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Titlebook: Lectures on Cosmology; Accelerated Expansio Georg Wolschin Book 2010 Springer-Verlag Berlin Heidelberg 2010 Cosmology.Redshift.Universe.acc

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書目名稱Lectures on Cosmology
副標(biāo)題Accelerated Expansio
編輯Georg Wolschin
視頻videohttp://file.papertrans.cn/584/583493/583493.mp4
概述Provides pedagogically written introductions to cosmological topics related to expansion of the universe.Contains an overview of statictical methods applied in cosmology.Includes supplementary materia
叢書名稱Lecture Notes in Physics
圖書封面Titlebook: Lectures on Cosmology; Accelerated Expansio Georg Wolschin Book 2010 Springer-Verlag Berlin Heidelberg 2010 Cosmology.Redshift.Universe.acc
描述The lectures that four authors present in this volume investigate core topics related to the accelerated expansion of the Universe. Accelerated expansion occured in the ?36 very early Universe – an exponential expansion in the in ationary period 10 s after the Big Bang. This well-established theoretical concept had rst been p- posed in 1980 by Alan Guth to account for the homogeneity and isotropy of the observable universe, and simultaneously by Alexei Starobinski, and has since then been developed by many authors in great theoretical detail. An accelerated expansion of the late Universe at redshifts z< 1 has been disc- ered in 1998; the expansion is not slowing down under the in uence of gravity, but is instead accelerating due to some uniformly distributed, gravitationally repulsive substance accounting for more than 70% of the mass–energy content of the U- verse, which is now known as dark energy. Its most common interpretation today is given in terms of the so-called CDM model with a cosmological constant .
出版日期Book 2010
關(guān)鍵詞Cosmology; Redshift; Universe; accelerated expansion of the universe; astrophysics; chronological inflati
版次1
doihttps://doi.org/10.1007/978-3-642-10598-2
isbn_softcover978-3-642-10597-5
isbn_ebook978-3-642-10598-2Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 2010
The information of publication is updating

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978-3-642-10597-5Springer-Verlag Berlin Heidelberg 2010
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Lectures on Cosmology978-3-642-10598-2Series ISSN 0075-8450 Series E-ISSN 1616-6361
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Type Ia Supernovae and Cosmology,rse on large scales. Pioneering astronomical surveys in the late 1990s exploited these distant cosmic explosions to directly reveal the presence of a “dark energy,” opposing the attractive, slowing force of gravity and instead accelerating the universe’s rate of expansion. Dark energy has since emer
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Modified Gravity Models of Dark Energy,(.) gravity, where the Lagrangian density . is a function of the Ricci scalar ., the coupling strength between dark energy and non-relativistic matter is of order 1 (.) in the Einstein frame. Even in this situation it is possible for .(.) models to be consistent with local gravity constraints under
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d by leading authorities in the field.Includes detailed protThe ?rst 30 cm of the earth’s surface represents a fragile and valuable ecos- tem, thanks to which terrestrial plants, and indirectly animals and humans, can live. The microbial activity occurring in soil is largely responsible for its phys
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