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Naslov:Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
Avtorji:ID Eckner, Christopher (Avtor)
ID Bhattacharyya, Saptashwa (Avtor)
ID MARČUN, Barbara (Avtor)
ID Pérez Romero, Judit (Avtor)
ID Stanič, Samo (Avtor)
ID Vodeb, Veronika (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zaharijas, Gabrijela (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Živec, Miha (Avtor), et al.
Datoteke:.pdf ICRC2021_547.pdf (2,47 MB)
MD5: 3612E7631E2AE49FBA1E9E456657F300
 
URL https://pos.sissa.it/395/
 
URL https://pos.sissa.it/395/547/pdf
 
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:High-energy gamma rays are promising tools to constrain or reveal the nature of dark matter, in particular Weakly Interacting Massive Particles. Being well into its pre-construction phase, the Cherenkov Telescope Array (CTA) will soon probe the sky in the 20 GeV - 300 TeV energy range. Thanks to its improved energy and angular resolutions as well as significantly larger e˙ective area when compared to the current generation of Cherenkov telescopes, CTA is expected to probe heavier dark matter, with unprecedented sensitivity, reaching the thermal annihilation cross-section at 1 TeV. This talk will summarise the planned dark matter search strategies with CTA, focusing on the signal from the Galactic centre. As observed with the Fermi LAT at lower energies, this region is rather complex and CTA will be the first ground-based observatory sensitive to the large scale di˙use astrophysical emission from that region. We report on the collaboration e˙ort to study the impact of such extended astrophysical backgrounds on the dark matter search, based on Fermi-LAT data in order to guide our observational strategies, taking into account various sources of systematic uncertainty.
Ključne besede:high-energy gamma rays, Cherenkov Telescope Array, dark matter, galactic centre
Status publikacije:Objavljeno
Leto izida:2021
PID:20.500.12556/RUNG-8419 Novo okno
COBISS.SI-ID:164768515 Novo okno
NUK URN:URN:SI:UNG:REP:ZPMCEWRG
Datum objave v RUNG:18.09.2023
Število ogledov:830
Število prenosov:8
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Vaša ocena:Ocenjevanje je dovoljeno samo prijavljenim uporabnikom.
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Gradivo je del monografije

Naslov:37th International Cosmic Ray Conference : ICRC2021
Kraj izida:Trst, Italija
Leto izida:2021

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Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
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