Electromagnetic radiation of superconducting cosmic strings

Cosmic strings are relics of the early Universe which can be formed during the phase transitions of fields with spontaneously broken symmetry in the early Universe. Their existence finds support in modern superstrings theories, both in compactification models and in theories with extended additional...

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Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2013
Автори: Rogozin, D.A., Zadorozhna, L.V.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2013
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119660
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Electromagnetic radiation of superconducting cosmic strings / D.A. Rogozin, L.V. Zadorozhna // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 2. — С. 135-140. — Бібліогр.: 19 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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Резюме:Cosmic strings are relics of the early Universe which can be formed during the phase transitions of fields with spontaneously broken symmetry in the early Universe. Their existence finds support in modern superstrings theories, both in compactification models and in theories with extended additional dimensions. Strings can hold currents, effectively become electrically superconducting wires of astrophysical dimensions. Superconducting cosmic strings can serve as powerful sources of non-thermal radiation in wide energy range. Mechanisms of radiation are synchrotron, synchrotron self-Compton and inverse-Compton on CMB photons radiation of electrons accelerated by bow shock wave, created by magnetosphere of relativistically moving string in intergalactic medium (IGM). Expected fluxes of radiation from the shocked plasma around superconducting cosmic strings are calculated for strings with various tensions and for different cases of their location. Possibilities of strings detection by existing facilities are estimated.
ISSN:2227-1481