Introduction to the theory of the early universe: hot big bang theory
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Format: | Elektronisch E-Book |
Sprache: | English |
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Singapore
World Scientific
©2011
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Online-Zugang: | FAW01 FAW02 Volltext |
Beschreibung: | Includes bibliographical references (pages 457-470) and index This book is written from the viewpoint of a deep connection between cosmology and particle physics. It presents the results and ideas on both the homogeneous and isotropic Universe at the hot stage of its evolution and in later stages. The main chapters describe in a systematic and pedagogical way established facts and concepts on the early and the present Universe. The comprehensive treatment, hence, serves as a modern introduction to this rapidly developing field of science. To help in reading the chapters without having to constantly consult other texts, essential materials from General Re 1. Cosmology : a preview. 1.1. Units. 1.2. The universe today. 1.3. Energy balance in the present universe. 1.4. Future of the universe. 1.5. Universe in the past. 1.6. Structure formation in the universe. 1.7. Inflationary epoch -- 2. Homogeneous isotropic universe. 2.1. Homogeneous isotropic spaces. 2.2. Friedmann-Lemaitre-Robertson-Walker metric. 2.3. Redshift. Hubble Law. 2.4. Slowing down of relative motion. 2.5. Gases of free particles in expanding universe -- 3. Dynamics of cosmological expansion. 3.1. Friedmann equation. 3.2. Sample cosmological solutions. Age of the universe. Cosmological horizon. 3.3. Solutions with recollapse -- 4. [Symbol]CDM : Cosmological model with dark matter and dark energy. 4.1. Composition of the present universe. 4.2. General properties of cosmological evolution. 4.3. Transition from deceleration to acceleration. 4.4. Transition from radiation domination to matter domination. 4.5. Present age of the universe and horizon size. 4.6. Brightness-Redshift relation for distant standard candles. 4.7. Angular sizes of distant objects. 4.8. Quintessence -- 5. Thermodynamics in expanding universe. 5.1. Distribution functions for bosons and fermions. 5.2. Entropy in expanding universe. Baryon-to-photon ratio. 5.3. Models with intermediate matter dominated stage : Entropy generation. 5.4. Inequilibrium processes -- 6. Recombination. 6.1. Recombination temperature in equilibrium approximation. 6.2. Photon last scattering in real universe. 6.3. Kinetic equilibrium. 6.4. Horizon at recombination and its present angular size. Spatial flatness of the universe |
Beschreibung: | 1 Online-Ressource (xiii, 473 pages) |
ISBN: | 9789814322249 9789814322256 9789814343978 9814322245 9814322253 9814343978 |
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500 | |a 1. Cosmology : a preview. 1.1. Units. 1.2. The universe today. 1.3. Energy balance in the present universe. 1.4. Future of the universe. 1.5. Universe in the past. 1.6. Structure formation in the universe. 1.7. Inflationary epoch -- 2. Homogeneous isotropic universe. 2.1. Homogeneous isotropic spaces. 2.2. Friedmann-Lemaitre-Robertson-Walker metric. 2.3. Redshift. Hubble Law. 2.4. Slowing down of relative motion. 2.5. Gases of free particles in expanding universe -- 3. Dynamics of cosmological expansion. 3.1. Friedmann equation. 3.2. Sample cosmological solutions. Age of the universe. Cosmological horizon. 3.3. Solutions with recollapse -- 4. [Symbol]CDM : Cosmological model with dark matter and dark energy. 4.1. Composition of the present universe. 4.2. General properties of cosmological evolution. 4.3. Transition from deceleration to acceleration. 4.4. Transition from radiation domination to matter domination. 4.5. Present age of the universe and horizon size. 4.6. Brightness-Redshift relation for distant standard candles. 4.7. Angular sizes of distant objects. 4.8. Quintessence -- 5. Thermodynamics in expanding universe. 5.1. Distribution functions for bosons and fermions. 5.2. Entropy in expanding universe. Baryon-to-photon ratio. 5.3. Models with intermediate matter dominated stage : Entropy generation. 5.4. Inequilibrium processes -- 6. Recombination. 6.1. Recombination temperature in equilibrium approximation. 6.2. Photon last scattering in real universe. 6.3. Kinetic equilibrium. 6.4. Horizon at recombination and its present angular size. Spatial flatness of the universe | ||
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Datensatz im Suchindex
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any_adam_object | |
author | Gorbunov, D. S., (Dmitriĭ Sergeevich) |
author_GND | (DE-588)128387408 |
author_facet | Gorbunov, D. S., (Dmitriĭ Sergeevich) |
author_role | aut |
author_sort | Gorbunov, D. S., (Dmitriĭ Sergeevich) |
author_variant | d s d s g dsds dsdsg |
building | Verbundindex |
bvnumber | BV043102057 |
collection | ZDB-4-EBA |
ctrlnum | (OCoLC)738434145 (DE-599)BVBBV043102057 |
