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what happens when ordinary matter is sogreatly pressed that the electr*** 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 thenucle*** and pi*** melt into quarks and glu***, as in high-energynuclear collisi***? what happened in the spontaneous symmetrybreak-ing of the unified theory of the weak and electromagicin***cti*** during the big bang? questi*** 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 questi***.the study of matter under extreme con-diti*** halossomed into afield of intense interdisciplinary activity and global extent. the***ysis of the collective behavior of in***cting rela-tivisticsystems spans a rich palette of physical phenomena. one of theultimate goals of the w*** program is to map out the phase diagramof the standard model and its extensi***. what happens when ordinary matter is sogreatly pressed that the electr*** 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 thenucle*** and pi*** melt into quarks and glu***, as in high-energynuclear collisi***? what happened in the spontaneous symmetrybreak-ing of the unified theory of the weak and electromagicin***cti*** during the big bang? questi*** 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 questi***.the study of matter under extreme con-diti*** halossomed into afield of intense interdisciplinary activity and global extent. the***ysis of the collective behavior of in***cting rela-tivisticsystems spans a rich palette of physical phenomena. one of theultimate goals of the w*** program is to map out the phase diagramof the standard model and its extensi***.
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 li***ture. 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 in***ctingfield theories. it also provides a framework for defining gaugetheories on finite lattices, which then enables integration bymonte carlo techniques. the formal ***ects are illustrated withapplicati*** 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.
书籍目录:
preface
1review of quantum statistical mechanics
1.1ensembles
1.2one bosonic degree of ***
1.3one fermionic-degree of ***
1.4nonin***cting gases
1.5exercises
bibliography
2functional integral representation of the partition functio
2.1transition amplitude for bos***
2.2partition function for bos***
2.3neutral scalar field
2.4bose-einstein condensatio
2.5fermi***
2.6remarks on functional integrals
2.7exercises
reference
bibliography
3 in***cti*** and diagrammatic techniques
3.1perturbation expansio
3.2diagrammatic rules forλφ4 theory
3.3propagators
3.4first-order correcti*** 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
5.4p***on self-energy
5.5loop correcti*** to in z
5.6exercises
references
bibliography
6linear resp***e theory
6.1linear resp***e to an external field
6.2lehmann representatio
6.3screening of static electric fields
***screening of a point charge
6.5exact formula for screening length in qed
6.6collective excitati***
6.7p***on 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 correcti***
7.4higgs model
7.5exercises
references
bibliography
8quantum chromodynamics
8.1quarks and glu***
8.2asymptotic ***
8.3perturbative evaluation of partition functio
8.4higher orders at finite temperature
8.5gluon propagator and linear resp***e
8.6instant***
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 fermi***
10.4 phase transiti*** in pure gauge theory
10.5 lattice qcd
10.6 exercises
references
bibliography
11dense nuclear matter
12*** hadronic matter
13nucleation theory
14heavy ion collisi***
15weak in***cti***
16 astrophysics and cosmology
appendix
index
作者介绍:
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 electr*** 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 nucle*** and pi*** melt into quarks and glu***, as in high-energy nuclear collisi***? what happened in the spontaneous symmetry break-ing of the unified theory of the weak and electromagnetic in***cti*** during the big bang? questi*** 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 questi***. the study of matter under extreme con-diti*** has blossomed into a field of intense interdisciplinary activity and global extent. the ***ysis of the collective behavior of in***cting rela-tivistic systems spans a rich palette of physical phenomena. one of the ultimate goals of the w*** program is to map out the phase diagram of the standard model and its extensi***.
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