This textbook teaches classical mechanics as one of the foundations of physics. It describes the mechanical stability and motion in physical systems ranging from the molecular to the galactic scale. Aside from the standard topics of mechanics in the physics curriculum, this book includes an introduction to the theory of elasticity and its use in selected modern engineering applications, e.g. dynamic mechanical analysis of viscoelastic materials. The text also covers many aspects of numerical mechanics, ranging from the solution of ordinary differential equations, including molecular dynamics simulation of many particle systems, to the finite element method. Attendant Mathematica programs or parts thereof are provided in conjunction with selected examples. Numerous links allow the reader to connect to related subjects and research topics. Among others this includes statistical mechanics (separate chapter), quantum mechanics, space flight, galactic dynamics, friction, and vibration spectroscopy. An introductory chapter compiles all essential mathematical tools, ranging from coordinates to complex numbers. Completely solved problems and examples facilitate a thorough understanding of the material.

Concise, detailed, and transparently structured, this upper-level undergraduate textbook is an excellent resource for a one-semester course on thermodynamics for students majoring in physics, chemistry, or materials science. Throughout the seven chapters and three-part appendix, students benefit from numerous practical examples and solved problems ranging in broad scope from cosmic to molecular evolution; cloud formation to rubber elasticity; and Carnot engines to Monte Carlo simulation of phase equilibria. Lauded in Physics Today as "a valuable resource for students and faculty", Hentschke's Thermodynamics presents in this long-anticipated second edition new and extended coverage of a range of topical material, such as thermodynamics of the universe and atmospheric thermodynamics, while also featuring a more application-oriented treatment of surfaces, interfaces, and polymers. Touching on subjects throughout soft-matter physics, superconductors, and complex fluids, this textbook delivers the foundation and breadth of scope necessary to prepare undergraduate students for further study in this timeless yet ever-changing field.

Unlike most traditional introductory textbooks on relativity and cosmology that answer questions like "Does accelerated expansion pull our bodies apart?", "Does the presence of dark matter affect the classical tests of general relativity?" in a qualitative manner, the present text is intended as a foundation, enabling students to read and understand the textbooks and many of the scientific papers on the subject. And, above all, the readers are taught and encouraged to do their own calculations, check the numbers and answer the above and other questions regarding the most exciting discoveries and theoretical developments in general relativistic cosmology, which have occurred since the early 1980s. In comparison to these intellectual benefits the text is short. In fact, its brevity without neglect of scope or mathematical accessibility of key points is rather unique. The authors connect the necessary mathematical concepts and their reward, i.e. the understanding of an important piece of modern physics, along the shortest path. The unavoidable mathematical concepts and tools are presented in as straightforward manner as possible. Even though the mathematics is not very difficult, it certainly is beneficial to know some statistical thermodynamics as well as some quantum mechanics. Thus the text is suitable for the upper undergraduate curriculum.

Thermodynamics is the foundation of many-body physics and thus of physical chemistry and material science as well. Today new sources of useful energy, energy storage, transport and conversion, requiring development of novel technology, are of rapidly increasing importance. This development strongly affects modern industry. Thus, thermodynamics will have to be given more prominence in the science curriculum in colleges and universities - something that is attempted in this book.
The structure of this text is simple and transparent, enabling the easy mapping of the text onto a one-semester course syllabus and the attendant study. There are 8 chapters total and one three-part appendix. Throughout the text the student finds numerous examples (solved problems) reaching from cosmic to molecular evolution or from cloud formation to Bose condensation.