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Cosmology:

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1. Verfasser:	Weinberg, Steven 1933-2021 (VerfasserIn)
Format:	Buch
Sprache:	English
Veröffentlicht:	Oxford [u.a.] Oxford Univ. Press 2008
Ausgabe:	1. publ.
Schlagworte:	Cosmologia Cosmology Kosmologie Gravitationstheorie Relativitätstheorie
Online-Zugang:	Inhaltsverzeichnis
Beschreibung:	Hier auch später erschienene, unveränderte Nachdrucke
Beschreibung:	XVII, 593 S. graph. Darst.
ISBN:	9780198526827

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Datensatz im Suchindex

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adam_text	Contents 1 THE EXPANSION OF THE UNIVERSE 1 1.1 Spacetime geometry 2 Robertson-Walker metric □ Co-moving coordinates D Proper distances □ Momentum decay D Spatial geodesies D Number conservation Π Energy & momentum conservation D Cold matter, hot matter, vacuum energy D Global geometry & topology 1.2 The cosmological redshift 10 Emission time vs. radial coordinate □ Redshifts & blueshifts D Hubble constant □ Discovery of expansion D Changing redshifts 1.3 Distances at small redshift: The Hubble constant 13 Trigonometric parallax □ Proper motions π Apparent luminosity: Main sequence, red clump stars, RR Lyrae stars, eclipsing binaries, Cepheid vari¬ ables D Tully-Fisher relation □ Faber-Jackson relation π Fundamental Plane □ Type Ia supernovae □ Surface brightness fluctuations □ Result for Hubble constant 1.4 Luminosity distances and angular diameter distances 31 Luminosity distance □ Deceleration parameter О Jerk & snap D Angular diameter distance 1.5 Dynamics of expansion 34 Einstein field equations D Friedmann equation □ Newtonian derivation □ Critical density □ Flatness problem D Matter-dominated expansion □ Radiation-dominated expansion □ Vacuum-dominated expansion Π De Sitter model □ Ωμ, Qr, Ω λ d Age of expansion □ Luminosity distance formula □ Future expansion D Historical note: cosmological constant □ Historical note: steady state model 1.6 Distances at large redshifts: Accelerated expansion 45 Discovery of accelerated expansion Π Newtonian interpretation □ Gray dust? D Discovery of early deceleration D Other effects О Equation of state parameter w О X-ray observations □ The cosmological constant problems 1.7 Cosmic expansion or tired light? 57 Surface brightness test Q Supernova decline slowdown 1.8 Ages 59 Heavy element abundance □ Main sequence turn-off □ Age vs. redshift xi Contents 1.9 Masses 65 Virialized clusters of galaxies: им □ X-ray luminosity of clusters of galaxies: Ωβ/Ωμ 1.10 Intergalactic absorption 75 Optical depth □ Resonant absorption Π 21 cm absorption □ Lyman a absorption □ Gunn-Peterson trough □ Alcock-Paczynski analysis 1.11 Number counts 82 Number vs. ζ and I □ Evolution D Radio source surveys 1.12 Quintessence 89 Scalar field theories □ Power-law potential □ Tracker solution □ Two- parameter models 1.13 Horizons 98 Particle horizon Π Event horizon 2 THE COSMIC MICROWAVE RADIATION BACKGROUND 101 2.1 Expectations and discovery of the microwave background 101 Black body radiation □ Early suggestions □ Discovery D Rayleigh-Jeans formula D CN absorption lines Π Balloons & rockets D СОВЕ & FIRAS □ Energy density Π Number density □ Effect on cosmic rays 2.2 The equilibrium era 109 Entropy per baryon □ Radiation-matter equality □ Energy decoupling 2.3 Recombination and last scattering 113 Maxwell-Boltzmann distribution □ Saha formula □ Delay of η — 2 to η = 1 □ Peebles analysis □ Lyman a escape probability □ Rate equation □ Fractional ionization D Opacity □ Jones-Wyse approximation 2.4 The dipole