Наукова електронна бібліотека
періодичних видань НАН України
періодичних видань НАН України
New emission line at ~3.5 keV - observational status, connection with radiatively decaying dark matter and directions for future studies
Репозиторій DSpace/Manakin
JavaScript is disabled for your browser. Some features of this site may not work without it.
New emission line at ~3.5 keV - observational status, connection with radiatively decaying dark matter and directions for future studies
Інший ID:
DOI: 10.17721/2227-1481.4.9-14
Посилання:
New emission line at ~3.5 keV - observational status, connection with radiatively decaying dark matter and directions for future studies / D.A. Iakubovskyi // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 9-14. — Бібліогр.: 98 назв. — англ.
Підтримка:
This work was supported by part by the Swiss National Science Foundation grant SCOPE IZ7370-152581, the Program of Cosmic Research of the National Academy of Sciences of Ukraine, the State Programme of Implementation of Grid Technologyin Ukraine, and the grant of President of Ukraine for young scientists.
Дата:
2014
Переглядів:
716
Завантажень:
301
Анотація:
Recent works of Bulbul et al. (2014) and Boyarsky et al. (2014), claiming the detection of the extra emission line with energy ∼3.5 keV in X-ray spectra of certain clusters of galaxies and nearby Andromeda galaxy, have raised a considerable interest in astrophysics and particle physics communities. A number of new observational studies
claim detection or non-detection of the extra line in X-ray spectra of various cosmic objects. In this review I summarise existing results of these studies, overview possible interpretations of the extra line, including intriguing connection with radiatively decaying dark matter, and show future directions achievable with existing and planned X-ray cosmic missions.
