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

The result's identifiers

  • Result code in 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>

  • Alternative codes found

    RIV/68378271:_____/15:00455614

  • Result on the web

    <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>

Alternative languages

  • Result language

    angličtina

  • Original language name

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

  • Original language description

    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

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BF - Elementary particle theory and high energy physics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

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

Others

  • Publication year

    2015

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astroparticle Physics

  • ISSN

    0927-6505

  • e-ISSN

  • Volume of the periodical

    62

  • Issue of the periodical within the volume

    mar

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    13

  • Pages from-to

    152-164

  • UT code for WoS article

    000346548200018

  • EID of the result in the Scopus database

    2-s2.0-84908663562