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Titlebook: Current Topics in Astrofundamental Physics; Primordial Cosmology N. Sánchez,A. Zichichi Book 1998 Springer Science+Business Media Dordrecht

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书目名称Current Topics in Astrofundamental Physics
副标题Primordial Cosmology
编辑N. Sánchez,A. Zichichi
视频video
丛书名称Nato Science Series C:
图书封面Titlebook: Current Topics in Astrofundamental Physics; Primordial Cosmology N. Sánchez,A. Zichichi Book 1998 Springer Science+Business Media Dordrecht
描述This NATO Advanced Study Institute course provided an updated 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 struc­ ture, dark matter problem, and the interplay between them. Emphasis was placed on the mutual impact of fundamental physics and cosmology, both at the theo­ retical 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. In addition, each course of this series introduced and promoted topics or sub­ jects which, although not of a purely astrophysical or cosmological nature, were of relevant physical interest for astrophysics and cosmology. Deep understanding, clarification, synthesis, and careful interdisciplinarity within a fundamental physics framework, were the main goals of the course. Lectures ranged from a motivation and pedagogical introduction for students and participants not directly working in the field to the latest developments and most recent results. All lectures were plenary, had the same duration, and were followed by
出版日期Book 1998
关键词Cosmology; Dark matter; Gravity; Universe; astrophysics
版次1
doihttps://doi.org/10.1007/978-94-011-5046-0
isbn_softcover978-94-010-6119-3
isbn_ebook978-94-011-5046-0Series ISSN 1389-2185
issn_series 1389-2185
copyrightSpringer Science+Business Media Dordrecht 1998
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978-94-010-6119-3Springer Science+Business Media Dordrecht 1998
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https://doi.org/10.1007/978-3-211-74420-8String Quantum Gravity is motivated and introduced. Recent Advances (1995–1996) in the study of the classical and quantum string dynamics in curved spacetime are reported:
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https://doi.org/10.1007/978-3-211-74420-8 gauge-invariant approach to Cosmic Background Radiation (‘CBR’) anisotropies — the Sachs-Wolfe (‘SW’) effect (including the so-called ‘integrated SW-effect’). In the first part we emphasize the differences between the results of the full covariant dynamic theory and (a) linearised theory in ‘almost
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https://doi.org/10.1007/978-3-211-74420-8se after inflation [1]. It makes this process extremely important. However, for many years the theory of reheating remained the least developed part of inflationary theory. Even now, when many features of the mechanism of reheating are understood, the literature on this subject is still full of cont
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https://doi.org/10.1007/978-3-211-74420-8nergy densities involved (∼1/g ∼ 10.) make necessary the use of non-perturbative approaches as the large . and Hartree methods. We start these lectures by introducing the such non-perturbative out of equilibrium methods in cosmological universes. We discuss the renormalization procedure and the choi
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https://doi.org/10.1007/978-3-211-74420-8iu, Lucchesi, and Manuel, I give the simplest derivation possible, using classical kinetic theory..The result is valid not just for a thermal, but for an arbitrary initial distributions. I use this to study the evolution, at short times, of a gluonic “tsunami wave”..I also suggest how classical kine
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