KHO THƯ VIỆN 🔎

Particle physics and inflationary cosmology linde

➤  Gửi thông báo lỗi    ⚠️ Báo cáo tài liệu vi phạm

Loại tài liệu:     PDF
Số trang:         270 Trang
Tài liệu:           ✅  ĐÃ ĐƯỢC PHÊ DUYỆT
 













Nội 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 th

e 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 t

Particle 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 think

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 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 parts

Particle 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 2

Particle 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 1.2P

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 of the development of the inflationary universe scenario 1.7The chaotic inflation scenario 1.8The self-reproducing universe 1.9Summary Scalar Field, E

ffective 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 29

Particle 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 breakin

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 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 symme

try 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 theory

Particle 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 7.7Isoth

Particle physics and inflationary cosmology linde

ermal perturbations and adiabatic perturbations with a nonflat spectrum139 7.8Nonperturbative effects: strings, hedgehogs, walls, bubbles,...145 7.9Re

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 ationary universe scenario160 8.2The Coleman Weinberg SU(5) theory and the new inflationary universe scenario (initial simplified version)162 8.3Refin

ement 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 que

Particle physics and inflationary cosmology linde

stion of initial conditions179VAVw.pdfgrip.comCONTENTSLx9.2The simplest model based on the SU(5) theory1829.3Chaotic inHation in supergravity1849.4The

arXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430

arXiv:hep-th/0503203 V1 26 Mar 2005PARTICLE PHYSICSAND INFLATIONARY COSMOLOGY1Andrei LindeDepartment of Physics, Stanford University, Stanford CA 9430

Gọi ngay
Chat zalo
Facebook