Entropy

Physics
NEET UG
Version 1Updated 22 Mar 2026

Entropy, denoted by SS, is a fundamental thermodynamic property that quantifies the degree of randomness or disorder within a system, or more precisely, the number of microscopic configurations (microstates) that are consistent with the macroscopic state (macrostate) of the system. It is a state function, meaning its value depends only on the current state of the system, not on the path taken to …

Quick Summary

Entropy is a fundamental thermodynamic property, denoted by SS, that quantifies the degree of energy dispersal and the number of accessible microstates in a system. It is a state function, meaning its value depends only on the system's current state, not the path taken.

The change in entropy for a reversible process is defined as DeltaS=Qrev/TDelta S = Q_{rev}/T, where QrevQ_{rev} is the heat transferred reversibly at absolute temperature TT. The Second Law of Thermodynamics states that the total entropy of an isolated system (or the universe) always increases for any spontaneous, irreversible process, and remains constant for reversible processes.

This law explains the natural direction of events, such as heat flowing from hot to cold, and the tendency of systems towards greater disorder. Boltzmann's formula, S=klnWS = k ln W, provides a statistical interpretation, linking entropy to the number of microscopic arrangements (WW).

Entropy is crucial for understanding the efficiency limits of heat engines and the spontaneity of physical and chemical processes. Its SI unit is Joules per Kelvin (J/K).

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Key Concepts

Entropy Change for Phase Transitions

When a substance undergoes a phase change (e.g., melting, boiling) at a constant temperature, the heat…

Entropy Change for Ideal Gas Processes

For an ideal gas undergoing a reversible process, the change in entropy can be calculated using specific heat…

Entropy of the Universe for Irreversible Processes

For any real, spontaneous (irreversible) process, the total entropy of the universe (system + surroundings)…

  • Definition:Entropy (SS) is a measure of energy dispersal and accessible microstates. State function.
  • SI Unit:Joules per Kelvin (J/K).
  • Second Law:For isolated system/universe, ΔS0\Delta S \ge 0.

* Reversible: ΔSuniverse=0\Delta S_{universe} = 0 * Irreversible: ΔSuniverse>0\Delta S_{universe} > 0

  • Entropy Change (General):ΔS=dQrevT\Delta S = \int \frac{dQ_{rev}}{T}
  • Constant Temperature (Phase Change):ΔS=QT=mLT\Delta S = \frac{Q}{T} = \frac{mL}{T}
  • Heating/Cooling (Constant Specific Heat):ΔS=mcln(T2T1)\Delta S = mc \ln\left(\frac{T_2}{T_1}\right)
  • Ideal Gas (General):ΔS=nCvln(T2T1)+nRln(V2V1)\Delta S = nC_v \ln\left(\frac{T_2}{T_1}\right) + nR \ln\left(\frac{V_2}{V_1}\right)
  • Ideal Gas (Isothermal):ΔS=nRln(V2V1)=nRln(P1P2)\Delta S = nR \ln\left(\frac{V_2}{V_1}\right) = nR \ln\left(\frac{P_1}{P_2}\right)
  • Ideal Gas (Isochoric):ΔS=nCvln(T2T1)\Delta S = nC_v \ln\left(\frac{T_2}{T_1}\right)
  • Ideal Gas (Isobaric):ΔS=nCpln(T2T1)\Delta S = nC_p \ln\left(\frac{T_2}{T_1}\right)
  • Boltzmann's Formula:S=klnWS = k \ln W (conceptual for NEET)
  • Key:Always use absolute temperature (Kelvin).

To remember the key aspects of Entropy:

Every Natural Transformation Raises Order's Problem, Yes!

  • Every Natural Transformation: Refers to spontaneous/irreversible processes.
  • Raises Order's Problem: Implies an increase in disorder or randomness (entropy).
  • Yes!: Confirms the Second Law of Thermodynamics (ΔSuniverse>0\Delta S_{universe} > 0).

Also, for calculations, remember Q/T for S (Quality/Temperature for Spontaneity): Heat divided by Absolute Temperature is the basis for entropy change.

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