, F. and De
Angelis, A. and De Caprio, V. and de Cássia dos Anjos, R.
and de Gouveia Dal Pino, E. M. and De Lotto, B. and De
Martino, D. and de Oña Wilhelmi, E. and De Palma, F. and de
Souza, V. and Delgado, C. and Delgado Giler, A. G. and della
Volpe, D. and Depaoli, D. and Di Girolamo, T. and Di Pierro,
F. and Di Venere, L. and Diebold, S. and Dmytriiev, A. and
Domínguez, A. and Donini, A. and Doro, M. and Ebr, J. and
Eckner, Christopher and Edwards, T. D. P. and Ekoume, T. R.
N. and Elsässer, D. and Evoli, C. and Falceta-Goncalves, D.
and Fedorova, E. and Fegan, S. and Feng, Q. and Ferrand, G.
and Ferrara, G. and Fiandrini, E. and Fiasson, A. and
Filipovic, M. and Fioretti, V. and Fiori, M. and Foffano, L.
and Fontaine, G. and Fornieri, O. and Franco, F. J. and
Fukami, S. and Fukui, Y. and Gaggero, D. and Galaz, G. and
Gammaldi, V. and Garcia, E. and Garczarczyk, Markus and
Gascon, D. and Gent, A. and Ghalumyan, A. and Gianotti, F.
and Giarrusso, M. and Giavitto, Gianluca and Giglietto, N.
and Giordano, F. and Giuliani, A. and Glicenstein, J. and
Gnatyk, R. and Goldoni, P. and González, M. M. and
Gourgouliatos, K. and Granot, J. and Grasso, D. and Green,
J. and Grillo, A. and Gueta, O. and Gunji, S. and Halim, A.
and Hassan Collado, Tarek and Heller, M. and Hernández
Cadena, S. and Hiroshima, N. and Hnatyk, B. and Hofmann, W.
and Holder, J. and Horan, D. and Hörandel, J. and Horvath,
P. and Hovatta, T. and Hrabovsky, M. and Hrupec, D. and
Hughes, G. and Humensky, T. B. and Hütten, M. and Iarlori,
M. and Inada, T. and Inoue, S. and Iocco, F. and Iori, M.
and Jamrozy, M. and Janecek, P. and Jin, W. and Jouvin, L.
and Jurysek, J. and Karukes, E. and Katarzyński, K. and
Kazanas, D. and Kerszberg, D. and Kherlakian, M. C. and
Kissmann, R. and Knödlseder, J. and Kobayashi, Y. and
Kohri, K. and Komin, N. and Kubo, H. and Kushida, J. and
Lamanna, G. and Lapington, J. and Laporte, P. and Leigui de
Oliveira, M. A. and Lenain, J. and Leone, F. and Leto, G.
and Lindfors, E. and Lohse, T. and Lombardi, S. and Longo,
F. and Lopez, A. and López, M. and López-Coto, R. and
Loporchio, S. and Luque-Escamilla, P. L. and Mach, E. and
Maggio, C. and Maier, G. and Mallamaci, M. and Malta Nunes
de Almeida, R. and Mandat, D. and Manganaro, M. and Mangano,
S. and Manicò, G. and Marculewicz, M. and Mariotti, M. and
Markoff, S. and Marquez, P. and Martí, J. and Martinez, O.
and Martínez, M. and Martínez, G. and Martínez-Huerta, H.
and Maurin, G. and Mazin, D. and Mbarubucyeye, Jean
Damascene and Medina Miranda, D. and Meyer, M. and Miceli,
M. and Miener, T. and Minev, M. and Miranda, J. M. and
Mirzoyan, R. and Mizuno, T. and Mode, B. and Moderski, R.
and Mohrmann, L. and Molina, E. and Montaruli, T. and
Moralejo, A. and Morcuende-Parrilla, D. and Morselli, A. and
Mukherjee, R. and Mundell, C. and Nagai, A. and Nakamori, T.
and Nemmen, R. and Niemiec, J. and Nieto, D. and Nikołajuk,
M. and Ninci, D. and Noda, K. and Nosek, D. and Nozaki, S.
and Ohira, Y. and Ohishi, M. and Ohtani, Y. and Oka, T. and
Okumura, A. and Ong, R. A. and Orienti, M. and Orito, R. and
Orlandini, M. and Orlando, S. and Orlando, E. and Ostrowski,
M. and Oya, I. and Pagano, I. and Pagliaro, A. and
Palatiello, M. and Pantaleo, F. R. and Paredes, J. M. and
Pareschi, G. and Parmiggiani, N. and Patricelli, B. and
Pavletić, L. and Pe'er, A. and Pecimotika, M. and
Pérez-Romero, J. and Persic, M. and Petruk, O. and Pfrang,
Konstantin Johannes and Piano, G. and Piatteli, P. and
Pietropaolo, E. and Pillera, R. and Pilszyk, B. and Pintore,
F. and Pohl, M. and Poireau, V. and Prado, R. R. and
Prandini, E. and Prast, J. and Principe, G. and Prokoph,
Heike and Prouza, M. and Przybilski, H. and Pühlhofer, G.
and Pumo, M. L. and Queiroz, F. and Quirrenbach, A. and
Rainò, S. and Rando, R. and Razzaque, S. and Recchia, S.