anisotropy 129 Angular dependence of temperature Π U2 discovery D СОВЕ & WMAP measurements □ Kinematic quadrupole 2.5 The Sunyaev-ZeI dovich effect 132 Kompaneets equation □ Spectrum shift О Use with X-ray luminosity 2.6 Primary fluctuations in the microwave background: A first look 135 Partial-wave coefficients a¿m □ Multipole coefficients Q □ Cosmic variance Π Sachs-Wolfe effect D Harrison-Zeľdovich spectrum □ Doppler fluctua¬ tions □ Intrinsic temperature fluctuations □ Integrated Sachs-Wolfe effect D СОВЕ observations xii Contents 3 THE EARLY UNIVERSE 149 3.1 Thermal history 149 Entropy density D Fermi-Dirac & Bose-Einstein distributions □ Time vs. temperature □ Effective number of species D Neutrino decoupling Π Heating by electron-positron annihilation □ Neutrino masses & chemical potentials 3.2 Cosmological nucleosynthesis 159 Neutron-proton conversion □ Equilibrium nuclear abundances □ Deuterium bottleneck □ Helium abundance □ Deuterium abundance □ He3 abundance □ Lithium abundance D ÇiBh2 3.3 Baryonsynthesis and Leptonsynthesis 173 Sakharov conditions □ Delayed decay D Electroweak nonconservation D Leptogenesis □ Affleck-Dine mechanism □ Equilibrium baryonsynthesis 3.4 Cold dark matter 185 The bullet cluster D Leftover WIMP abundance α Sparticles □ WIMP searches О Annihilation γ rays □ Axions & axinos 4 INFLATION 201 4.1 Three puzzles 202 Flatness □ Horizons □ Monopoles 4.2 Slow-roll inflation 208 Bubble formation □ New inflation □ Slow-roll conditions π Power-law potential □ Exponential potential □ Reheating 4.3 Chaotic inflation, eternal inflation 216 Condition for eternal inflation □ Condition for chaotic inflation 5 GENERAL THEORY OF SMALL FLUCTUATIONS 219 5.1 Field equations 219 Perturbed Ricci tensor □ Perturbed energy-momentum tensor G Scalar modes D Vector modes α Tensor modes 5.2 Fourier decomposition and stochastic initial conditions 228 Plane wave solutions □ Stochastic parameters О Correlation functions Π Helicity decomposition 5.3 Choosing a gauge 235 Gauge transformations □ Newtonian gauge □ Synchronous gauge □ Conversion α Other gauges ХШ Contents 5.4 Conservation outside the horizon 245 The quantities ΊΖ and ζ □ A conservation theorem D Conservation for isolated components 6 EVOLUTION OF COSMOLOGICAL FLUCTUATIONS 257 6.1 Scalar perturbations - kinetic theory 258 Cold dark matter □ Baryonic plasma D Photon number density matrix perturbation 8nV □ Photon dimensionless intensity matrix Jy О Photon Boltzmann equations □ Photon source functions □ Photon pressure, den¬ sity, anisotropic inertia □ Photon line-of-sight solutions □ Neutrino number density perturbation bnv D Neutrino dimensionless intensity J О Neutrino Boltzmann equations D Neutrino pressure, density, anisotropic inertia □ Neutrino line-of-sight solutions □ Gravitational field equations □ Initial conditions 6.2 Scalar perturbations - the hydrodynamic limit 274 Hydrodynamic & field equations О Adiabatic initial conditions D Non- adiabatic modes □ Long & short wavelengths 6.3 Scalar perturbations - long wavelengths 282 Evolution far outside horizon □ Evolution in matter-dominated era 6.4 Scalar perturbations - short wavelengths 289 Evolution in radiation-dominated era □ Evolution deep inside horizon Π Fast & slow modes □ Matching 6.5 Scalar perturbations - interpolation & transfer functions 303 Exact solution for рв = 0 О Transfer functions О Baryon density & damp¬ ing effects 6.6 Tensor perturbations 312 Gravitational field equations D Photon Boltzmann equations Π Photon source functions □ Photon anisotropic inertia □ Photon line-of-sight sol¬ ution □ Neutrino Boltzmann equations D Neutrino