Izpis gradiva

A+ | A- | | SLO | ENG

Naslov: Cherenkov Telescope Array potential in the search for Galactic PeVatrons Avtorji: ID Angüner, E.O. (Avtor) ID Eckner, Christopher (Avtor) ID Kukec Mezek, Gašper (Avtor) ID Stanič, Samo (Avtor) ID Vorobiov, Serguei (Avtor) ID Yang, Lili (Avtor) ID Zaharijas, Gabrijela (Avtor) ID Zavrtanik, Danilo (Avtor) ID Zavrtanik, Marko (Avtor) ID Zehrer, Lukas (Avtor), et al. Datoteke: ICRC2019_618.pdf (677,22 KB) MD5: 3D3AF627FD383A346879A60249C9A661   https://pos.sissa.it/358/618/pdf   https://pos.sissa.it/358/   To gradivo ima še več datotek. Celoten seznam je na voljo spodaj. Jezik: Angleški jezik Vrsta gradiva: Delo ni kategorizirano Tipologija: 1.08 - Objavljeni znanstveni prispevek na konferenci Organizacija: UNG - Univerza v Novi Gorici Opis: One of the major scientific objectives of the future Cherenkov Telescope Array (CTA) Observatory is the search for PeVatrons. PeVatrons are cosmic-ray factories able to accelerate nuclei at least up to the knee feature seen in the spectrum of cosmic rays measured near the Earth. CTA will perform a survey of the full Galactic plane at TeV energies and beyond with unprecedented sensitivity. The determination of efficient criteria to identify PeVatron candidates during the survey is essential in order to trigger further dedicated observations. Here, we present results from a study based on simulations to determine these criteria. The outcome of the study is a PeVatron figure of merit, defined as a metric that provides relations between spectral parameters and spectral cutoff energy lower limits. In addition, simulations of the PeVatron candidate HESS J1641−463 and its parental particle spectrum are presented and discussed. Eventually, our work is applied to simulated population of Galactic PeVatrons, with the aim to determine the sensitivity of CTA. Ključne besede: Galactic cosmic rays, very-high-energy gamma rays, Galactic PeVatrons, Cherenkov Telescope Array (CTA) Observatory, Galactic plane survey, H.E.S.S. J1641−463 PeVatron candidate Status publikacije: Objavljeno Verzija publikacije: Objavljena publikacija Leto izida: 2019 COBISS.SI-ID: 214297603  NUK URN: URN:SI:UNG:REP:XN085ERJ Datum objave v RUNG: 08.11.2024 Število ogledov: 171 Število prenosov: 5 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

Skupna ocena: (0 glasov) Vaša ocena: Ocenjevanje je dovoljeno samo prijavljenim uporabnikom. Objavi na: Postavite miškin kazalec na naslov za izpis povzetka. Klik na naslov izpiše podrobnosti ali sproži prenos.

Gradivo je del monografije

Naslov:	Proceedings of the 36th International Cosmic Ray Conference : ICRC2019, July 24th - August 1st, 2019, Madison, WI, U.S.A.
Kraj izida:	SISSA, Trieste
Leto izida:	2019

Gradivo je financirano iz projekta

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

Licence

Licenca:	CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
Povezava:	http://creativecommons.org/licenses/by-nc-nd/4.0/deed.sl
Opis:	Najbolj omejujoča licenca Creative Commons. Uporabniki lahko prenesejo in delijo delo v nekomercialne namene in ga ne smejo uporabiti za nobene druge namene.

Datoteke

Podatki se nalagajo...

Nazaj