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Naslov:Probing dark matter and fundamental physics with the Cherenkov Telescope Array
Avtorji:ID Iocco, Fabio (Avtor)
ID Meyer, Manuel (Avtor)
ID Doro, M. (Avtor)
ID Hofmann, Werner (Avtor)
ID Pérez Romero, Judit (Avtor)
ID Zaharijas, Gabrijela (Avtor)
ID Aguirre-Santaella, A. (Avtor)
ID Amato, E. (Avtor)
ID Angüner, E. O. (Avtor)
ID Eckner, Christopher (Avtor), et al.
Datoteke:URL https://arxiv.org/pdf/2106.03582?
 
.pdf 2106.03582v2.pdf (6,31 MB)
MD5: 708C1BBA5984DACDC35B5C8AAE907696
 
URL https://arxiv.org/pdf/2106.03582
 
To gradivo ima še več datotek. Celoten seznam je na voljo spodaj.
Jezik:Angleški jezik
Vrsta gradiva:Neznano
Tipologija:1.25 - Drugi sestavni deli
Organizacija:UNG - Univerza v Novi Gorici
Opis:Astrophysical observations provide strong evidence that more than 80% of all matter in the Universe is in the form of dark matter (DM). Two leading candidates of particles beyond the Standard Model that could constitute all or a fraction of the DM content are the so-called Weakly Interacting Massive Particles (WIMPs) and Axion-Like Particles (ALPs). The upcoming Cherenkov Telescope Array, which will observe gamma rays between 20 GeV and 300 TeV with unprecedented sensitivity, will have unique capabilities to search for these DM candidates. A particularly promising target for WIMP searches is the Galactic Center. WIMPs with annihilation cross sections correctly producing the DM relic density will be detectable with CTA, assuming an Einasto-like density profile and WIMP masses between 200 GeV and 10 TeV. Regarding new physics beyond DM, CTA observations will also enable tests of fundamental symmetries of nature such as Lorentz invariance.
Ključne besede:dark matter, weakly interacting massive particles, axion-like particles, fundamental physics, Lorentz invariance, 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-9694 Novo okno
COBISS.SI-ID:221646851 Novo okno
UDK:52
ISSN pri članku:2331-8422
NUK URN:URN:SI:UNG:REP:SHKKXNNF
Datum objave v RUNG:09.01.2025
Število ogledov:528
Število prenosov:5
Metapodatki:XML DC-XML DC-RDF
:
IOCCO, Fabio, MEYER, Manuel, DORO, M., HOFMANN, Werner, PÉREZ ROMERO, Judit, ZAHARIJAS, Gabrijela, AGUIRRE-SANTAELLA, A., AMATO, E., ANGÜNER, E. O. in ECKNER, Christopher, 2021, Probing dark matter and fundamental physics with the Cherenkov Telescope Array. V : ArXiv.org [na spletu]. p. 1–7. Vol. 2021, p. 1–7. [Dostopano 7 april 2025]. Pridobljeno s: https://repozitorij.ung.si/IzpisGradiva.php?lang=slv&id=9694
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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

Licence

Licenca:Drugo
Opis:The URI http://arxiv.org/licenses/nonexclusive-distrib/1.0/ is used to record the fact that the submitter granted the following license to arXiv.org on submission of an article: I grant arXiv.org a perpetual, non-exclusive license to distribute this article. I certify that I have the right to grant this license. I understand that submissions cannot be completely removed once accepted. I understand that arXiv.org reserves the right to reclassify or reject any submission. Revision history 2004-01-16 - License above introduced as part of arXiv submission process 2007-06-21 - This HTML page created

Datoteke

URL https://arxiv.org/pdf/2106.03582?
Izvorni URL
.pdf 2106.03582v2.pdf
Predstavitvena datoteka - 6,31 MB
MD5: 708C1BBA5984DACDC35B5C8AAE907696
URL https://arxiv.org/pdf/2106.03582
Izvorni URL
URL https://arxiv.org/html/2106.08952v1/
Izvorni URL
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