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书名 光的相干与偏振理论导论(影印版)/引进系列/中外物理学精品书系
分类 科学技术-自然科学-物理
作者 (美)沃尔夫
出版社 北京大学出版社
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简介
目录

Preface page xi

1. Elementary coherence phenomena

 1.1 Interference and statistical similarity

 1.2 Temporal coherence and the coherence time

 1.3 Spatial coherence and the coherence area

 1.4 The coherence volume

 Problems

2. Mathematical preliminaries

 2.1 Elementary concepts of the theory of random processes

 2.2 Ergodicity

 2.3 Complex representation of a real signal and the envelope of a narrow-band signal

 2.4 The autocorrelation and the cross-correlation functions

2.4.1 The autocorrelation function of a finite sum of periodic components with random amplitudes

 2.5 The spectral density and the Wiener-Khintchine theorem

 Problems

3. Second-order coherence phenomena in the space-time domain

 3.1 Interference law for stationary optical fields. The mutual coherence function and the complex degree of coherence

 3.2 Generation of spatial coherence from an incoherent source. The van Cittert-Zernike theorem

 3.3 Illustrative examples

3.3.1 Michelson's method for measuring stellar diameters

3.3.2 Michelson's method for determining energy distribution in spectral lines

 3.4 Propagation of the mutual intensity

 3.5 Wave equations for the propagation of mutual coherence in free space

 Problems

4. Second-order coherence phenomena in the space-frequency domain

 4.1 Coherent-mode representation and the cross-spectral density as a correlation function

 4.2 The spectral interference law and the spectral degree of coherence

 4.3 An illustrative example: spectral changes on interference

 4.4 Interference of narrow-band light

 Problems

5. Radiation from sources of different states of coherence

 5.1 Fields generated by sources with different coherence properties

 5.2 Correlations and the spectral density in the far field

 5.3 Radiation from some model sources

5.3.1 Schell-model sources

5.3.2 Quasi-homogeneous sources

 5.4 Sources of different states of spatial coherence which generate identical distributions of the radiant intensity

 5.5 Coherence properties of Lambertian sources

 5.6 Spectral changes on propagation. The scaling law

 Problems

6. Coherence effects in scattering

 6.1 Scattering of a monochromatic plane wave on a deterministic medium

 6.2 Scattering of partially coherent waves on a deterministic medium

 6.3 Scattering on random media

6.3.1 General formulas

6.3.2 Examples

6.3.3 Scattering on a quasi-homogeneous medium

 Problems

7. Higher-order coherence effects

 7.1 Introduction

 7.2 Intensity interferometry with radio waves

 7.3 The Hanbury Brown-Twiss effect and intensity interferometry with light

 7.4 Einstein's formula for energy fluctuations in blackbody radiation and the wave-particle duality

 7.5 Mandel's theory of photoelectric detection of light fluctuations

7.5.1 Mandel's formula for photocount statistics

7.5.2 The variance of counts from a single photodetector

7.5.3 Correlation between count fluctuations from two detectors

 7.6 Determination of statistical properties of light from photocount measurements

 Problems

8. Elementary theory of polarization of stochastic electromagnetic beams

 8.1 The 2 _ 2 equal-time correlation matrix of a quasi-monochromatic electromagnetic beam

 8.2 Polarized, unpolarized and partially polarized light. The degree of polarization

8.2.1 Completely polarized light

8.2.2 Natural (unpolarized) light

8.2.3 Partially polarized light and the degree of polarization

8.2.4 The geometrical significance of complete polarization. The Stokes parameters of completely polarized light. The Poincaré sphere

 Problems

9. Unified theory of polarization and coherence

 9.1 The 2 × 2 cross-spectral density matrix of a stochastic electromagnetic beam

 9.2 The spectral interference law, the spectral degree of coherence and the spectral degree of polarization of stochastic electromagnetic beams

 9.3 Determination of the cross-spectral density matrix from experiments

 9.4 Changes in random electromagnetic beams on propagation

9.4.1 Propagation of the cross-spectral density matrix of a stochastic electromagnetic beam - general formulas

9.4.2 Propagation of the cross-spectral density matrix of an electromagnetic Gaussian Schell-model beam

9.4.3 Examples of correlation-induced changes in stochastic electromagnetic beams on propagation

9.4.4 Coherence-induced changes of the degree of polarization in Young's interference experiment

 9.5 Generalized Stokes parameters

 Problems

Appendices

 Ⅰ Cells of phase space and the degeneracy parameter

(a) Cells of phase space of a quasi-monochromatic light wave (Section 1.4)

(b) Cells of phase space of radiation in a cavity (Sections 7.4 and 7.5)

(c) The degeneracy parameter

 Ⅱ Derivation of Mandel's formula for photocount statistics [Eq. (2) of Section 7.5.1]

 Ⅲ The degree of polarization of an electromagnetic Gaussian Schell-model source

 Ⅳ Some important probability distributions

(a) The binomial (or Bernoulli) distribution and some of its limiting cases

(b) The Bose-Einstein distribution

Author index

Subject index

编辑推荐

光的相干和偏振是光学中最重要的现象,其应用也极为广泛。《光的相干与偏振理论导论(英文影印版)》的作者是国际光学界的著名学者沃尔夫,在相关的研究取中取得过突破性的进展。也正是因为作者的贡献,本书能够以统一处理方法研究光的相干与偏振这两种现象。对于光通信、光学成像等领域的研究者及研究生,乃至对此领域感兴趣的读者来说,本书是不可多得的优秀读物。

内容推荐
所有的光场都是随机涨落的, 有些光场的随机涨落很小, 例如许多激光器输出的光 ; 有些光场的随机涨落相当大, 例如从热光源辐射的光。描述涨落光场的基础理论是相干理论。部分偏振现象就是涨落的重要表现。实际上, 相干理论所能处理的问题不仅限于涨落。与常规的处理方法不同, 相干理论是依据可观测量描述光场, 并解释这些可观测量, 例如光的光谱以及它在传输中如何变化的。本书给出了光的相干与偏振现象的统一处理方法。
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