Interstellar hydrogen and cosmic background radiation
نویسندگان
چکیده
منابع مشابه
Interstellar Hydrogen and Cosmic Background Radiation
It is shown that a collection of photons with nearly the same frequency exhibits a ”condensation” type of phenomenon corresponding to a peak intensity. The observed cosmic background radiation can be explained from this standpoint in terms of the radiation due to fluctuations in interstellar Hydrogen. In a previous communication[1] it was suggested that the origin of the Cosmic Background Radia...
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The observed cosmic microwave background (CMB) radiation provides strong evidence for the hot big bang. The success of pri-mordial nucleosynthesis calculations (see Sec. 16, " Big-bang nucle-osynthesis ") requires a cosmic background radiation (CBR) characterized by a temperature kT ∼ 1 MeV at a redshift of z ≃ 10 9. In their pioneering work, Gamow, Alpher, and Herman [1] realized this and pred...
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These lectures will attempt to convey the excitement and promise in studies of the microwave radiation left over from the early universe. They are aimed at an audience of experimental high energy physicists. The first lecture will concentrate on how the radiation is characterized, how it and its anisotropies are generated, and the physics that it reveals. The second lecture will concentrate on ...
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ژورنال
عنوان ژورنال: Chaos, Solitons & Fractals
سال: 2001
ISSN: 0960-0779
DOI: 10.1016/s0960-0779(00)00158-2