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Record ID marc_nuls/NULS_PHC_180925.mrc:84213786:6984
Source marc_nuls
Download Link /show-records/marc_nuls/NULS_PHC_180925.mrc:84213786:6984?format=raw

LEADER: 06984cam 2200421 i 4500
001 9925318603801661
005 20180808104351.0
007 cr#cnunnn|uu|u
008 150113t20152015enka b 001 0 eng
010 $a 2015001070
019 $a921124116$a921873511$a940929030$a942844064$a951476465$a983781221$a990686064
020 $a9781118502099$q(pbk. ;$qalk. paper)
020 $a1118502094$q(pbk. ;$qalk. paper)
020 $a9781118502143
020 $a1118502140
035 $a99977204270
035 $a(OCoLC)890068133$z(OCoLC)921124116$z(OCoLC)921873511$z(OCoLC)940929030$z(OCoLC)942844064$z(OCoLC)951476465$z(OCoLC)983781221$z(OCoLC)990686064
035 $a(OCoLC)ocn890068133
040 $aDLC$beng$erda$cDLC$dYDXCP$dOCLCF$dHEBIS$dSDB$dCDX$dIAC$dCUY$dERL$dGZM$dZ5A$dLIP$dOCLCO$dOCLCQ
042 $apcc
050 00 $aQB981$b.L567 2015
082 00 $a523.1$223
100 1 $aLiddle, Andrew R.
245 13 $aAn introduction to modern cosmology /$cAndrew Liddle, Institute for Astronomy, University of Edinburgh, Abbreviate to 'UK'.
250 $aThird edition.
264 1 $aChichester, West Sussex :$bJohn Wiley and Sons, Inc.,$c2015.
300 $axv, 182 pages :$billustrations ;$c23 cm
336 $atext$btxt$2rdacontent
337 $aunmediated$bn$2rdamedia
338 $avolume$bnc$2rdacarrier
504 $aIncludes bibliographical references and index.
505 0 $a1. A (Very) Brief History of Cosmological Ideas -- 2. Observational Overview -- 3. Newtonian Gravity -- 4. The Geometry of the Universe -- 5. Simple Cosmological Models -- 6. Observational Parameters -- 7. The Cosmological Constant -- 8. The Age of the Universe -- 9. The Density of the Universe and Dark Matter -- 10. The Cosmic Microwave Background -- 11. The Early Universe -- 12. Nucleosynthesis: The Origin of the Light Elements -- 13. The Inflationary Universe -- 14. The Initial Singularity -- 15. Overview: The Standard Cosmological Model.
505 00 $g1.$tA (Very) Brief History of Cosmological Ideas --$g2.$tObservational Overview --$t2.1 In visible light --$t2.2 In other wavebands --$t2.3 Homogeneity and isotropy --$t2.4 The expansion of the Universe --$t2.5 Particles in the Universe --$g3.$tNewtonian Gravity --$t3.1 The Friedmann equation --$t3.2 On the meaning of the expansion --$t3.3 Things that go faster than light --$t3.4 The fluid equation --$t3.5 The acceleration equation --$t3.6 On mass, energy and vanishing factors of c2 --$g4.$tThe Geometry of the Universe --$t4.1 Flat geometry --$t4.2 Spherical geometry --$t4.3 Hyperbolic geometry --$t4.4 Infinite and observable Universes --$t4.5 Where did the Big Bang happen? --$t4.6 Three values of k --$g5.$tSimple Cosmological Models --$t5.1 Hubble's law --$t5.2 Expansion and redshift --$t5.3 Solving the equations --$t5.4 Particle number densities --$t5.5 Evolution including curvature --$g6.$tObservational Parameters --$t6.1 The expansion rate H0 --$t6.2 The density parameter 0 --$t6.3 The deceleration parameter q0 --$g7.$tThe Cosmological Constant --$t7.1 Introducing _ --$t7.2 Fluid description of _ --$t7.3 Cosmological models with _ --$g8.$tThe Age of the Universe --$g9.$tThe Density of the Universe and Dark Matter --$t9.1 Weighing the Universe --$t9.2 What might the dark matter be? --$t9.3 Dark matter searches --$g10.$tThe Cosmic Microwave Background --$t10.1 Properties of the microwave background --$t10.2 The photon to baryon ratio --$t10.3 The origin of the microwave background --$t10.4 The origin of the microwave background (advanced) --$g11.$tThe Early Universe --$g12.$tNucleosynthesis: The Origin of the Light Elements --$t12.1 Hydrogen and Helium --$t12.2 Comparing with observations --$t12.3 Contrasting decoupling and nucleosynthesis --$g13.$tThe Inflationary Universe --$t13.1 Problems with the Hot Big Bang --$t13.2 Inflationary expansion --$t13.3 Solving the Big Bang problems --$t13.4 How much inflation? --$t13.5 Inflation and particle physics --$g14.$tThe Initial Singularity --$g15.$tOverview: The Standard Cosmological Model --$tAdvanced Topic 1 General Relativistic Cosmology --$t1.1 The metric of space-time --$t1.2 The Einstein equations --$t1.3 Aside: Topology of the Universe --$tAdvanced Topic 2 Classic Cosmology: Distances and Luminosities --$t2.1 Light propagation and redshift --$t2.2 The observable Universe --$t2.3 Luminosity distance --$t2.4 Angular diameter distance --$t2.5 Source counts --$tAdvanced Topic 3 Neutrino Cosmology --$t3.1 The massless case --$t3.2 Massive neutrinos --$t3.3 Neutrinos and structure formation --$tAdvanced Topic 4 Baryogenesis --$tAdvanced Topic 5 Structures in the Universe --$t5.1 The observed structures --$t5.2 Gravitational instability --$t5.3 The clustering of galaxies --$t5.4 Cosmic microwave background anisotropies --$t5.5 The origin of structure --$tAdvanced Topic 6 Constraining cosmological models --$t6.1 Cosmological models and parameters --$t6.2 Key cosmological observations --$t6.3 Cosmological data analysis --$t6.4 The Standard Cosmological Model: 2014 edition --$t6.5 The future.
520 $a"An Introduction to Modern Cosmology Third Edition is an accessible account of modern cosmological ideas. The Big Bang Cosmology is explored, looking at its observational successes in explaining the expansion of the Universe, the existence and properties of the cosmic microwave background, and the origin of light elements in the universe. Properties of the very early Universe are also covered, including the motivation for a rapid period of expansion known as cosmological inflation. The third edition brings this established undergraduate textbook up-to-date with the rapidly evolving observational situation. This fully revised edition of a bestseller takes an approach which is grounded in physics with a logical flow of chapters leading the reader from basic ideas of the expansion described by the Friedman equations to some of the more advanced ideas about the early universe. It also incorporates up-to-date results from the Planck mission, which imaged the anisotropies of the Cosmic Microwave Background radiation over the whole sky. The Advanced Topic sections present subjects with more detailed mathematical approaches to give greater depth to discussions. Student problems with hints for solving them and numerical answers are embedded in the chapters to facilitate the reader's understanding and learning. Cosmology is now part of the core in many degree programs. This current, clear and concise introductory text is relevant to a wide range of astronomy programs worldwide and is essential reading for undergraduates and Masters students, as well as anyone starting research in cosmology"--Publisher's website.
650 0 $aCosmology.
776 08 $iOnline version:$aLiddle, Andrew R.$tIntroduction to modern cosmology.$bThird edition.$dChichester, West Sussex : John Wiley and Sons, Inc., 2015$z9781118690277$w(DLC) 2015001688
947 $hCIRCSTACKS$r31786103081565
980 $a99977204270