The Cherenkov Telescope Array potential for the study of young supernova remnants

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10320433" target="_blank" >RIV/00216208:11320/15:10320433 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68378271:_____/15:00455614

Výsledek na webu

<a href="http://dx.doi.org/10.1016/j.astropartphys.2014.08.005" target="_blank" >http://dx.doi.org/10.1016/j.astropartphys.2014.08.005</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.astropartphys.2014.08.005" target="_blank" >10.1016/j.astropartphys.2014.08.005</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The Cherenkov Telescope Array potential for the study of young supernova remnants

Popis výsledku v původním jazyce

Supernova remnants (SNRs) are among the most important targets for c-ray observatories. Being prominent non-thermal sources, they are very likely responsible for the acceleration of the bulk of Galactic cosmic rays (CRs). To firmly establish the SNR paradigm for the origin of cosmic rays, it should be confirmed that protons are indeed accelerated in, and released from, SNRs with the appropriate flux and spectrum. This can be done by detailed theoretical models which account for microphysics of acceleration and various radiation processes of hadrons and leptons. The current generation of Cherenkov telescopes has insufficient sensitivity to constrain theoretical models. A new facility, the Cherenkov Telescope Array (CTA), will have superior capabilitiesand may finally resolve this long standing issue of high-energy astrophysics. We want to assess the capabilities of CTA to reveal the physics of various types of SNRs in the initial 2000 years of their evolution. During this time, the eff

Název v anglickém jazyce

The Cherenkov Telescope Array potential for the study of young supernova remnants

Popis výsledku anglicky

Supernova remnants (SNRs) are among the most important targets for c-ray observatories. Being prominent non-thermal sources, they are very likely responsible for the acceleration of the bulk of Galactic cosmic rays (CRs). To firmly establish the SNR paradigm for the origin of cosmic rays, it should be confirmed that protons are indeed accelerated in, and released from, SNRs with the appropriate flux and spectrum. This can be done by detailed theoretical models which account for microphysics of acceleration and various radiation processes of hadrons and leptons. The current generation of Cherenkov telescopes has insufficient sensitivity to constrain theoretical models. A new facility, the Cherenkov Telescope Array (CTA), will have superior capabilitiesand may finally resolve this long standing issue of high-energy astrophysics. We want to assess the capabilities of CTA to reveal the physics of various types of SNRs in the initial 2000 years of their evolution. During this time, the eff

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BF - Elementární částice a fyzika vysokých energií

OECD FORD obor

—

Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Astroparticle Physics

ISSN

0927-6505

e-ISSN

—

Svazek periodika

62

Číslo periodika v rámci svazku

mar

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

13

Strana od-do

152-164

Kód UT WoS článku

000346548200018

EID výsledku v databázi Scopus

2-s2.0-84908663562