and Reimer, O. and Reisenegger, A. and Renier, Y. and Rhode,
W. and Ribeiro, D. and Ribó, M. and Richtler, T. and Rico,
J. and Rieger, F. and Rinchiuso, L. and Rizi, V. and
Rodriguez, J. and Rodriguez Fernandez, G. and Rodriguez
Ramirez, J. C. and Rojas, G. and Romano, P. and Romeo, G.
and Rosado, J. and Rowell, G. and Rudak, B. and Russo, F.
and Sadeh, I. and Sæther Hatlen, E. and Safi-Harb, S. and
Salesa Greus, F. and Salina, G. and Sanchez, D. and
Sánchez-Conde, M. and Sangiorgi, P. and Sano, H. and
Santander, M. and Santos, E. M. and Santos-Lima, R. and
Sanuy, A. and Sarkar, S. and Saturni, F. G. and Sawangwit,
U. and Schussler, F. and Schwanke, U. and Sciacca, E. and
Scuderi, S. and Seglar-Arroyo, M. and Sergijenko, O. and
Servillat, M. and Seweryn, K. and Shalchi, A. and Sharma, P.
and Shellard, R. C. and Siejkowski, H. and Silk, J. and
Siqueira, C. and Sliusar, V. and Słowikowska, A. and
Sokolenko, A. and Sol, H. and Spencer, S. and Stamerra, A.
and Stanič, S. and Starling, R. and Stolarczyk, T. and
Straumann, U. and Strišković, J. and Suda, Y. and
Suomijarvi, T. and Świerk, P. and Tavecchio, F. and Taylor,
L. and Tejedor, L. A. and Teshima, M. and Testa, V. and
Tibaldo, L. and Todero Peixoto, C. J. and Tokanai, F. and
Tonev, D. and Tosti, G. and Tosti, L. and Tothill, N. and
Truzzi, S. and Travnicek, P. and Vagelli, V. and Vallage, B.
and Vallania, P. and van Eldik, C. and Vandenbroucke, J. and
Varner, G. S. and Vassiliev, V. and Vázquez Acosta, M. and
Vecchi, M. and Ventura, S. and Vercellone, S. and Vergani,
S. and Verna, G. and Viana, A. and Vigorito, C. F. and Vink,
J. and Vitale, V. and Vorobiov, S. and Vovk, I. and
Vuillaume, T. and Wagner, S. J. and Walter, R. and Watson,
Jason John and Weniger, C. and White, R. and White, M. and
Wiemann, R. and Wierzcholska, A. and Will, M. and Williams,
D. A. and Wischnewski, Ralf and Yanagita, S. and Yang, L.
and Yoshikoshi, T. and Zacharias, M. and Zaharijas,
Gabrijela and Zakaria, A. A. and Zampieri, L. and Zanin, R.
and Zaric, D. and Zavrtanik, M. and Zavrtanik, D. and
Zdziarski, A. A. and Zech, A. and Zechlin, H. and Zehrer, L.
and Zhdanov$^ and Živec, M. and {CTA Collaboration}},
title = {{S}ensitivity of the {C}herenkov {T}elescope {A}rray to a
dark matter signal from the {G}alactic centre},
journal = {Journal of cosmology and astroparticle physics},
volume = {01},
number = {01},
issn = {1475-7516},
address = {London},
publisher = {IOP},
reportid = {PUBDB-2021-00966, arXiv:2007.16129},
pages = {057 (1-62)},
year = {2021},
abstract = {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.},
keywords = {scale: TeV (INSPIRE) / dark matter: density (INSPIRE) /
dark matter: heavy (INSPIRE) / dark matter: annihilation
(INSPIRE) / Cherenkov counter: atmosphere (INSPIRE) /
Cherenkov Telescope Array (INSPIRE) / sensitivity (INSPIRE)
/ galaxy (INSPIRE) / track data analysis (INSPIRE) / cross
section: thermal (INSPIRE) / energy: flux (INSPIRE) / cosmic
background radiation (INSPIRE) / correlation (INSPIRE) /
charged particle: relativistic (INSPIRE) / spatial
distribution (INSPIRE) / p: cosmic radiation (INSPIRE) /
noise (INSPIRE) / supersymmetry (INSPIRE) / benchmark
(INSPIRE) / WIMP (INSPIRE) / MAGIC (INSPIRE) / HESS
(INSPIRE) / AGN (INSPIRE) / VERITAS (INSPIRE) / gamma ray
(INSPIRE) / satellite (INSPIRE) / GLAST (INSPIRE) /
radiation: Cherenkov (INSPIRE) / energy resolution (INSPIRE)
/ Monte Carlo (INSPIRE) / imaging (INSPIRE)},
cin = {ZEU-CTA},
ddc = {530},
cid = {I:(DE-H253)ZEU-CTA-20120731},
pnm = {613 - Matter and Radiation from the Universe (POF4-613)},
pid = {G:(DE-HGF)POF4-613},
experiment = {EXP:(DE-H253)CTA-20150101},
typ = {PUB:(DE-HGF)16},
eprint = {2007.16129},
howpublished = {arXiv:2007.16129},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2007.16129;\%\%$},
UT = {WOS:000620675000057},
doi = {10.1088/1475-7516/2021/01/057},
url = {https://bib-pubdb1.desy.de/record/455158},
}
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