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Naslov:Expected exclusion limits to TeV dark matter from the perseus cluster with the Cherenkov Telescope Array
Avtorji:ID Adam, Rémi (Avtor)
ID Bhattacharyya, Saptashwa (Avtor)
ID Pérez Romero, Judit (Avtor)
ID Stanič, Samo (Avtor)
ID Vodeb, Veronika (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Živec, Miha (Avtor), et al.
Datoteke:.pdf ICRC2023_1436.pdf (1,33 MB)
MD5: 85FCD2B9500C8C0B840D946C0DB3E505
 
URL https://pos.sissa.it/444
 
URL https://pos.sissa.it/444/1436/pdf
 
Jezik:Angleški jezik
Vrsta gradiva:Neznano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:Clusters of galaxies are the largest gravitationally-bound structures in the Universe. They are composed of galaxies and gas (approximately 15% of the total mass) mostly dark matter (DM, accounts up to 85% of the total mass). If the DM is composed of Weakly Interacting Massive Particles (WIMPs), galaxy clusters represent one of the best targets to search for gamma-ray signals induced by the decay of WIMPs, with masses around the TeV scale. Due to its sensitivity and energy range of operation (from 20 GeV to 300 TeV), the Cherenkov Telescope Array (CTA) Observatory has a unique opportunity to test WIMPs with masses close to the unitarity limit. This will complement the searches for DM from other gamma-ray observatories as well as direct and collider experiments. The CTA Observatory is planning to search for gamma-ray emission, either its origin may be cosmic-ray (CR) or DM related, in the Perseus galaxy cluster during the first years of operation. In this poster, we will present the software created to perform the analysis using the ctools software and the corresponding results.
Ključne besede:Cherenkov Telescope Array, CTA, dark matter, standard model, dwarf spheroidal galaxies
Status publikacije:Objavljeno
Verzija publikacije:Objavljena publikacija
Datum objave:01.01.2023
Leto izida:2023
Št. strani:str. 1-16
PID:20.500.12556/RUNG-8461-bc21f8eb-14f7-a98e-f6e6-76539a870b8b Novo okno
COBISS.SI-ID:165858563 Novo okno
UDK:539.1
ISSN pri članku:1824-8039
NUK URN:URN:SI:UNG:REP:TL57RWVH
Datum objave v RUNG:26.09.2023
Število ogledov:2099
Število prenosov:10
Metapodatki:XML DC-XML DC-RDF
:
ADAM, Rémi, BHATTACHARYYA, Saptashwa, PÉREZ ROMERO, Judit, STANIČ, Samo, VODEB, Veronika, VOROBIOV, Serguei, ZAVRTANIK, Danilo, ZAVRTANIK, Marko in ŽIVEC, Miha, 2023, Expected exclusion limits to TeV dark matter from the perseus cluster with the Cherenkov Telescope Array. V : 38th International Cosmic Ray Conference [also] ICRC2023 [na spletu]. Objavljeni znanstveni prispevek na konferenci. 2023. p. 1–16. [Dostopano 4 april 2025]. Pridobljeno s: https://repozitorij.ung.si/IzpisGradiva.php?lang=slv&id=8461
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Gradivo je del zbornika

Naslov:38th International Cosmic Ray Conference [also] ICRC2023
COBISS.SI-ID:162195971 Novo okno

Gradivo je del revije

Naslov:Proceedings of science
Skrajšan naslov:Pos proc. sci.
Založnik:Sissa
ISSN:1824-8039
COBISS.SI-ID:20239655 Novo okno

Gradivo je financirano iz projekta

Financer:ARRS - Agencija za raziskovalno dejavnost Republike Slovenije
Številka projekta:P1-0031
Naslov:Večglasniška astrofizika

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Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by-nc-nd/4.0/deed.sl
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