Particle physics and inflationary cosmology linde
➤ Gửi thông báo lỗi ⚠️ Báo cáo tài liệu vi phạmNội dung chi tiết: Particle physics and inflationary cosmology linde
Particle physics and inflationary cosmology linde
arXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde 05-4060, USA'This is tin? LaTeX version of my book "Particle Physics and Inflationary Cosmology" (Harwood, Chur, Switzerland, 1990).AbstractThis is the LaTeX version of my book “Particle Physics and Inflationary Cosmology” (Harwood. Chur. Switzerland. 1990). I decided to put it to hep-th, to make it Particle physics and inflationary cosmology linde easily available. Many things hapi>ened during the 15 years since the time when it was written. In particular, we have learned a lot about the high tParticle physics and inflationary cosmology linde
emperature behavior in the electroweak theory and about baryogenesis. A discovery of the acceleration of the universe has changed the way we are thinkarXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde nt cosmological observations have shown that the universe is Hat, or almost exactly Hat, and confirmed many other predictions of inflationary theory. Many new versions of this theory have been developed, including hybrid inflation and inflationary models based on string theory. There was a substanti Particle physics and inflationary cosmology linde al progress in the theory of reheating of the universe after inflation, and in the theory of eternal inflation.It s clear, therefore, that some partsParticle physics and inflationary cosmology linde
of the book should be updated, which I might do sometimes in the future. I hope, however, that this book may be of some interest even in its original arXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde d suggest to read this book in parallel with the book by Liddle and Lyth "Cosmological Inflation and Large Scale Structure.” with the book by Mukhanov “Physical Foundations of Cosmology,” which is to be published soon, and with my review article hep-th/0503195, which contains a discussion of some (b Particle physics and inflationary cosmology linde ut certainly not all) of the recent developments in inflationary theory.VAVw.pdfgrip.comContentsPreface to the SeriesIntroductionxiCHAPTER 1 CHAPTER 2Particle physics and inflationary cosmology linde
Overview of Unified Theories of Elementary Particles and the Inflationary Universe Scenario 1.1The scalar field and spontaneous symmetry breaking 1.2ParXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde of the development of the inflationary universe scenario 1.7The chaotic inflation scenario 1.8The self-reproducing universe 1.9Summary Scalar Field, Effective Potential, and Spontaneous Symmetry Breaking 2.1Classical and quantum .scalar fields 2.2Quantum corrections to the effective potential V(yd 2 Particle physics and inflationary cosmology linde .3The 1/N expansion and the effective potential in the A^>4/N theory 2.1 The effective potential and quantum gravitational effects1 1 6 9 13 16 25 29Particle physics and inflationary cosmology linde
42 49 50 50 53 59 61CHAPTER 3Restoration of Symmetry al High Temperature 3.1Phase transitions in the simplest models with spontaneous symmetry breakinarXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde he infrared problem ill the thermodynamics of gauge fields67 67 72 74CHAPTER 4Phase Transitions in Cold s 11 perde use Matter 4.1 Restoration of symmetry ill theories with no neutral currents78 78VA»AV. pdfgrip.comCONTENTSviii4.2 Enhancement of symmetry breaking and thecondensation of vector mesons Particle physics and inflationary cosmology linde in theories withneutral currents79CHAPTER 5Tunneling Theory and the Decay of a Metastable Phase in a First- Order Phase Transition82 5.1General theoryParticle physics and inflationary cosmology linde
of the formation of bubbles of a new phase82 5.2The thin-wall approximation86 5.3Beyond the thin-wall approximation90CHAPTER 6Phase Transitions in a arXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde d monopoles99CHAPTER 7General Principles of Inflationary Cosmology108 7.1Introduction108 7.2The inflationary universe and de Sitterspace109 7.3Quantum fluctuations in the inflationary universe113 7.4Tunneling in the inflationary universe120 7.5Quantum fluctuat ions and the generation of adiabatic de Particle physics and inflationary cosmology linde nsity perturbations126 7.6Are scale-free adiabatic perturbations sufficient to produce the observed large scale structure of the universe?136 7.7IsothParticle physics and inflationary cosmology linde
ermal perturbations and adiabatic perturbations with a nonflat spectrum139 7.8Nonperturbative effects: strings, hedgehogs, walls, bubbles,...145 7.9RearXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430 Particle physics and inflationary cosmology linde ationary universe scenario160 8.2The Coleman Weinberg SU(5) theory and the new inflationary universe scenario (initial simplified version)162 8.3Refinement of the new inflationary universe scenario165 8.4Primordial inflation in N = 1 supergravity170 8.5The Shafi-Vilenkin model171 8.6The new inflatio Particle physics and inflationary cosmology linde nary universe scenario: problems and prospects 176CHAPTER 9The Chaotic Inflation Scenario179 9.1 Introduction. Basic features of the scenario. The queParticle physics and inflationary cosmology linde
stion of initial conditions179VAVw.pdfgrip.comCONTENTSLx9.2The simplest model based on the SU(5) theory1829.3Chaotic inHation in supergravity1849.4ThearXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430arXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430Gọi ngay
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