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Titlebook: Current Topics in Astrofundamental Physics: The Cosmic Microwave Background; Norma G. Sánchez Book 2001 Kluwer Academic Publishers 2001 Ac

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書(shū)目名稱(chēng)Current Topics in Astrofundamental Physics: The Cosmic Microwave Background
編輯Norma G. Sánchez
視頻videohttp://file.papertrans.cn/242/241344/241344.mp4
叢書(shū)名稱(chēng)Nato Science Series C:
圖書(shū)封面Titlebook: Current Topics in Astrofundamental Physics: The Cosmic Microwave Background; Norma G. Sánchez Book 2001 Kluwer Academic Publishers 2001 Ac
描述This NATO Advanced Study Institute provided an up dated understanding, from a fundamental and deep point of view, of the progress and current problems in the early universe, cosmic microwave background radiation, large scale structure, dark matter problem, and the interplay between them. The focus was placed on the Cosmic Microwave Background Radiation. Emphasis was given to the mutual impact of fundamental physics and cosmology, both at theoretical and experimental-or observational-levels, within a deep and well defined programme, and a global unifying view, which, in addition, provides of careful inter-disciplinarity. Special Lectures were devoted to neutrinos in astrophysics and high energy astrophysics. In addition, each Course of this series, introduced and promoted topics or subjects, which, although not being of purely astrophysical or cosmological nature, were of relevant physical interest for astrophysics and cosmology. Deep understanding, clarification, synthesis, careful interdisciplinarity within a fundamental physics framework, werethe maingoals ofthe course. Lectures ranged from a motivation and pedagogical introduction for students and participants not directly worki
出版日期Book 2001
關(guān)鍵詞Accretion; Cosmology; Dark matter; EFE; Gravity; Redshift; Renormalization group; Universe; astronomy; astrop
版次1
doihttps://doi.org/10.1007/978-94-010-0748-1
isbn_softcover978-0-7923-6856-4
isbn_ebook978-94-010-0748-1Series ISSN 1389-2185
issn_series 1389-2185
copyrightKluwer Academic Publishers 2001
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https://doi.org/10.1007/978-3-319-17428-0tructure of the polarization field would be effective for further investigation of the primordial signal and noise in the maps of anisotropy and polarization of the cosmic microwave background. Also we discuss the classification of singular points of the vector field of the CMB polarization where po
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S. Valero,E. del Val,J. Alemany,V. Bottiity predicted by CDM. The core radius .. and halo circular velocity .. are related by ..=0.44(..).., analogous to the scaling of degenerate dwarf stars. Particle velocities also filter primordial perturbations, with a filtering scale κ. ∝ ..Ω.(.ρ.).. Particle candidates for warm matter are briefly d
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Minimal String Driven Cosmology and its Predictionsr order corrections and graceful exit of inflation, we find this model closer to the observational Universe properties than the current available string cosmology scenarii. At a more fundamental level, this model is by its construction close to the standard cosmological evolution, and it is driven s
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Some problems of the CMB polarizationtructure of the polarization field would be effective for further investigation of the primordial signal and noise in the maps of anisotropy and polarization of the cosmic microwave background. Also we discuss the classification of singular points of the vector field of the CMB polarization where po
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