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Sunyaev-Zeldovich signatures from non-thermal, relativistic electrons using CMB maps

Relativistically energetic, non-thermal population of electrons can give rise to unique CMB spectral distortion signatures which can be significantly different from thermal Sunyaev-Zeldovich signal or $y$-distortion. These signatures depend upon the spectrum of non-thermal electrons, therefore, a de...

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書誌詳細
第一著者: Sandeep Kumar Acharya
フォーマット: Artigo
言語:Inglês
出版事項: Maynooth Academic Publishing 2024-07-01
シリーズ:The Open Journal of Astrophysics
オンライン・アクセス:https://doi.org/10.33232/001c.120979
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