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引力的量子效應(yīng)導(dǎo)論

引力的量子效應(yīng)導(dǎo)論

定 價(jià):¥45.00

作 者: (德)馬克翰維 著
出版社: 世界圖書出版公司
叢編項(xiàng):
標(biāo) 簽: 理論物理學(xué)

ISBN: 9787510005527 出版時(shí)間: 2010-04-01 包裝: 平裝
開本: 16開 頁數(shù): 273 字?jǐn)?shù):  

內(nèi)容簡介

  本書系統(tǒng)地介紹了引力中的量子場論方法,適合用作理論天體物理,宇宙學(xué),粒子物理和超弦理論等專業(yè)的本科生和研究生教材。本書首先介紹了量子場論中的一般概念,重點(diǎn)講解了利用量子場論方法研究引力,同時(shí)還介紹了基本且必要的不斷擴(kuò)張宇宙中的場量子化和膨脹時(shí)空中的量子漲落。此外,本書還詳細(xì)討論了Casimir效應(yīng),Unruh效應(yīng)和霍金效應(yīng),并介紹了計(jì)算外部重力場中量子系統(tǒng)的反向反應(yīng)的有效作用量。作者從最初的基本原理出發(fā),經(jīng)過演繹得出最終結(jié)果,并對最終結(jié)果做詳細(xì)的解釋,幫助讀者對該領(lǐng)域建立完整的物理圖像。本書內(nèi)容全面,講解深刻,附有習(xí)題及其答案。閱讀本書只需要基本的廣義相對論知識。前言;(第一部分)正則量子化和粒子產(chǎn)生:概述:量子場;回顧:經(jīng)典和量子理論;受迫諧振子;從諧振子到場;回顧:經(jīng)典場;擴(kuò)張宇宙中的量子場;Sitter宇宙中的量子場;Unruh效應(yīng);Hawking效應(yīng),黑洞熱力學(xué);Casimir效應(yīng);(第二部分)路徑積分和真空極化:路徑積分;有效作用量;熱核計(jì)算;從有效作用量導(dǎo)出的結(jié)論;附錄1:數(shù)學(xué)補(bǔ)充;附錄2:反向反應(yīng)的有效作用量推導(dǎo);附錄3:模展開要點(diǎn);附錄4:習(xí)題答案;索引。讀者對象:理論天體物理,宇宙學(xué),粒子物理和超弦理論等專業(yè)的高年級本科生、研究生和相關(guān)領(lǐng)域的科研人員。

作者簡介

暫缺《引力的量子效應(yīng)導(dǎo)論》作者簡介

圖書目錄

Preface
Part I Canonical quantization and particle production
 1 Overview: a taste of quantum fields
  1.1 Classical field
  1.2 Quantum field and its vacuum state
  1.3 The vacuum energy
  1.4 Quantum vacuum fluctuations
  1.5 Particle interpretation of quantum fields
  1.6 Quantum field theory in classical backgrounds
  1.7 Examples of particle creation
 2 Reminder: classical and quantum theory
  2.1 Lagrangian formalism
  2.1.1 Functional derivatives
  2.2 Hamiltonian formalism
  2.3 Quantization of Hamiltonian systems
  2.4 Hilbert spaces and Dirac notation
  2.5 Operators, eigenvalue problem and basis in a Hilbert space
  2.6 Generalized eigenvectors and basic matrix elements
  2.7 Evolution in quantum theory
 3 Driven harmonic oscillator
  3.1 Quantizing an oscillator
  3.2 The "in" and "out" states
  3.3 Matrix elements and Green's functions
 4 From harmonic oscillators to fields
  4.1 Quantum harmonic oscillators
  4.2 From oscillators to fields
  4.3 Quantizing fields in a flat spacetime
  4.4 The mode expansion
  4.5 Vacuum energy and vacuum fluctuations
  4.6 The Schr'odinger equation for a quantum field
 5 Reminder: classical fields
  5.1 The action functional
  5.2 Real scalar field and its coupling to the gravity
  5.3 Gauge invariance and coupling to the electromagnetic field
  5.4 Action for the gravitational and gauge fields
  5.5 Energy-momentum tensor
 6 Quantum fields in expanding universe
  6.1 Classical scalar field in expanding background
  6.1.1 Mode expansion
  6.2 Quantization
  6.3 Bogolyubov transformations
  6.4 Hilbert space; "a- and b-particles"
  6.5 Choice of the physical vacuum
  6.5.1 The instantaneous lowest-energy state
  6.5.2 Ambiguity of the vacuum state
  6.6 Amplitude of quantum fluctuations
  6.6.1 Comparing fluctuations in the vacuum and excited states
  6.7 An example of particle production
 7 Quantum fields in the de Sitter universe
  7.1 De Sitter universe
  7.2 Quantization
  7.2.1 Bunch-Davies vacuum
  7.3 Fluctuations in inflationary universe
 8 Unruh effect
  8.1 Accelerated motion
  8.2 Comoving frame of accelerated observer
  8.3 Quantum fields in inertial and accelerated frames
  8.4 Bogolyubov transformations
  8.5 Occupation numbers and Unmh temperature
 9 Hawking effect. Thermodynamics of black holes
  9.1 Hawking radiation
  9.1.1 Schwarzschild solution
  9.1.2 Kruskal-Szekeres coordinates
  9.1.3 Field quantization and Hawking radiation
  9.1.4 Hawking effect in 3 + 1 dimensions
  9.2 Therroodynamics of black holes
  9.2.1 Laws of black.hole thermodynamics
 10 The Casimir effect
  10.1 Vacuum energy betw.een plates
  10.2 Regularization and renormalization
Part II Path integrals and vacuum polarization
 11 Path integrals
  11.1 Evolution operator. Propagator
  11.2 Propagator as a path integral
  11.3 Lagrangian path integrals
  11.4 Propagators for free particle and harmonic oscillator
  11.4.1 Free particle
  11.4.2 Quadratic potential
  11.4.3 Euclidean path integral
  11.4.4 Ground state as a path integral
 12 Effective action
  12.1 Driven harmonic oscillator (continuation)
  12.1.1 Green's functions and matrix elements
  12.1.2 Euclidean Green's function
  12.1.3 Introducing effective action
  12.1.4 Calculating effective action for a driven oscillator
  12.1.5 Matrix elements
  12.1.6 The effective action "recipe"
  12.1.7 Backreaction
  12.2 Effective action in external gravitational field
  12.2.1 Euclidean action for scalar field
  12.3 Effective action as a functional determinant
  12.3.1 Reformulation of the eigenvalue problem
  12.3.2 Zeta function
  12.3.3 Heat kernel
 13 Calculation of heat kernel
  13.1 Perturbative expansion for the heat kernel
  13.1.1 Matrix elements
  13.2 Trace of the heat kernel
  13.3 The Seeley-DeWitt expansion
 14 Results from effective action
  14.1 Renormalization of the effective action
  14.2 Finite terms in the effective action
  14.2.1 EMT from the Polyakov action
  14.3 Conformal anomaly
Appendix 1 Mathematical supplement
 A1.1 Functionals and distributions (generalized functions)
 A1.2 Green's functions, boundary conditions, and contours
 A1.3 Euler's gamma function and analytic continuations
Appendix 2 Backreaction derived from effective action
Appendix 3 Mode expansions cheat sheet
Appendix 4 Solutions to exercises
Index

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