anisotropic inertia □ Neutrino line-of-sight solutions □ Evolution without damping D Transfer functions □ Effect of damping 7 ANISOTROPIES IN THE MICROWAVE SKY 329 7.1 General formulas for the temperature fluctuations 329 Line-of-sight formula □ Rearrangement of scalar temperature fluctuation о Integrated Sachs-Wolfe effect □ Sudden decoupling approximation □ Re-derivation following photon trajectories □ Gauge invariance XIV Contents 7.2 Temperature multipole coefficients: Scalar modes 343 General formula □ Large I approximation □ Calculation of form fac¬ tors □ Silk & Landau damping □ Comparison with numerical codes α Balloon & ground-based observations □ WMAP D Results for cosmological parameters 7.3 Temperature multipole coefficients: Tensor modes 362 General formula □ Calculation of gravitational wave amplitude □ Calcu¬ lation of source function □ Large Ł approximation □ Sudden decoupling approximation D Numerical results 7.4 Polarization 370 Stokes parameters □ Spherical harmonics of spin ±2 □ Space-inversion properties □ E and В polarization G Scalar modes: general formula О Scalar modes: large і approximation D Scalar modes: numerical results Π Scalar modes: observations □ Tensor modes: general formula О Tensor modes: large і approximation G Tensor modes: numerical results □ Correlation functions 8 THE GROWTH OF STRUCTURE 403 8.1 Linear perturbations after recombination 403 Hydrodynamic and field equations □ Factorization of perturbations □ Effect of vacuum energy □ Power spectral function P(k) □ Correlation function ü Direct measurement of P(k) □ Rms fluctuation or □ Mea¬ surements of P(k) □ Baryon acoustic oscillations □ Cosmic variance in measuring P(k) 8.2 Nonlinear growth 421 Spherically symmetric collapse □ Calculation of ал Ο Press-Schechter mass function 8.3 Collapse of baryonic matter 427 Jeans mass □ Continuity & Euler equations □ Power-law solutions D Critical wave number for baryon collapse 9 GRAVITATIONAL LENSES 433 9.1 Lens equation for point masses 433 Derivation of lens equation □ Image separation □ Einstein ring 9.2 Magnification: Strong lensing and microlensing 436 Image luminosity α Conservation of surface brightness □ Effective radius for strong lensing □ Number counts □ De Sitter model Π Einstein-de Sitter model D Lens survey □ Microlensing observations xv Contents 9.3 Extended lenses 443 Isothermal spheres □ Lens equation □ Lens luminosity □ Number counts □ Surveys 9.4 Time delay 447 Geometrical delay □ Potential delay □ Observations 9.5 Weaklensing 452 Calculation of deflection Π Shear matrix D Ellipse matrix D Mean shear matrix □ Shear field к D Multipole coefficients □ Large í approximation D Measurement of P(k) Π Correlation functions □ Shear surveys 9.6 Cosmic strings 467 Calculation of deflection □ A string suspect 10 INFLATION AS THE ORIGIN OF COSMOLOGICAL FLUCTUATIONS 469 10.1 Scalar fluctuations during inflation 470 Scalar field action □ Field, density, pressure, and velocity perturbations D Field equations □ WKB early-time solution Π Fourier decomposition D Commutation relations □ Bunch-Davies vacuum □ Gaussian statis¬ tics □ Curvature perturbation ΊΖ □ Mukhanov-Sasaki equation D Limit TV q outside horizon □ Number of е -foldings after horizon exit □ Expo¬ nential potential D Measurement of spectral index & fluctuation strength □ Values of exponential potential parameters D Justification of simple action 10.2 Tensor fluctuations during inflation 485 Gravitational field equation Π WKB early-time solution □ Fourier decomposition □ Commutation relations □ Scalar/tensor ratio r □ Obser¬ vational bounds on r 10.3 Fluctuations during