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Naslov:Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation
Avtorji:ID Abdalla, H. (Avtor)
ID Abe, H. (Avtor)
ID Acero, Fabio (Avtor)
ID Acharyya, A. (Avtor)
ID Adam, R. (Avtor)
ID Eckner, Christopher (Avtor)
ID Stanič, Samo (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zaharijas, Gabrijela (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Živec, Miha (Avtor)
Datoteke:URL https://iopscience.iop.org/article/10.1088/1475-7516/2021/02/048/pdf
 
Jezik:Angleški jezik
Vrsta gradiva:Neznano
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:UNG - Univerza v Novi Gorici
Opis:The Cherenkov Telescope Array (CTA), the new-generation ground-based observatory for γ astronomy, provides unique capabilities to address significant open questions in astrophysics, cosmology, and fundamental physics. We study some of the salient areas of γ cosmology that can be explored as part of the Key Science Projects of CTA, through simulated observations of active galactic nuclei (AGN) and of their relativistic jets. Observations of AGN with CTA will enable a measurement of γ absorption on the extragalactic background light with a statistical uncertainty below 15% up to a redshift z=2 and to constrain or detect γ halos up to intergalactic-magnetic-field strengths of at least 0.3 pG . Extragalactic observations with CTA also show promising potential to probe physics beyond the Standard Model. The best limits on Lorentz invariance violation from γ astronomy will be improved by a factor of at least two to three. CTA will also probe the parameter space in which axion-like particles could constitute a significant fraction, if not all, of dark matter. We conclude on the synergies between CTA and other upcoming facilities that will foster the growth of γ cosmology.
Ključne besede:Cherenkov Telescope Array, active galactic nuclei, gamma-ray experiments, axions, extragalactic magnetic fields
Leto izida:2021
Št. strani:str. 1-63
Številčenje:Vol. 2021, no. 2
PID:20.500.12556/RUNG-6314 Novo okno
COBISS.SI-ID:53539843 Novo okno
UDK:52
ISSN pri članku:1475-7516
DOI:10.1088/1475-7516/2021/02/048 Novo okno
NUK URN:URN:SI:UNG:REP:OS63PKZY
Datum objave v RUNG:02.03.2021
Število ogledov:2427
Število prenosov:72
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Gradivo je del revije

Naslov:Journal of cosmology and astroparticle physics
Založnik:Institute of Physics Pub.
ISSN:1475-7516
COBISS.SI-ID:389627 Novo okno

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