التفاصيل البيبلوغرافية
| العنوان: |
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre |
| المؤلفون: |
Truzzi S, Jamrozy M, Prouza M, Patricelli B, Vink J, Hassan T, Bertucci B, Araudo A, Bernardini E, Lopez A, Grasso D, Zech A, Bulgarelli A, Bocchino F, Taylor L, Suomijarvi T, Bordas P, Vallage B, Peixoto CJT, Straumann U, Humensky TB, Delgado C, Dominguez A, Persic M, Perez-Romero J, Foffano L, Anguner EO, Batista RA, Sergijenko O, Russo F, Striskovic J, Cascone E, Greus FS, Mukherjee R, Okumura A, Zdziarski AA, Martinez G, Hutten M, Marculewicz M, Arbeletche LB, Sol H, Laporte P, Prado RR, Tosti L, Benito M, Cotter G, Marti J, Beck G, Green J, Puhlhofer G, Sciacca E, Nikolajuk M, Inoue S, Eckner C, Beshley V, Mallamaci M, Iarlori M, Blanch O, Lombardi S, Cameron R, Travnicek P, Mangano S, Fioretti V, Giler AGD, Bernlohr K, Amati L, Moralejo A, Giuliani A, Zaharijas G, Daniel MK, Carosi R, Zhdanov VI, Niemiec J, Maier G, Luque-Escamilla PL, Alfaro R, Orlando E, Falceta-Goncalves D, Stolarczyk T, Zanin R, Asano K, Vagelli V, Coronado-Blazquez J, Vercellone S, Tothill N, van Eldik C, Ramirez JCR, Iocco F, Bruno P, Chiaro G, Dmytriiev A, Markoff S, Saturni FG, Martinez M, Lopez-Coto R, Fiandrini E, Servillat M, Fegan S, Elsasser D, Sliusar V, Kerszberg D, Wilhelmi ED, De Lotto B, Mizuno T, Paredes JM, Recchia S, Bregeon J, Biasuzzi B, Yanagita S, Gunji S, Bringmann T, Contreras JL, Caproni A, Evoli C, Rodriguez J, Moderski R, dos Anjos RD, Pintore F, Mariotti M, Williams DA, Tokanai F, Fornieri O, Zavrtanik M, Mandat D, Richtler T, Vandenbroucke J, Di Venere L, Palatiello M, Starling R, Prokoph H, Leone F, Orlandini M, Horan D, Silk J, Ribo M, Colak M, Franco FJ, Kissmann R, Pantaleo FR, Rudak B, Ribeiro D, Bozhilov V, Przybilski H, Cassol F, Pe'er A, Santos-Lima R, Petruk O, Pareschi G, Oya I, Seweryn K, Vallania P, Casanova S, Holder J, Vitale V, Aramo C, Lopez M, Kherlakian MC, Doro M, Capuzzo-Dolcetta R, Shellard RC, Iori M, Pumo ML, Pavletic L, Alfaro J, Ong RA, Vuillaume T, Ekoume TRN, Ebr J, Cadena SH, Ambrosi G, Conte F, Romano P, Orito R, Gammaldi V, Orienti M, Santander M, Glicenstein J, Gaggero D, Gnatyk R, Santos EM, Ostrowski M, Gonzalez MM, Reisenegger A, Wiemann R, Rosado J, Sharma P, Dal Pino EMD, Maurin G, Rico J, Benbow W, Martinez-Huerta H, Maggio C, Romeo G, Halim A, Rojas G, Yang L, Garcia E, Razzaque S, De Martino D, Dazzi F, Fedorova E, Mirzoyan R, Galaz G, Hrabovsky M, Inada T, Jin W, Gueta O, Berge D, Chernyakova M, Vovk I, della Volpe D, Nakamori T, Kobayashi Y, Ballester O, Prandini E, de Almeida UB, Chadwick P, Conforti V, Miener T, Hughes G, Brill A, Rieger F, Biland A, Cerruti M, Manganaro M, Barkov M, Pfrang K, Miranda DM, Karukes E, Watson J, Damone LA, Orlando S, Wischnewski R, Depaoli D, Molina E, Seglar-Arroyo M, de Oliveira MAL, Tavecchio F, Donini A, Caraveo P, Horandel J, Stamerra A, Weniger C, Sadeh I, Coniglione R, Carosi A, Fernandez GR, Longo F, Fiori M, Noda K, Quirrenbach A, Hovatta