Definition · Plain-language
Thermodynamics
Thermodynamics is the branch of physics that studies heat, energy and work, and the way energy moves and changes form between systems.
The step most authors miss
Doing CRediT right? Don’t stop at the statement.
A CRediT statement credits you inside one paper. The recognition CRediT was built for happens when those roles are tied to you, persistently. Sign in with your ORCID — free — and claim your CRediT contributions on casrai.org, the home of the standard. They become a verified, portable part of your identity, not a line that disappears into one PDF.
Free: claim your contributions, then export a journal-ready CRediT statement, schema.org structured data, JATS XML, CSV or BibTeX — and preview your public profile. A membership publishes that profile publicly and verifies the journals you serve.
The science of heat and energy
Thermodynamics studies how energy, especially heat, moves between objects and changes from one form to another. It treats a defined region — a system — and tracks the energy crossing its boundary as heat or as work. From the steam engine to the human body, almost every process that involves energy obeys thermodynamic rules. The field grew out of attempts to make engines more efficient in the nineteenth century and now underpins chemistry, engineering, biology and cosmology.
The four laws in plain words
The zeroth law says that if two systems are each in thermal equilibrium with a third, they are in equilibrium with each other — the basis for measuring temperature. The first law is conservation of energy: energy can change form but is never created or destroyed, so the energy of an isolated system is constant. The second law states that the total entropy, a measure of disorder, never decreases in an isolated system, which sets the direction of natural processes. The third law says entropy approaches a constant minimum as temperature nears absolute zero, which can never quite be reached.
Why entropy sets time’s arrow
The second law is what makes many processes one-way. Heat flows naturally from hot to cold, never the reverse, and a smashed cup never reassembles itself, because these changes increase the overall disorder of the universe. This tendency for entropy to increase is often called the arrow of time — it is one of the few physical principles that distinguishes the past from the future. Local order can still grow, as when life builds complex structures, but only by exporting even more disorder to the surroundings.
Key facts
At a glance
- Definition: the physics of heat, energy, work and temperature
- Zeroth law: defines thermal equilibrium and lets us measure temperature
- First law: energy is conserved — it changes form but is never lost
- Second law: total entropy (disorder) tends to increase over time
- Third law: entropy nears a minimum as temperature approaches absolute zero
- Absolute zero: 0 kelvin (−273.15 °C), unreachable in practice
Common misconceptions
What people often get wrong
Often heard: The laws of thermodynamics mean energy gradually runs out.
Actually: Energy is conserved — the first law says it is never destroyed. What degrades is the quality of energy: it spreads out and becomes less useful as entropy rises, even though the total amount is unchanged.
Often heard: Entropy can never decrease anywhere.
Actually: Entropy can fall locally, such as when a fridge cools its contents or life builds order. The second law only forbids the total entropy of an isolated system from decreasing; local order is paid for by greater disorder elsewhere.
Often heard: You can reach absolute zero with a good enough cooler.
Actually: The third law implies absolute zero cannot be reached in a finite number of steps. Temperatures can get extraordinarily close, but never quite touch 0 kelvin.
Going deeper







