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Introduction to the theory of the early universe : cosmological perturbations and inflationary theory /

This book accompanies another book by the same authors, "Introduction to the Theory of the Early Universe: Hot Big Bang Theory" and presents the theory of the evolution of density perturbations and relic gravity waves, theory of cosmological inflation and post-inflationary reheating. Writt...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Gorbunov, Dmitry S.
Otros Autores: Rubakov, V. A.
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Singapore ; Hackensack, N.J. : World Scientific, ©2011.
Temas:
Acceso en línea:Texto completo

MARC

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100 1 |a Gorbunov, Dmitry S. 
245 1 0 |a Introduction to the theory of the early universe :  |b cosmological perturbations and inflationary theory /  |c Dmitry S Gorbunov, Valery A Rubakov. 
260 |a Singapore ;  |a Hackensack, N.J. :  |b World Scientific,  |c ©2011. 
300 |a 1 online resource (xiii, 489 pages) :  |b illustrations 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
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504 |a Includes bibliographical references (pages 479-485) and index. 
520 |a This book accompanies another book by the same authors, "Introduction to the Theory of the Early Universe: Hot Big Bang Theory" and presents the theory of the evolution of density perturbations and relic gravity waves, theory of cosmological inflation and post-inflationary reheating. Written in a pedagogical style, the main chapters give a detailed account of the established theory, with derivation of formulas. Being self-contained, it is a useful textbook for advanced undergraduate students and graduate students. Essential materials from General Relativity, theory of Gaussian random 
588 0 |a Print version record. 
505 0 |a 1. Jeans instability in Newtonian gravity. 1.1. Jeans instability in static background. 1.2. Development of instability in expanding universe. 1.3. Linear sizes of perturbations and masses of objects -- 2. Cosmological perturbations in general relativity. Equations of linearized theory. 2.1. Background metric. 2.2. Generalities. 2.3. Equations in helicity sectors. 2.4. Regimes of evolution. 2.5. Scalar field condensate as dark matter -- 3. Evolution of vector and tensor perturbations. 3.1. Vector modes. 3.2. Tensor modes : Relic gravity waves -- 4. Scalar perturbations : Single-component fluids. 4.1. Master equation. 4.2. Relativistic matter. 4.3. Non-relativistic matter. 4.4. Matter perturbations at [symbol] domination -- 5. Primordial perturbations in real universe. 5.1. Adiabatic and isocurvature modes. 5.2. Adiabatic mode in superhorizon regime. 5.3. Initial data for isocurvature modes. 5.4. Primordial spectra : Results from observations. 5.5. Evolution of adiabatic perturbations : A preview -- 6. Scalar perturbations before recombination. 6.1. Adiabatic modes of large wavelengths. 6.2. Adiabatic modes entering the sound horizon at radiation domination. 6.3. Adiabatic perturbations of intermediate momenta. 6.4. CDM isocurvature perturbations. 6.5. Baryon isocurvature perturbations -- 7. Structure formation. 7.1. Matter perturbations after recombination : Linear regime. 7.2. Beginning of non-linear regime. 
546 |a English. 
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650 0 |a Inflationary universe. 
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650 7 |a SCIENCE  |x Cosmology.  |2 bisacsh 
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700 1 |a Rubakov, V. A. 
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