dewey-full | 523.18 |
dewey-hundreds | 500 - Natural sciences and mathematics |
dewey-ones | 523 - Specific celestial bodies and phenomena |
dewey-raw | 523.18 |
dewey-search | 523.18 |
dewey-sort | 3523.18 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
format | Electronic eBook |
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spelling | Gorbunov, D. S., (Dmitriĭ Sergeevich) Verfasser aut Vvedenie v teorii͡u ranneĭ Vselennoĭ Introduction to the theory of the early universe hot big bang theory Dmitry S. Gorbunov, Valery A. Rubakov Singapore World Scientific ©2011 1 Online-Ressource (xiii, 473 pages) txt rdacontent c rdamedia cr rdacarrier Includes bibliographical references (pages 457-470) and index This book is written from the viewpoint of a deep connection between cosmology and particle physics. It presents the results and ideas on both the homogeneous and isotropic Universe at the hot stage of its evolution and in later stages. The main chapters describe in a systematic and pedagogical way established facts and concepts on the early and the present Universe. The comprehensive treatment, hence, serves as a modern introduction to this rapidly developing field of science. To help in reading the chapters without having to constantly consult other texts, essential materials from General Re 1. Cosmology : a preview. 1.1. Units. 1.2. The universe today. 1.3. Energy balance in the present universe. 1.4. Future of the universe. 1.5. Universe in the past. 1.6. Structure formation in the universe. 1.7. Inflationary epoch -- 2. Homogeneous isotropic universe. 2.1. Homogeneous isotropic spaces. 2.2. Friedmann-Lemaitre-Robertson-Walker metric. 2.3. Redshift. Hubble Law. 2.4. Slowing down of relative motion. 2.5. Gases of free particles in expanding universe -- 3. Dynamics of cosmological expansion. 3.1. Friedmann equation. 3.2. Sample cosmological solutions. Age of the universe. Cosmological horizon. 3.3. Solutions with recollapse -- 4. [Symbol]CDM : Cosmological model with dark matter and dark energy. 4.1. Composition of the present universe. 4.2. General properties of cosmological evolution. 4.3. Transition from deceleration to acceleration. 4.4. Transition from radiation domination to matter domination. 4.5. Present age of the universe and horizon size. 4.6. Brightness-Redshift relation for distant standard candles. 4.7. Angular sizes of distant objects. 4.8. Quintessence -- 5. Thermodynamics in expanding universe. 5.1. Distribution functions for bosons and fermions. 5.2. Entropy in expanding universe. Baryon-to-photon ratio. 5.3. Models with intermediate matter dominated stage : Entropy generation. 5.4. Inequilibrium processes -- 6. Recombination. 6.1. Recombination temperature in equilibrium approximation. 6.2. Photon last scattering in real universe. 6.3. Kinetic equilibrium. 6.4. Horizon at recombination and its present angular size. Spatial flatness of the universe Cosmology General relativity (Physics) Science Astronomy SCIENCE / Cosmology bisacsh Big bang theory fast Naturwissenschaft Big bang theory Kosmologie (DE-588)4114294-9 gnd rswk-swf Kosmologie (DE-588)4114294-9 s 1\p DE-604 Rubakov, Valerij A. 1955-2022 Sonstige (DE-588)128387408 oth http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=373250 Aggregator Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
spellingShingle | Gorbunov, D. S., (Dmitriĭ Sergeevich) Introduction to the theory of the early universe hot big bang theory Cosmology General relativity (Physics) Science Astronomy SCIENCE / Cosmology bisacsh Big bang theory fast Naturwissenschaft Big bang theory Kosmologie (DE-588)4114294-9 gnd |
subject_GND | (DE-588)4114294-9 |
title | Introduction to the theory of the early universe hot big bang theory |
title_alt | Vvedenie v teorii͡u ranneĭ Vselennoĭ |
title_auth | Introduction to the theory of the early universe hot big bang theory |
title_exact_search | Introduction to the theory of the early universe hot big bang theory |
title_full | Introduction to the theory of the early universe hot big bang theory Dmitry S. Gorbunov, Valery A. Rubakov |
title_fullStr | Introduction to the theory of the early universe hot big bang theory Dmitry S. Gorbunov, Valery A. Rubakov |
title_full_unstemmed | Introduction to the theory of the early universe hot big bang theory Dmitry S. Gorbunov, Valery A. Rubakov |
title_short | Introduction to the theory of the early universe |
title_sort | introduction to the theory of the early universe hot big bang theory |
title_sub | hot big bang theory |
topic | Cosmology General relativity (Physics) Science Astronomy SCIENCE / Cosmology bisacsh Big bang theory fast Naturwissenschaft Big bang theory Kosmologie (DE-588)4114294-9 gnd |
topic_facet | Cosmology General relativity (Physics) Science Astronomy SCIENCE / Cosmology Big bang theory Naturwissenschaft Kosmologie |
url | http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=373250 |
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