Izpis gradiva

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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: https://arxiv.org/pdf/2106.03582?   2106.03582v2.pdf (6,31 MB) MD5: 708C1BBA5984DACDC35B5C8AAE907696   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  COBISS.SI-ID: 221646851  UDK: 52 ISSN pri članku: 2331-8422 NUK URN: URN:SI:UNG:REP:SHKKXNNF Datum objave v RUNG: 09.01.2025 Število ogledov: 281 Število prenosov: 4 Metapodatki:    Citiraj gradivo Navadno besedilo BibTeX EndNote XML EndNote/Refer RIS ABNT ACM Ref AMA APA Chicago 17th Author-Date Harvard IEEE ISO 690 MLA Vancouver : Kopiraj citat

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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

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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