Intermediate Quantum Mechanics: Third Edition
暫譯: 中級量子力學：第三版

對於理論與實驗物理的研究生來說，這本於1986年精煉和更新的《中級量子力學》第三版是不可或缺的。書的第一部分探討原子結構的理論，而第二和第三部分則涉及相對論波動方程及場論的介紹，使得《中級量子力學》比其他任何單卷作品更為完整。

Hans A. Bethe took his Ph.D. in Munich in 1928. In 1935, he came to Cornell University, where he is now Professor Emeritus. In 1967, he received the Nobel Prize in Physics, primarily for his explanation of the processes by which stars produce their energy. His early scientific work was mainly in the theory of atoms, of the solid state, and of atomic collisions. Later he concentrated on nuclear physics. His explanation of stellar energy grew out of his work in nuclear theory. Recently, he has worked on neutron stars and supernova stars. Roman Jackiw has been professor of physics at the Massachusetts Institute of Technology since 1969, after spending three years as a Junior Fellow with Harvard University's Society of Fellows. His primary research area is theoretical physics and he has contributed to particle, condensed matter, and gravitational physics. Recently he received the Dannie Heineman Prize for mathematical physics from the American Physical Society and the American Institute of Physics.

漢斯·阿爾弗雷德·貝特於1928年在慕尼黑獲得博士學位。1935年，他來到康奈爾大學，現在是名譽教授。1967年，他因為解釋恆星產生能量的過程而獲得諾貝爾物理學獎。他早期的科學工作主要集中在原子理論、固態物理和原子碰撞上。後來，他專注於核物理學。他對恆星能量的解釋源於他在核理論方面的研究。最近，他的研究方向包括中子星和超新星。羅曼·傑基夫自1969年以來一直擔任麻省理工學院的物理學教授，此前他在哈佛大學的學會擔任了三年的初級研究員。他的主要研究領域是理論物理，並對粒子物理、凝聚態物理和引力物理做出了貢獻。最近，他獲得了美國物理學會和美國物理學研究所頒發的丹尼·海寧曼數學物理獎。