Introduction to the theory of the early universe :: hot big bang theory /
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...
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Format: | Elektronisch E-Book |
Sprache: | English Russian |
Veröffentlicht: |
Singapore ; Hackensack, NJ :
World Scientific,
©2011.
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Schlagworte: | |
Online-Zugang: | Volltext |
Zusammenfassung: | 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. |
Beschreibung: | 1 online resource (xiii, 473 pages) : illustrations |
Bibliographie: | Includes bibliographical references (pages 457-470) and index. |
ISBN: | 9789814322256 9814322253 |
Internformat
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240 | 1 | 0 | |a Vvedenie v teorii︠u︡ ranneĭ Vselennoĭ. |l English |
245 | 1 | 0 | |a Introduction to the theory of the early universe : |b hot big bang theory / |c Dmitry S. Gorbunov, Valery A. Rubakov. |
260 | |a Singapore ; |a Hackensack, NJ : |b World Scientific, |c ©2011. | ||
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504 | |a Includes bibliographical references (pages 457-470) and index. | ||
520 | |a 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. | ||
588 | 0 | |a Print version record. | |
505 | 0 | |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. | |
546 | |a Translated from the original Russian into English. | ||
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700 | 1 | |a Rubakov, V. A. | |
776 | 0 | 8 | |i Print version: |a Gorbunov, D.S. (Dmitriĭ Sergeevich). |s Vvedenie v teorii︠u︡ ranneĭ Vselennoĭ. English. |t Introduction to the theory of the early universe. |d Singapore ; Hackensack, NJ : World Scientific, ©2011 |z 9814343978 |w (OCoLC)704340492 |
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adam_text | |
any_adam_object | |
author | Gorbunov, D. S. (Dmitriĭ Sergeevich) |
author2 | Rubakov, V. A. |
author2_role | |
author2_variant | v a r va var |
author_GND | http://id.loc.gov/authorities/names/n2009069990 |
author_facet | Gorbunov, D. S. (Dmitriĭ Sergeevich) Rubakov, V. A. |
author_role | |
author_sort | Gorbunov, D. S. |
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building | Verbundindex |
bvnumber | localFWS |
callnumber-first | Q - Science |
callnumber-label | QB991 |
callnumber-raw | QB991.B54 G6713 2011eb |
callnumber-search | QB991.B54 G6713 2011eb |
callnumber-sort | QB 3991 B54 G6713 42011EB |
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collection | ZDB-4-EBA |
contents | 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. |
ctrlnum | (OCoLC)738434145 |
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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illustrated | Illustrated |
indexdate | 2024-11-27T13:17:53Z |
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isbn | 9789814322256 9814322253 |
language | English Russian |
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spelling | Gorbunov, D. S. (Dmitriĭ Sergeevich) https://id.oclc.org/worldcat/entity/E39PCjyQj4XjC739vJKVm6YFDm http://id.loc.gov/authorities/names/n2009069990 Vvedenie v teorii︠u︡ ranneĭ Vselennoĭ. English Introduction to the theory of the early universe : hot big bang theory / Dmitry S. Gorbunov, Valery A. Rubakov. Singapore ; Hackensack, NJ : World Scientific, ©2011. 1 online resource (xiii, 473 pages) : illustrations text txt rdacontent computer c rdamedia online resource 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. Print version record. 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. Translated from the original Russian into English. Big bang theory. http://id.loc.gov/authorities/subjects/sh85013943 Big bang. SCIENCE Cosmology. bisacsh Big bang theory fast Kosmologie. idszbz Urknall. idszbz Stora smällen. sao Kosmologi. sao Rubakov, V. A. Print version: Gorbunov, D.S. (Dmitriĭ Sergeevich). Vvedenie v teorii︠u︡ ranneĭ Vselennoĭ. English. Introduction to the theory of the early universe. Singapore ; Hackensack, NJ : World Scientific, ©2011 9814343978 (OCoLC)704340492 FWS01 ZDB-4-EBA FWS_PDA_EBA https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=373250 Volltext |
spellingShingle | Gorbunov, D. S. (Dmitriĭ Sergeevich) Introduction to the theory of the early universe : hot big bang theory / 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. Big bang theory. http://id.loc.gov/authorities/subjects/sh85013943 Big bang. SCIENCE Cosmology. bisacsh Big bang theory fast Kosmologie. idszbz Urknall. idszbz Stora smällen. sao Kosmologi. sao |
subject_GND | http://id.loc.gov/authorities/subjects/sh85013943 |
title | Introduction to the theory of the early universe : hot big bang theory / |
title_alt | Vvedenie v teorii︠u︡ 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 | Big bang theory. http://id.loc.gov/authorities/subjects/sh85013943 Big bang. SCIENCE Cosmology. bisacsh Big bang theory fast Kosmologie. idszbz Urknall. idszbz Stora smällen. sao Kosmologi. sao |
topic_facet | Big bang theory. Big bang. SCIENCE Cosmology. Big bang theory Kosmologie. Urknall. Stora smällen. Kosmologi. |
url | https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=373250 |
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