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
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10303 - Particles and field physics
Result continuities
Project
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Continuities
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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
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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