Thermodynamics (from the Greek thermos meaning heat and dynamis meaning power) is a branch of physics that studies the effects of changes in temperature, pressure, and volume on physical systems at the macroscopic scale by analyzing the collective motion of their particles using statistics. Roughly, heat means "energy in transit" and dynamics relates to "movement"; thus, in essence thermodynamics studies the movement of energy and how energy instills movement. Historically, thermodynamics developed out of the need to increase the efficiency of early steam engines.
With these tools, thermodynamics describes how systems respond to changes in their surroundings. This can be applied to a wide variety of topics in science and engineering, such as engines, phase transitions, chemical reactions, transport phenomena, and even black holes. The results of thermodynamics are essential for other fields of physics and for chemistry, chemical engineering, cell biology, biomedical engineering, and materials science to name a few.
Statistical Mechanics :: Mathematical Physics
Thermodynamics :: Physics

Black Hole Entropy and Quantum Gravity - An elementary introduction is given to the problem of black hole entropy as formulated by Bekenstein and Hawking.
Black Hole Evaporation - A tutorial in the actual computation of Unruh, Hawking, Gibbons and other radiation
Black Hole Thermodynamics - An simple introduction to black hole thermodynamics
Hawking Radiation - A brief overview of Hawking radiation
Introductory Lectures on Black Hole Thermodynamics - A review of black hole thermodynamics
Quantum Aspects of Black Holes - A brief introduction to quantum aspects of black holes.
The Thermodyanmics of Black Holes - This review includes discussion of classical black hole thermodynamics, Hawking radiation from black holes, the generalized second law, and the issue of entropy bounds.
| MIT 5.60 Thermodynamics & Kinetics, Spring 2008 | |
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