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Titlebook: Generation of Cosmological Large-Scale Structure; David N. Schramm,P. Galeotti Book 1997 Kluwer Academic Publishers 1997 Astronomical Obse

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书目名称Generation of Cosmological Large-Scale Structure
编辑David N. Schramm,P. Galeotti
视频video
丛书名称Nato Science Series C:
图书封面Titlebook: Generation of Cosmological Large-Scale Structure;  David N. Schramm,P. Galeotti Book 1997 Kluwer Academic Publishers 1997 Astronomical Obse
描述This volwne is the proceedings of the third school in particle astrophysics that Schramm and Galeotti have organized at Erice. The focus of thirs third school was the Generation of Cosmological Large-Scale Structure. It was held in November of 1996. The fIrst school in the series was on "Gauge Theory and the Early Universe" in May 1986, the second was on "Dark Matter in the Universe" in May 1988. All three schools have been successful under the auspices of the NATO Advanced Study Institute. This volume is thus the third in the series of the proceedings of these schools. The choice of the topic for this third school was natural, since the problem of generating a large-scale structure has become the most pressing problem in cosmology today. In particular, it is this generation of structure that is the interface between astronomical observations and particle models for the early universe. To date, all models for generating structures inevitably require new fundamental physics beyond the standard, SU x SU X U , model of high energy physics. The 3 2 I seeds for generating structures usually invoke unifIcation physics, and the matter needed to clump and form them seems to require particl
出版日期Book 1997
关键词Astronomical Observation; Cosmology; Dark matter; Redshift; Universe; astronomy; astrophysics
版次1
doihttps://doi.org/10.1007/978-94-009-0053-0
isbn_softcover978-94-010-6513-9
isbn_ebook978-94-009-0053-0Series ISSN 1389-2185
issn_series 1389-2185
copyrightKluwer Academic Publishers 1997
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https://doi.org/10.1007/978-1-4419-6330-7 more complex than two-point statistics, primarily because of the combinatorial explosion of terms and the large number of parameters involved. For this reason special techniques are necessary for the extraction of cosmologically important information.
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https://doi.org/10.1007/978-4-431-55040-2utions as one of three topological types: connected, structureless or clumpy. Connected topologies are consistent with galaxy distributions described as filaments or sheets. Clumpy topologies are often referred to as “meatball” topologies where aggregates of galaxies are surrounded and separated by voids.
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DARK MATTER: An Introductionons as well as the other light element abundancea are examined in detail. Comparison of nucleosynthesis baryonic density arguments with other baryon density arguments is made. Discussion of the interface of density and age arguments is also presented.
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A Two-Dimensional Percolation Analysis of the Las Campanas Redshift Surveyutions as one of three topological types: connected, structureless or clumpy. Connected topologies are consistent with galaxy distributions described as filaments or sheets. Clumpy topologies are often referred to as “meatball” topologies where aggregates of galaxies are surrounded and separated by voids.
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The Findings: Dependent Variables,surements of both the absolute temperature and the anisotropy of the CMB and discuss the relation between the data and the general theoretical framework. Future directions are indicated and the upcoming satellite experiments are discussed.
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