有限温度场论原理和应用 第2版 卡普斯塔 世界图书出版公司【正版书】 azw3 极速 lit 地址 下载 rb pdf mobi

what happens when ordinary matter is sogreatly pressed that the electrons form a relativisticdegenerate gas, as in a white dwarf star? what happens when thematter is pressed even further so that atomic nuclei overlap toform superdense nuclear matter, as in a neutron star? what happenswhen nuclear matter is heated to such great temperatures that thenucleons and pions melt into quarks and gluons, as in high-energynuclear collisions? what happened in the spontaneous symmetrybreak-ing of the unified theory of the weak and electromagicinteractions during the big bang? questions like these havefascinated us for a long time. the purpose of thiook is todevelop the fundamental principles and mathematical techniques thatenable the formulation of answers to these mind-boggling questions.the study of matter under extreme con-ditions halossomed into afield of intense interdisciplinary activity and global extent. theanalysis of the collective behavior of interacting rela-tivisticsystems spans a rich palette of physical phenomena. one of theultimate goals of the whole program is to map out the phase diagramof the standard model and its extensions.　　what happens when ordinary matter is sogreatly pressed that the electrons form a relativisticdegenerate gas, as in a white dwarf star? what happens when thematter is pressed even further so that atomic nuclei overlap toform superdense nuclear matter, as in a neutron star? what happenswhen nuclear matter is heated to such great temperatures that thenucleons and pions melt into quarks and gluons, as in high-energynuclear collisions? what happened in the spontaneous symmetrybreak-ing of the unified theory of the weak and electromagicinteractions during the big bang? questions like these havefascinated us for a long time. the purpose of thiook is todevelop the fundamental principles and mathematical techniques thatenable the formulation of answers to these mind-boggling questions.the study of matter under extreme con-ditions halossomed into afield of intense interdisciplinary activity and global extent. theanalysis of the collective behavior of interacting rela-tivisticsystems spans a rich palette of physical phenomena. one of theultimate goals of the whole program is to map out the phase diagramof the standard model and its extensions.

this text assumes that the reader has pleted graduate levelcourses in thermal and statistical physics and in relativisticquantum field theory.our aims are to convey a coherent picture ofthe field and to prepare the reader to read and understand theoriginal and current literature. the book is not, however, apendium of all known results; this would havemade itprohibitively long. we start from the basic principles ofquantumfield theory, thermodynamics, and statistical mechanics.this develop-ment is most elegantly acplished by means offeynman's functionalintegral formalism. having a functionalintegral expression for the parti-tion function allows astraightforward derivation of diagrammatic rules for interactingfield theories. it also provides a framework for defining gaugetheories on finite lattices, which then enables integration bymonte carlo techniques. the formal aspects are illustrated withapplications drawn from fields of research that are close to theauthors' own experience. eachchapter carries its own exercises,reference list, and select bibliography.the book iased onfinite-temperature field theory, written by one of us (jk) andpublished in 1989. although the fundamental principles have notchanged, there have been many important developments since then,necessitating a new book.

preface

1review of quantum statistical mechanics

　1.1ensembles

　1.2one bosonic degree of freedom

　1.3one fermionic-degree of freedom

　1.4noninteracting gases

　1.5exercises

　bibliography

2functional integral representation of the partition functio

　2.1transition amplitude for bosons

　2.2partition function for bosons

　2.3neutral scalar field

　2.4bose-einstein condensatio

　2.5fermions

　2.6remarks on functional integrals

　2.7exercises

　reference

　bibliography

3 interactions and diagrammatic techniques

　3.1perturbation expansio

　3.2diagrammatic rules forλφ4 theory

　3.3propagators

　3.4first-order corrections to il and in z

　3.5summation of infrared divergences

　3.6yukawa theory

　3.7remarks on real time perturbation theory

　3.8exercises

　references

　bibliography

4renormalizatio

　4.1renormalizingλφ4 theory

　4.2renormalization group

　4.3regularization schemes

　4.4application to the partition functio

　4.5exercises

　references

　bibliography

5quantum electrodynamics

　5.1quantizing the electromagic field

　5.2blackbody radiatio

　5.3diagrammatic expansio

　5.4photon self-energy

　5.5loop corrections to in z

　5.6exercises

　references

　bibliography

6linear response theory

　6.1linear response to an external field

　6.2lehmann representatio

　6.3screening of static electric fields

　6.4screening of a point charge

　6.5exact formula for screening length in qed

　6.6collective excitations

　6.7photon dispersion relatio

　6.8electron dispersion relatio

　6.9kubo formulae for viscosities and conductivities

　6.10 exercises

　references

　bibliography

7 spontaneous symmetry breaking and restoratio

　7.1charged scalar field with mass-squared

　7.2goldstone's theorem

　7.3loop corrections

　7.4higgs model

　7.5exercises

　references

　bibliography

8quantum chromodynamics

　8.1quarks and gluons

　8.2asymptotic freedom

　8.3perturbative evaluation of partition functio

　8.4higher orders at finite temperature

　8.5gluon propagator and linear response

　8.6instantons

　8.7infrared problems

　8.8strange quark matter

　8.9color superconductivity

　8.10 exercises

　references

　bibliography

9resummation and hard thermal loops

　9.1isolating the hard thermal loop contributio

　9.2hard thermal loops and ward identities

　9.3hard thermal loops and effective perturbation theory

　9.4spectral densities

　9.5kiic theory

　9.6transport coefficients

　9.7exercises

　references

10lattice gauge theory

　10.1 abelian gauge theory

　10.2 nonabelian gauge theory

　10.3 fermions

　10.4 phase transitions in pure gauge theory

　10.5 lattice qcd

　10.6 exercises

　references

　bibliography

11dense nuclear matter

12hot hadronic matter

13nucleation theory

14heavy ion collisions

15weak interactions

16 astrophysics and cosmology

appendix

index

作者：（美国）卡普斯塔（Joseph I. Kapusta） （美国）Charles Gale

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《有限温度场论原理和应用(第2版)》主要内容：what happens when ordinary matter is so greatly compressed that the electrons form a relativistic degenerate gas, as in a white dwarf star? what happens when the matter is compressed even further so that atomic nuclei overlap to form superdense nuclear matter, as in a neutron star? what happens when nuclear matter is heated to such great temperatures that the nucleons and pions melt into quarks and gluons, as in high-energy nuclear collisions? what happened in the spontaneous symmetry break-ing of the unified theory of the weak and electromagnetic interactions during the big bang? questions like these have fascinated us for a long time. the purpose of this book is to develop the fundamental principles and mathematical techniques that enable the formulation of answers to these mind-boggling questions. the study of matter under extreme con-ditions has blossomed into a field of intense interdisciplinary activity and global extent. the analysis of the collective behavior of interacting rela-tivistic systems spans a rich palette of physical phenomena. one of the ultimate goals of the whole program is to map out the phase diagram of the standard model and its extensions.