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Energy spread over many particles, and which way it flows.

T1

Temperature

Temperature is what two systems in thermal contact end up sharing once energy stops flowing between them.

T1.1Thermal Equilibrium

Two systems in thermal contact exchange energy until they reach the same temperature — thermal equilibrium. The zeroth law of thermodynamics: if A is in equilibrium with B, and B with C, then A is in equilibrium with C — the principle that makes a thermometer's reading meaningful.

T1.2Temperature Scales

Celsius, Fahrenheit and Kelvin measure the same physical quantity with different zero points and step sizes.

Convention(T1.2.1)Conversion between Celsius, Kelvin and Fahrenheit
T1.3Thermal Expansion

Most materials expand slightly as temperature rises, in proportion to the temperature change and the material's original size.

Result(T1.3.1)Change in length or volume with temperature
T1.4The Ideal Gas Law

An idealized gas of point particles with no intermolecular forces obeys a single equation relating pressure, volume, amount, and temperature.

Law(T1.4.1)Pressure, volume and temperature of an ideal gas
T2

Heat and the First Law

Heat and work are two different ways of moving energy across a system's boundary; the first law tracks both.

T2.1Heat Capacity

Different materials require different amounts of heat to raise their temperature by the same amount.

Definition(T2.1.1)Heat required for a given temperature change
T2.2Latent Heat

During a phase change, added or removed heat changes the proportion of substance in each phase rather than the temperature.

Definition(T2.2.1)Heat required for a phase change at constant temperature
T2.3Work in Thermodynamic Processes

A gas does work on its surroundings by changing volume against an external pressure.

Definition(T2.3.1)Work done by a gas changing volume
T2.4The First Law

Energy conservation applied to a system that can exchange both heat and work with its surroundings.

Principle(T2.4.1)Energy conservation for heat and work combined
T3

Kinetic Theory

Pressure, temperature and heat capacity are all statistical consequences of enormous numbers of colliding molecules.

T3.1Molecular Model of Pressure

Gas pressure arises from the cumulative momentum transferred by molecules colliding with a container's walls.

Result(T3.1.1)Gas pressure from molecular collisions
T3.2Equipartition of Energy

At thermal equilibrium, energy distributes equally among every independent way a molecule can store it.

Principle(T3.2.1)Average thermal energy per degree of freedom
T3.3Molar Heat Capacities

Heat capacity follows directly from how many degrees of freedom a gas molecule has to store energy in.

Result(T3.3.1)Molar heat capacity from degrees of freedom
T3.4Distribution of Molecular Speeds

Not every molecule in a gas moves at the same speed: the Maxwell-Boltzmann distribution describes the spread, skewed toward higher speeds with a long tail. The most probable, mean, and root-mean-square speeds are three distinct values, in that increasing order, and all shift higher as temperature rises.

T4

Entropy and the Second Law

Heat never flows spontaneously from cold to hot; every engine, refrigerator and irreversible process obeys that one restriction.

T4.1Heat Engines

A heat engine converts part of the heat flowing from a hot reservoir into useful work, exhausting the rest to a cold reservoir.

Definition(T4.1.1)Fraction of heat input converted to work
T4.2Refrigerators and Heat Pumps

A refrigerator or heat pump uses work input to move heat against its natural direction, from cold to hot.

Definition(T4.2.1)Heat moved per unit of work, for a refrigerator or heat pump
T4.3The Carnot Cycle

No engine operating between two fixed temperatures can exceed the efficiency of an idealized, fully reversible cycle.

Result(T4.3.1)Maximum possible efficiency between two reservoirs
T4.4Entropy

Entropy quantifies the direction in which spontaneous processes run: toward greater disorder, never the reverse.

Definition(T4.4.1)Entropy change from heat exchanged at a given temperature