inflation: The slow-roll approximation 488 Parameters e and б D Slow-roll approximation D Spectral index and fluc¬ tuation strength Π Observational constraints on potential □ Number of е -foldings after horizon exit 10.4 Multifield inflation 497 Gaussian, adiabatic, scale-invariant, & weak fluctuations D Thermal equi¬ librium after inflation □ Evolution equations □ WKB early-time solution D Vielbeins □ Commutation relations О Slow-roll conditions □ 7Ł after horizon exit О What we have learned about inflation xvi Contents APPENDICES A. Some Useful Numbers 509 B. Review of General Relativity 511 C. Energy Transfer between Radiation and Electrons 53 1 D. The Ergodic Theorem 537 E. Gaussian Distributions 541 F. Newtonian Cosmology 543 G. Photon Polarization 547 H. The Relativistic Boltzmann Equation 551 GLOSSARY OF SYMBOLS 565 ASSORTED PROBLEMS 569 AUTHOR INDEX 575 SUBJECT INDEX 587 XVII
adam_txt	Contents 1 THE EXPANSION OF THE UNIVERSE 1 1.1 Spacetime geometry 2 Robertson-Walker metric □ Co-moving coordinates D Proper distances □ Momentum decay D Spatial geodesies D Number conservation Π Energy & momentum conservation D Cold matter, hot matter, vacuum energy D Global geometry & topology 1.2 The cosmological redshift 10 Emission time vs. radial coordinate □ Redshifts & blueshifts D Hubble constant □ Discovery of expansion D Changing redshifts 1.3 Distances at small redshift: The Hubble constant 13 Trigonometric parallax □ Proper motions π Apparent luminosity: Main sequence, red clump stars, RR Lyrae stars, eclipsing binaries, Cepheid vari¬ ables D Tully-Fisher relation □ Faber-Jackson relation π Fundamental Plane □ Type Ia supernovae □ Surface brightness fluctuations □ Result for Hubble constant 1.4 Luminosity distances and angular diameter distances 31 Luminosity distance □ Deceleration parameter О Jerk & snap D Angular diameter distance 1.5 Dynamics of expansion 34 Einstein field equations D Friedmann equation □ Newtonian derivation □ Critical density □ Flatness problem D Matter-dominated expansion □ Radiation-dominated expansion □ Vacuum-dominated expansion Π De Sitter model □ Ωμ, Qr, Ω λ d Age of expansion □ Luminosity distance formula □ Future expansion D Historical note: cosmological constant □ Historical note: steady state model 1.6 Distances at large redshifts: Accelerated expansion 45 Discovery of accelerated expansion Π Newtonian interpretation □ Gray dust? D Discovery of early deceleration D Other effects О Equation of state parameter w О X-ray observations □ The cosmological constant problems 1.7 Cosmic expansion or tired light? 57 Surface brightness test Q Supernova decline slowdown 1.8 Ages 59 Heavy element abundance □ Main sequence turn-off □ Age vs. redshift xi Contents 1.9 Masses 65 Virialized clusters of galaxies: им □ X-ray luminosity of clusters of galaxies: Ωβ/Ωμ 1.10 Intergalactic absorption 75 Optical depth □ Resonant absorption Π 21 cm absorption □ Lyman a absorption □ Gunn-Peterson trough □ Alcock-Paczynski analysis 1.11 Number counts 82 Number vs. ζ and I □ Evolution D Radio source surveys 1.12 Quintessence 89 Scalar field theories □ Power-law potential □ Tracker solution □ Two- parameter models 1.13 Horizons 98 Particle horizon Π Event horizon 2 THE COSMIC MICROWAVE RADIATION BACKGROUND 101 2.1 Expectations and discovery of the microwave background 101 Black body radiation □ Early suggestions □ Discovery D Rayleigh-Jeans formula D CN absorption lines Π Balloons & rockets D СОВЕ & FIRAS □ Energy density Π Number density □ Effect on cosmic rays 2.2 The equilibrium era 109 Entropy per baryon □ Radiation-matter equality □ Energy decoupling 2.3 Recombination