热物理学导论

施罗德

出版时间

2008-03-31

ISBN

9787506291965

评分

★★★★★
书籍介绍
翻开这本书,你会先被它"接地气"的写法打动:从冰箱、发动机到宇宙学、生物细胞,热力学定律仿佛就藏在生活各处。但真正让读者记住它的,是作者对热学概念的重新排序——在施罗德笔下,熵才是核心,温度退居其次,它只是系统"愿意放出多少能量"的一种表征;第二定律也不是自然界的铁律,而是大量概率与巨大数字运算的必然结果。这种"把熟悉的东西讲陌生、把陌生的讲自然"的处理,让概念的引入毫无突兀感。它适合那些不满足于背公式、想真正理解热统"为什么是这样"的读者;也提醒我们:一本好的物理教材,未必从最抽象处起步,却可能带你走得更远。
AI导读
核心看点
  • 本书严格遵循物理直觉,拒绝空洞的数学推导,所有概念引入均基于自然逻辑,无“显然”等跳步,确保读者建立清晰物理图像。
  • 内容涵盖热力学与统计力学全貌,从基本原理到量子统计,结合化学、生物、天文等多领域实例,展现物理学的广泛应用价值。
  • 习题设计极具引导性,难题拆解为多步小问题,逐步引导正确思路,配合风趣配图,大幅降低学习门槛,提升理解深度。
读者共识
  • 被公认为最友好的热统入门书,概念引入自然,无垃圾教材套路,配图幽默,习题质量极高,完美符合优秀教科书标准。
  • 强烈建议替换传统教材,读者反馈读后豁然开朗,物理图像清晰,理论框架搭建迅速,对初学者极其友好且高效。
  • 尽管存在逻辑简化争议,但瑕不掩瑜,其突出主体、避免读者淹没于细节的设计广受好评,是热统学习的最佳起点。
精彩摘录
  • "The second law is not built into the fundamental laws of nature, though; it arises purely through the laws of probability and the mathematics of very large numbers. But since the probabilities are so overwhelming for any system large enough to see with our eyes, we might as well forget about probabi"
  • "Entropy is the more fundamental quantity, governed by the second law of thermodynamics. Temperature is less fundamental; it is merely a characterization of a system's "willingness" to give up energy, that is, of the relationship between its energy and entropy."
  • "thermodynamic identity: dU = T*dS - P*dV + ∑ μ*dN."
  • "Extensive and Intensive Quantities The number of potentially interesting thermodynamic variables has been growing lately. We now have U, V, iV, S, T, P, /i, H, P, and G, among others. One way to organize all these quantities is to pick out the ones that double if you simply double the amount of stuf"
  • "Because a system will spontaneously seek out the state of lowest free energy, this property tells us that equilibrium phases almost always contain impurities."
  • "The usefulness of the formula F = -k*T* In Z is that from F we can compute the entropy, pressure, and chemical potential, using the partial-derivative formulas"
  • "Degeneracy pressure is what keeps matter from collapsing under the huge electrostatic forces that try to pull electrons and protons together. Please note that degeneracy pressure has absolutely nothing to do with electrostatic repulsion between the electrons (which we've completely ignored); it aris"
  • "Heat is defined as any spontaneous flow of energy from one object to another, cause by a difference in temperature between the objects."
目录
PartI:Fundamentals
Chapter1 Energy in Thermal Physics
Chapter2 The Second Law
Chapter3 Interactions and Implications
PartII:Thermodynamics

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用户评论
这本热力学编的真不错!
最好的热学入门书籍,大一寒假刷完感觉写得太好,写得非常容易理解,习题也都出现得恰到好处,完美的物理学教科书应该有的样子。
最为友好的热力学统计物理入门书!概念的引入十分自然,而且配图风趣幽默,课后习题都是作者精心挑选的,质量很高,强烈推荐啊!
很好的一本热力学教材,讲解很细致,也涵盖了最新的领域。
全部深度解读 →主题书单高分榜最近更新