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Titlebook: Calibrating the Cosmos; How Cosmology Explai Frank S. Levin (Professor Emeritus of Physics) Book 2007 Springer-Verlag New York 2007 Big Ban

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發(fā)表于 2025-3-21 17:50:30 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Calibrating the Cosmos
副標(biāo)題How Cosmology Explai
編輯Frank S. Levin (Professor Emeritus of Physics)
視頻videohttp://file.papertrans.cn/221/220900/220900.mp4
概述Concentrates on, and explains in clear, non-technical language, the ideas and methods scientists have used in achieving the current understanding of the universe.Bridges the gap between advanced techn
叢書名稱Astronomers‘ Universe
圖書封面Titlebook: Calibrating the Cosmos; How Cosmology Explai Frank S. Levin (Professor Emeritus of Physics) Book 2007 Springer-Verlag New York 2007 Big Ban
描述.Calibrating the Cosmos describes hard science, but is gently written. It explains in clear, non-mathematical language the measurements and the interpretation of the resulting data that have led to the current understanding of the origin, evolution and properties of our expanding Big Bang universe...Many people have a sketchy idea of the work of cosmologists, but Professor Levin’s experience in teaching both scientific and liberal arts students has enabled him to impart much of our current thinking without resorting to difficult mathematics. Theoretical concepts are emphasized, in particular the symmetries of homogeneity and isotropy enjoyed by our universe on the largest scales, how these symmetries lead to only one quantity being needed to describe the growth of the universe from its infancy to the present time, and how the so-called parameters of the universe are the ingredients used to construct the model universes to which ours – the real thing – is compared...Levin includes the 2003 results from the Wilkinson Microwave Anisotropy Probe (WMAP) and the 2003 and 2004 results of the Sloan Digital Sky Survey to ensure that the book?is up to date.?He?explains the relevance of the d
出版日期Book 2007
關(guān)鍵詞Big Bang; Big Bang explained; Cosmology; Universe; evolution of the universe; stars; what is cosmology
版次1
doihttps://doi.org/10.1007/978-0-387-49768-6
isbn_softcover978-1-4419-2152-9
isbn_ebook978-0-387-49768-6Series ISSN 1614-659X Series E-ISSN 2197-6651
issn_series 1614-659X
copyrightSpringer-Verlag New York 2007
The information of publication is updating

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Wachen, Aufmerksamkeit und Schlafen of intrinsic brightness: a 1000-W bulb is more intense than a 100-W bulb; the sun is far more intense than either. It is usually easier to see a source of greater intensity than it is a weaker one, but just as too weak a source will not lead to seeing, too strong a source cannot be viewed for too long.
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H. O. Handwerker,H.-G. Schaiblermous distance from the earth: apart from white dwarfs, neutron stars, and nonmassive black holes, stars are huge. An example is the sun, whose mass and volume, respectively, are roughly 300,000 and a million times that of the earth.
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Light, Radiation, and Quanta, of intrinsic brightness: a 1000-W bulb is more intense than a 100-W bulb; the sun is far more intense than either. It is usually easier to see a source of greater intensity than it is a weaker one, but just as too weak a source will not lead to seeing, too strong a source cannot be viewed for too long.
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Stars: Attributes, Energetics, End Stages,rmous distance from the earth: apart from white dwarfs, neutron stars, and nonmassive black holes, stars are huge. An example is the sun, whose mass and volume, respectively, are roughly 300,000 and a million times that of the earth.
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Kognitive Funktionen und Denken, Herman on primordial nucleosynthesis and has enabled cosmologists not only to deduce which events occurred as the Universe evolved but also, with increasing accuracy, to pinpoint the times of their occurrences.
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