and last scattering 113 Maxwell-Boltzmann distribution □ Saha formula □ Delay of η — 2 to η = 1 □ Peebles analysis □ Lyman a escape probability □ Rate equation □ Fractional ionization D Opacity □ Jones-Wyse approximation 2.4 The dipole anisotropy 129 Angular dependence of temperature Π U2 discovery D СОВЕ & WMAP measurements □ Kinematic quadrupole 2.5 The Sunyaev-ZeI'dovich effect 132 Kompaneets equation □ Spectrum shift О Use with X-ray luminosity 2.6 Primary fluctuations in the microwave background: A first look 135 Partial-wave coefficients a¿m □ Multipole coefficients Q □ Cosmic variance Π Sachs-Wolfe effect D Harrison-Zeľdovich spectrum □ Doppler fluctua¬ tions □ Intrinsic temperature fluctuations □ Integrated Sachs-Wolfe effect D СОВЕ observations xii Contents 3 THE EARLY UNIVERSE 149 3.1 Thermal history 149 Entropy density D Fermi-Dirac & Bose-Einstein distributions □ Time vs. temperature □ Effective number of species D Neutrino decoupling Π Heating by electron-positron annihilation □ Neutrino masses & chemical potentials 3.2 Cosmological nucleosynthesis 159 Neutron-proton conversion □ Equilibrium nuclear abundances □ Deuterium bottleneck □ Helium abundance □ Deuterium abundance □ He3 abundance □ Lithium abundance D ÇiBh2 3.3 Baryonsynthesis and Leptonsynthesis 173 Sakharov conditions □ Delayed decay D Electroweak nonconservation D Leptogenesis □ Affleck-Dine mechanism □ Equilibrium baryonsynthesis 3.4 Cold dark matter 185 The bullet cluster D Leftover WIMP abundance α Sparticles □ WIMP searches О Annihilation γ rays □ Axions & axinos 4 INFLATION 201 4.1 Three puzzles 202 Flatness □ Horizons □ Monopoles 4.2 Slow-roll inflation 208 Bubble formation □ New inflation □ Slow-roll conditions π Power-law potential □ Exponential potential □ Reheating 4.3 Chaotic inflation, eternal inflation 216 Condition for eternal inflation □ Condition for chaotic inflation 5 GENERAL THEORY OF SMALL FLUCTUATIONS 219 5.1 Field equations 219 Perturbed Ricci tensor □ Perturbed energy-momentum tensor G Scalar modes D Vector modes α Tensor modes 5.2 Fourier decomposition and stochastic initial conditions 228 Plane wave solutions □ Stochastic parameters О Correlation functions Π Helicity decomposition 5.3 Choosing a gauge 235 Gauge transformations □ Newtonian gauge □ Synchronous gauge □ Conversion α Other gauges ХШ Contents 5.4 Conservation outside the horizon 245 The quantities ΊΖ and ζ □ A conservation theorem D Conservation for isolated components 6 EVOLUTION OF COSMOLOGICAL FLUCTUATIONS 257 6.1 Scalar perturbations - kinetic theory 258 Cold dark matter □ Baryonic plasma D Photon number density matrix perturbation 8nV □ Photon dimensionless intensity matrix Jy О Photon Boltzmann equations □ Photon source functions □ Photon pressure, den¬ sity, anisotropic inertia □ Photon line-of-sight solutions □ Neutrino number density perturbation bnv D Neutrino dimensionless intensity J О Neutrino Boltzmann equations D Neutrino pressure, density, anisotropic inertia □ Neutrino line-of-sight solutions □ Gravitational field equations □ Initial conditions 6.2 Scalar perturbations - the hydrodynamic limit 274 Hydrodynamic & field equations О Adiabatic initial conditions D Non- adiabatic modes □ Long & short wavelengths 6.3 Scalar perturbations - long wavelengths 282 Evolution far outside horizon □ Evolution in matter-dominated era 6.4 Scalar perturbations - short wavelengths 289 Evolution in radiation-dominated era □ Evolution deep inside horizon Π Fast & slow modes □ Matching 6.5 Scalar perturbations - interpolation & transfer functions 303 Exact solution for рв = 0 О Transfer functions О Baryon density & damp¬ ing effects 6.6 Tensor perturbations 312 Gravitational field equations D Photon Boltzmann equations Π Photon source functions □ Photon anisotropic inertia □ Photon line-of-sight sol¬ ution □ Neutrino Boltzmann equations D Neutrino anisotropic inertia □ Neutrino line-of-sight solutions □ Evolution without damping D Transfer functions □ Effect of damping 7 ANISOTROPIES IN THE MICROWAVE SKY 329 7.1 General formulas for the temperature fluctuations 329 Line-of-sight formula □ Rearrangement of scalar temperature fluctuation о Integrated Sachs-Wolfe effect □ Sudden decoupling approximation □ Re-derivation following photon trajectories □ Gauge invariance XIV Contents 7.2 Temperature multipole coefficients: Scalar modes 343 General formula □ Large I approximation □ Calculation of form fac¬ tors □ Silk & Landau damping □ Comparison with numerical codes α Balloon & ground-based observations □ WMAP D Results for cosmological parameters 7.3 Temperature multipole coefficients: Tensor modes 362 General formula □ Calculation of gravitational wave amplitude □ Calcu¬ lation of source function □ Large Ł approximation □ Sudden decoupling approximation D Numerical results 7.4 Polarization 370 Stokes parameters □ Spherical harmonics of spin ±2 □ Space-inversion properties □ E and В polarization G Scalar modes: general formula О Scalar modes: large і approximation D Scalar modes: numerical results Π Scalar modes: observations □ Tensor modes: general formula О Tensor modes: large і approximation G Tensor modes: numerical results □ Correlation functions 8 THE GROWTH OF STRUCTURE 403 8.1 Linear perturbations after recombination 403 Hydrodynamic and field equations □ Factorization of perturbations □ Effect of vacuum energy □ Power spectral function P(k) □ Correlation function ü Direct measurement of P(k) □ Rms fluctuation or □ Mea¬ surements of P(k) □ Baryon acoustic oscillations □ Cosmic variance in measuring P(k) 8.2 Nonlinear growth 421 Spherically symmetric collapse □ Calculation of ал Ο Press-Schechter mass function 8.3 Collapse of baryonic matter 427 Jeans mass □ Continuity & Euler equations □ Power-law solutions D Critical wave number for baryon collapse 9 GRAVITATIONAL LENSES 433 9.1 Lens equation for point masses 433 Derivation of lens equation □ Image separation □ Einstein ring 9.2 Magnification: Strong lensing and microlensing 436 Image luminosity α Conservation of surface brightness □ Effective radius for strong lensing □ Number counts □ De Sitter model Π Einstein-de Sitter model D Lens survey □ Microlensing observations xv Contents 9.3 Extended lenses 443 Isothermal spheres □ Lens equation □ Lens luminosity □ Number counts □ Surveys 9.4 Time delay 447 Geometrical delay □ Potential delay □ Observations 9.5 Weaklensing 452 Calculation of deflection Π Shear matrix D Ellipse matrix D Mean shear matrix □ Shear field к D Multipole coefficients □ Large í approximation D Measurement of P(k) Π Correlation functions □ Shear surveys 9.6 Cosmic strings 467 Calculation of deflection □ A string suspect 10 INFLATION AS THE ORIGIN OF COSMOLOGICAL FLUCTUATIONS 469 10.1 Scalar fluctuations during inflation 470 Scalar field action □ Field, density, pressure, and velocity perturbations D Field equations □ WKB early-time solution Π Fourier decomposition D Commutation relations □ Bunch-Davies vacuum □ Gaussian statis¬ tics □ Curvature perturbation ΊΖ □ Mukhanov-Sasaki equation D Limit TV'q outside horizon □ Number of е -foldings after horizon exit □ Expo¬ nential potential D Measurement of spectral index & fluctuation strength □ Values of exponential potential parameters D Justification of simple