T, Di Pierro F, Agudo I, Pillera R, Montaruli T, Swierk P, Zaric D, Kazanas D, Loporchio S, Leto G, Kohri K, Chudoba J, Piatteli P, Brun P, Sanuy A, Mohrmann L, Armstrong T, Viana A, Lamanna G, Siqueira C, Pecimotika M, Boisson C, Piano G, Manico G, Tibaldo L, Hrupec D, Varner GS, Burtovoi A, Vassiliev V, Nosek D, Costantini H, Aloisio R, Katarzynski K, Chaty S, Antonelli LA, Ascasibar Y, Hatlen ES, Lindfors E, Gianotti F, Catalani F, Kushida J, Walter R, Bottacini E, Mbarubucyeye JD, Costa A, Ventura S, Parmiggiani N, Zakaria AA, Tejedor LA, Giglietto N, Pilszyk B, Yoshikoshi T, Shalchi A, Miranda JM, Feng Q, Sanchez D, Acharyya A, Teshima M, Ninci D, Miceli M, D'Ai A, Rowell G, Knodlseder J, Sano H, Martins VB, Granot J, Bastieri D, Sangiorgi P, Zavrtanik D, Zacharias M, Adam R, Cristofari P, Filipovic M, Brown AM, Pietropaolo E, Lenain J, Ferrara G, Ghalumyan A, Buscemi M, Garczarczyk M, D'Ammando A, White M, Bosnjak Z, Salina G, Biteau J, Will M, Nozaki S, Minev M, Rhode W, Sokolenko A, Testa V, Komin N, Adams C, De Angelis A, Zivec M, Arqueros F, Larriva AB, De Palma F, Tjus JB, Hnatyk B, Siejkowski H, Safi-Harb S, Bissaldi E, de Almeida RMN, Gourgouliatos K, Becerra J, Ferrand G, White R, Lapington J, Ohira Y, Hofmann W, Raino S, De Caprio V, Sawangwit U, Scuderi S, Morcuende-Parrilla D, Mundell C, Hiroshima N, Marquez P, Barrio JA, Zechlin H, Poireau V, Vigorito CF, Jurysek J, Meyer M, Grillo A, Reimer O, Sarkar S, Jouvin L, Alispach C, Giordano F, Fukami S, Morselli A, Schwanke U, Cauz D, Tosti G, Vorobiov S, Mach E, Oka T, Brun F, Ashley M, Nieto D, Wierzcholska A, Martinez O, Giavitto G, Lohse T, Verna G, Rizi V, Ohtani Y, Suda Y, Zampieri L, Tonev D, Nagai A, Janecek P, Vergani S, Heller M, Spencer S, Giarrusso M, Rando R, Pohl M, Pagano I, Fontaine G, Fukui Y, Ohishi M, Horvath P, Chen A, Schussler F, Vecchi M, Capasso M, Chikawa M, de Souza V, Balazs C, Diebold S, Stanic S, Principe G, Goldoni P, Acosta MV, Renier Y, Blazek J, Pagliaro A, Edwards TDP, Kubo H, Di Girolamo T, Mazin D, Berti A, Rinchiuso L, Aguirre-Santaella A, Fiasson A, Gascon D, Nemmen R, Wagner SJ, Queiroz F, Sanchez-Conde M, Burton M, Prast J, Chiavassa A, Gent A, Mode B |
| المساهمون: |
Suomen ESO-keskus, yhteiset, Finnish Centre for Astronomy with ESO - FINCA, 2609700 |
| بيانات النشر: |
IOP PUBLISHING LTD
United Kingdom
Britannia
GB |
| سنة النشر: |
2022 |
| المجموعة: |
University of Turku: UTUPub / Turun yliopisto |
| الوصف: |
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. |
| نوع الوثيقة: |
other/unknown material |
| اللغة: |
English |
| تدمد: |
1475-7516 |
| العلاقة: |
ARTN 057; Journal of Cosmology and Astroparticle Physics; https://www.utupub.fi/handle/10024/172745Test; https://iopscience.iop.org/article/10.1088/1475-7516/2021/01/057Test; URN:NBN:fi-fe2021042827549 |
| DOI: |
10.1088/1475-7516/2021/01/057 |
| الإتاحة: |
https://www.utupub.fi/handle/10024/172745Test |
| رقم الانضمام: |
edsbas.802332BA |
| قاعدة البيانات: |
BASE |
