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Naslov:Probing extreme environments with the Cherenkov Telescope Array
Avtorji:ID Boisson, C. (Avtor)
ID Brown, Anthony M. (Avtor)
ID Burtovoi, A. (Avtor)
ID Cerruti, M. (Avtor)
ID Chernyakova, M. (Avtor)
ID Hassan, T. (Avtor)
ID Lenain, J.-P. (Avtor)
ID Manganaro, Marina (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zavrtanik, Danilo (Avtor)
Datoteke:.05971 RAZ_Boisson_C._2021.05971 (7,40 MB)
MD5: C2236DBF357DC4EC014157BFDE672B4D
 
URL https://arxiv.org/pdf/2106.05971
 
URL https://arxiv.org/html/2106.08952v1/
 
Jezik:Angleški jezik
Vrsta gradiva:Neznano
Tipologija:1.25 - Drugi sestavni deli
Organizacija:UNG - Univerza v Novi Gorici
Opis:The physics of the non-thermal Universe provides information on the acceleration mechanisms in extreme environments, such as black holes and relativistic jets, neutron stars, supernovae or clusters of galaxies. In the presence of magnetic fields, particles can be accelerated towards relativistic energies. As a consequence, radiation along the entire electromagnetic spectrum can be observed, and extreme environments are also the most likely sources of multi-messenger emission. The most energetic part of the electromagnetic spectrum corresponds to the very-high-energy (VHE, E>100 GeV) gamma-ray regime, which can be extensively studied with ground based Imaging Atmospheric Cherenkov Telescopes (IACTs). The results obtained by the current generation of IACTs, such as H.E.S.S., MAGIC, and VERITAS, demonstrate the crucial importance of the VHE band in understanding the non-thermal emission of extreme environments in our Universe. In some objects, the energy output in gamma rays can even outshine the rest of the broadband spectrum. The Cherenkov Telescope Array (CTA) is the next generation of IACTs, which, with cutting edge technology and a strategic configuration of ~100 telescopes distributed in two observing sites, in the northern and southern hemispheres, will reach better sensitivity, angular and energy resolution, and broader energy coverage than currently operational IACTs. With CTA we can probe the most extreme environments and considerably boost our knowledge of the non-thermal Universe.
Ključne besede:black holes, relativistic jets, neutron stars, supernovae, clusters of galaxies, particle acceleration mechanisms, very-high-energy gamma rays, Cherenkov Telescope Array Observatory
Status publikacije:Objavljeno
Verzija publikacije:Objavljena publikacija
Datum objave:01.06.2021
Leto izida:2021
Št. strani:str. 1-7
Številčenje:2021
PID:20.500.12556/RUNG-9696 Novo okno
COBISS.SI-ID:221825027 Novo okno
UDK:52
ISSN pri članku:2331-8422
NUK URN:URN:SI:UNG:REP:K6RAYQY3
Datum objave v RUNG:10.01.2025
Število ogledov:615
Število prenosov:4
Metapodatki:XML DC-XML DC-RDF
:
BOISSON, C., BROWN, Anthony M., BURTOVOI, A., CERRUTI, M., CHERNYAKOVA, M., HASSAN, T., LENAIN, J.-P., MANGANARO, Marina, VOROBIOV, Serguei in ZAVRTANIK, Danilo, 2021, Probing extreme environments with the Cherenkov Telescope Array. V : ArXiv.org [na spletu]. p. 1–7. Vol. 2021, p. 1–7. [Dostopano 28 april 2025]. Pridobljeno s: https://repozitorij.ung.si/IzpisGradiva.php?lang=slv&id=9696
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Gradivo je del revije

Naslov:ArXiv.org
Skrajšan naslov:ArXiv.org
Založnik:Cornell University Library
ISSN:2331-8422
COBISS.SI-ID:10638614 Novo okno

Gradivo je financirano iz projekta

Financer:ARIS - Javna agencija za znanstvenoraziskovalno in inovacijsko dejavnost Republike Slovenije
Številka projekta:P1-0031
Naslov:Večglasniška astrofizika

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