Search for annihilating dark matter towards dwarf galaxies with the Cherenkov Telescope Array

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00553220" target="_blank" >RIV/68378271:_____/17:00553220 - isvavai.cz</a>
Result on the web
<a href="https://www.epj-conferences.org/articles/epjconf/pdf/2017/05/epjconf_ricap2017_01005.pdf" target="_blank" >https://www.epj-conferences.org/articles/epjconf/pdf/2017/05/epjconf_ricap2017_01005.pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/epjconf/201713601005" target="_blank" >10.1051/epjconf/201713601005</a>

Result language
angličtina
Original language name
Search for annihilating dark matter towards dwarf galaxies with the Cherenkov Telescope Array
Original language description
The standard model of cosmology indicates that approximately 27% of the energy density of the Universe is in the form of dark matter. The nature of dark matter is an open question in modern physics. Indirect dark matter searches with imaging atmospheric Cherenkov telescopes are playing a crucial role in constraining the nature of the dark matter particle through the study of their potential annihilation that could produce very high energy gamma rays from different astrophysical structures. The Cherenkov Telescope Array will provide an unprecedented sensitivity over a range of dark matter mass from ~100 GeV to ~30 TeV. In this contribution we review the status of indirect dark matter searches at dwarf spheroidal galaxies.
Czech name
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Czech description
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Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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