action 10.2 Tensor fluctuations during inflation 485 Gravitational field equation Π WKB early-time solution □ Fourier decomposition □ Commutation relations □ Scalar/tensor ratio r □ Obser¬ vational bounds on r 10.3 Fluctuations during inflation: The slow-roll approximation 488 Parameters e and б D Slow-roll approximation D Spectral index and fluc¬ tuation strength Π Observational constraints on potential □ Number of е -foldings after horizon exit 10.4 Multifield inflation 497 Gaussian, adiabatic, scale-invariant, & weak fluctuations D Thermal equi¬ librium after inflation □ Evolution equations □ WKB early-time solution D Vielbeins □ Commutation relations О Slow-roll conditions □ 7Ł after horizon exit О What we have learned about inflation xvi Contents APPENDICES A. Some Useful Numbers 509 B. Review of General Relativity 511 C. Energy Transfer between Radiation and Electrons 53 1 D. The Ergodic Theorem 537 E. Gaussian Distributions 541 F. Newtonian Cosmology 543 G. Photon Polarization 547 H. The Relativistic Boltzmann Equation 551 GLOSSARY OF SYMBOLS 565 ASSORTED PROBLEMS 569 AUTHOR INDEX 575 SUBJECT INDEX 587 XVII
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author	Weinberg, Steven 1933-2021
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format	Book
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id	DE-604.BV022969782
illustrated	Illustrated
index_date	2024-07-02T19:08:05Z
indexdate	2024-07-09T21:08:50Z
institution	BVB
isbn	9780198526827
language	English
oai_aleph_id	oai:aleph.bib-bvb.de:BVB01-016174046
oclc_num	254595506
open_access_boolean
owner	DE-91G DE-BY-TUM DE-703 DE-20 DE-19 DE-BY-UBM DE-355 DE-BY-UBR DE-29T DE-83 DE-11 DE-188 DE-92
owner_facet	DE-91G DE-BY-TUM DE-703 DE-20 DE-19 DE-BY-UBM DE-355 DE-BY-UBR DE-29T DE-83 DE-11 DE-188 DE-92
physical	XVII, 593 S. graph. Darst.
publishDate	2008
publishDateSearch	2008
publishDateSort	2008
publisher	Oxford Univ. Press
record_format	marc
spelling	Weinberg, Steven 1933-2021 Verfasser (DE-588)11562855X aut Cosmology Steven Weinberg 1. publ. Oxford [u.a.] Oxford Univ. Press 2008 XVII, 593 S. graph. Darst. txt rdacontent n rdamedia nc rdacarrier Hier auch später erschienene, unveränderte Nachdrucke Cosmologia sbt Cosmology Kosmologie (DE-588)4114294-9 gnd rswk-swf Gravitationstheorie (DE-588)4158117-9 gnd rswk-swf Relativitätstheorie (DE-588)4049363-5 gnd rswk-swf Kosmologie (DE-588)4114294-9 s Gravitationstheorie (DE-588)4158117-9 s Relativitätstheorie (DE-588)4049363-5 s DE-604 Digitalisierung UB Regensburg application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=016174046&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis
spellingShingle	Weinberg, Steven 1933-2021 Cosmology Cosmologia sbt Cosmology Kosmologie (DE-588)4114294-9 gnd Gravitationstheorie (DE-588)4158117-9 gnd Relativitätstheorie (DE-588)4049363-5 gnd
subject_GND	(DE-588)4114294-9 (DE-588)4158117-9 (DE-588)4049363-5
title	Cosmology
title_auth	Cosmology
title_exact_search	Cosmology
title_exact_search_txtP	Cosmology
title_full	Cosmology Steven Weinberg
title_fullStr	Cosmology Steven Weinberg
title_full_unstemmed	Cosmology Steven Weinberg
title_short	Cosmology
title_sort	cosmology
topic	Cosmologia sbt Cosmology Kosmologie (DE-588)4114294-9 gnd Gravitationstheorie (DE-588)4158117-9 gnd Relativitätstheorie (DE-588)4049363-5 gnd
topic_facet	Cosmologia Cosmology Kosmologie Gravitationstheorie Relativitätstheorie
url	http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=016174046&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA
work_keys_str_mv	AT weinbergsteven cosmology

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