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Sensitivity of the Cherenkov telescope array to the detection of intergalactic magnetic fields

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F16%3A00538444" target="_blank" >RIV/68378271:_____/16:00538444 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.3847/0004-637X/827/2/147" target="_blank" >https://doi.org/10.3847/0004-637X/827/2/147</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/0004-637X/827/2/147" target="_blank" >10.3847/0004-637X/827/2/147</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Sensitivity of the Cherenkov telescope array to the detection of intergalactic magnetic fields

  • Original language description

    Very high energy (VHE, energy E greater than or similar to 100 GeV) gamma-rays originating from extragalactic sources undergo pair production with low-energy photons of background radiation fields. These pairs can inverse-Compton-scatter background photons, initiating an electromagnetic cascade. The spatial and temporal structure of this secondary gamma-ray signal is altered as the e(+)e(-) pairs are deflected in an intergalactic magnetic field (IGMF). We investigate how VHE observations with the future Cherenkov Telescope Array, with its high angular resolution and broad energy range, can potentially probe the IGMF. We identify promising sources and simulate gamma-ray spectra over a wide range of values of the IGMF strength and coherence length using the publicly available ELMAG Monte. Carlo code. Combining simulated observations in a joint likelihood approach, we find that current limits on the IGMF can be significantly improved. The projected sensitivity depends strongly on the time a source has been gamma-ray active and on the emitted maximum gamma-ray energy.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

  • Continuities

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astrophysical Journal

  • ISSN

    0004-637X

  • e-ISSN

  • Volume of the periodical

    827

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    10

  • Pages from-to

    1-10

  • UT code for WoS article

    000384001600059

  • EID of the result in the Scopus database

    2-s2.0-84984689217