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  • [SCI] Newtonian Mechanics

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  • [SCI] Classical Thermodynamics
  • [SCI] Classical Electromagnetism
  • [SCI] Analytical Mechanics
  • [SCI] Hydrodynamics
  • [SCI] Statistical Mechanics
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  • [TECH] Steam Engine & Heat Engines

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  • [SCI] Statistical Mechanics
  • [SCI] Blackbody Radiation & Planck's Law
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Restructure: USD fix + updated descendants

Description:Replace dollar signs with USD; correct descendants section
# [SCI] Classical Thermodynamics

**Classical Thermodynamics** is the science of heat, work, and energy transformations, developed between 1820 and 1870 by Carnot, Clausius, Kelvin, and Gibbs.

## Overview

Sadi Carnot (1824) proved the existence of a maximum efficiency for heat engines — the Carnot limit — depending only on the temperatures of the hot and cold reservoirs. Rudolf Clausius (1850) reformulated this as two laws: energy is conserved (first law); the entropy of an isolated system never decreases (second law). William Thomson (Lord Kelvin) established the absolute temperature scale. Josiah Willard Gibbs synthesised thermodynamics into its modern form (chemical potential, phase equilibria, free energy).

Thermodynamics was the first deep theory of industrially relevant physics, born partly from the need to understand and improve steam engines already in use.

## Key Figures & Recognition

- **Sadi Carnot** (1796–1832): *Réflexions sur la puissance motrice du feu*, 1824.
- **Rudolf Clausius** (1822–1888): Named entropy; stated the Second Law. No Nobel (predates prize).
- **Lord Kelvin** (1824–1907): Absolute temperature scale, energy conservation.
- **J. W. Gibbs** (1839–1903): *On the Equilibrium of Heterogeneous Substances*, 1876–78.

## Seminal Papers

- Carnot, S. *Réflexions sur la puissance motrice du feu*. 1824.
- Clausius, R. "Über die bewegende Kraft der Wärme." *Ann. Phys.* 79 (1850).
- Gibbs, J.W. "On the Equilibrium of Heterogeneous Substances." *Trans. Conn. Acad.* 1876–78.

## What This Enables

- **[SCI] Statistical Mechanics** — Macroscopic thermodynamic laws cry out fordemand a microscopic explanation via: counting of molecular statesmicrostates gives entropy.
- **[SCI] Blackbody Radiation & Planck's Law** — Thermal equilibrium of radiation in a cavity is a thermodynamic problem that defeats classical theory fatally fails to solve.
- **[TECH] Steam Engine & Heat Engines** — The Carnot efficiency limit and energy accounting give engineers the design principles for practical heat engines.
- **[TECH] Chemical Industry** — Free energy, reaction equilibria, and process heat managementbalances are direct thermodynamic engineering applications.
- **[SCI] Electrochemistry** — Gibbs free energy determines battery open-circuit voltage; the Nernst equation adds temperature and concentration dependence.
- **[SCI] Cryogenics** — The Joule-Thomson throttling effect and Linde refrigeration cycle are applied thermodynamics used to liquefy gases.
- **[TECH] Rocket & Space Launch** — Rocket propulsion is combustion thermodynamics: the Tsiolkovsky equation relates exhaust velocity and mass ratio to delta-v.⏎

# Parents

* [SCI] Newtonian Mechanics
* [SCI] Newtonian Mechanics
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