Thermodynamics

Updated 22 Mar 2026
In this chapter
7 topics · 19 pages
  1. 1Concepts of System and SurroundingsTypes of Systems · State Functions and Path FunctionsHigh yield
  2. 2Work, Heat, EnergyInternal Energy · First Law of ThermodynamicsHigh yield
  3. 3EnthalpyHeat Capacity · Enthalpy of Phase Transition · Standard Enthalpy of FormationHigh yield
  4. 4Measurement of ΔU and ΔHCalorimetry
  5. 5Hess's Law of Constant Heat SummationHigh yield
  6. 6Bond EnthalpyBond Dissociation EnthalpyHigh yield
  7. 7SpontaneityEntropy · Gibbs Energy Change · Criteria for EquilibriumHigh yield

Thermodynamics, derived from Greek words 'therme' (heat) and 'dynamis' (power), is a branch of physical chemistry that deals with the quantitative relationships between heat and other forms of energy. It provides a framework to understand energy transformations in physical and chemical processes, predicting the feasibility and direction of reactions without considering their rates. At its core, th…

Quick Summary

Thermodynamics is the study of energy transformations, particularly involving heat and work. It defines a 'system' (the part of the universe under study) and 'surroundings' (everything else), separated by a boundary.

Systems can be open (exchange matter and energy), closed (exchange energy only), or isolated (no exchange). Key properties are either extensive (depend on amount, like volume) or intensive (independent of amount, like temperature).

State functions (e.g., internal energy, enthalpy, entropy, Gibbs free energy) depend only on the initial and final states, while path functions (heat, work) depend on the process path. The First Law states energy conservation: ΔU=Q+W\Delta U = Q + W.

The Second Law introduces entropy (disorder) and predicts spontaneity: ΔStotal>0\Delta S_{total} > 0 for spontaneous processes. Gibbs free energy (ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S) is the practical criterion for spontaneity at constant T and P.

The Third Law defines zero entropy at absolute zero for perfect crystals. Understanding these laws and concepts is fundamental for predicting chemical and physical changes.

Full explanation

Thermodynamics is a macroscopic science, meaning it deals with the bulk properties of matter rather than individual atoms or molecules. It provides a powerful framework for understanding energy transformations and predicting the feasibility and direction of physical and chemical processes. It is crucial for NEET aspirants to grasp its fundamental principles, as it forms the basis for understanding chemical reactions, equilibrium, and various energy-related phenomena.

Conceptual Foundation

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  1. System, Surroundings, and BoundaryThe universe is conceptually divided into a 'system' and 'surroundings'.

* System: The specific part of the universe under thermodynamic investigation (e.g., reactants in a flask, a gas in a cylinder). * Surroundings: Everything in the universe outside the system that can interact with it. * Boundary: The real or imaginary surface separating the system from its surroundings.

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  1. Types of SystemsBased on the exchange of matter and energy with surroundings:

* Open System: Exchanges both matter and energy (e.g., an open beaker of boiling water). * Closed System: Exchanges energy but not matter (e.g., a sealed reaction vessel). * Isolated System: Exchanges neither matter nor energy (e.g., a perfectly insulated thermos flask; the universe is considered an isolated system).

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  1. Properties of a SystemThese describe the state of the system.

* Extensive Properties: Depend on the amount of matter in the system (e.g., mass, volume, internal energy, enthalpy, entropy, Gibbs free energy). * Intensive Properties: Independent of the amount of matter (e.g., temperature, pressure, density, specific heat, molarity).

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  1. State Functions vs. Path FunctionsThis distinction is fundamental.

* State Functions: Properties whose values depend only on the initial and final states of the system, irrespective of the path taken (e.g., ΔU\Delta U, ΔH\Delta H, ΔS\Delta S, ΔG\Delta G, P, V, T). Their change is denoted by Δ\Delta. * Path Functions: Properties whose values depend on the path taken to go from one state to another (e.g., heat (Q) and work (W)).

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  1. Internal Energy (U)The total energy contained within a system, including kinetic and potential energies of its constituent particles. It is a state function. For a given system, its absolute value cannot be determined, but the change in internal energy (ΔU\Delta U) can be calculated.
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  1. Heat (Q)Energy transferred between a system and its surroundings due to a temperature difference. By convention, Q is positive when heat is absorbed by the system (endothermic) and negative when heat is released by the system (exothermic).
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  1. Work (W)Energy transferred between a system and its surroundings by means other than temperature difference (e.g., mechanical work, electrical work). In chemistry, pressure-volume (PV) work is common. By convention, W is positive when work is done on the system (compression) and negative when work is done by the system (expansion).

Key Principles and Laws of Thermodynamics

1. Zeroth Law of Thermodynamics

If two systems are each in thermal equilibrium with a third system, then they are in thermal equilibrium with each other. This law establishes the concept of temperature as a fundamental property.

2. First Law of Thermodynamics (Law of Conservation of Energy)

It states that energy can neither be created nor destroyed, but can be converted from one form to another. Mathematically, for a closed system:

ΔU=Q+W\Delta U = Q + W
Where:

  • ΔU\Delta U is the change in internal energy of the system.
  • QQ is the heat exchanged between the system and surroundings.
  • WW is the work done on or by the system.

Sign Conventions: Crucial for calculations.

  • Q>0Q > 0: Heat absorbed by the system.
  • Q<0Q < 0: Heat released by the system.
  • W>0W > 0: Work done on the system (compression).
  • W<0W < 0: Work done by the system (expansion).

Types of Processes: The First Law applies to various processes:

  • Isothermal ProcessTemperature (T) remains constant (ΔT=0\Delta T = 0). For an ideal gas, ΔU=0\Delta U = 0, so Q=WQ = -W.
  • Adiabatic ProcessNo heat exchange (Q=0Q = 0). Thus, ΔU=W\Delta U = W.
  • Isobaric ProcessPressure (P) remains constant. W=PextΔVW = -P_{ext}\Delta V. ΔH=Qp\Delta H = Q_p.
  • Isochoric ProcessVolume (V) remains constant (ΔV=0\Delta V = 0). Thus, W=0W = 0, and ΔU=Qv\Delta U = Q_v.
  • Cyclic ProcessThe system returns to its initial state. ΔU=0\Delta U = 0, so Q=WQ = -W.

Work Done in Reversible Isothermal Expansion/Compression of an Ideal Gas:

Wrev=nRTln(V2V1)=nRTln(P1P2)W_{rev} = -nRT \ln\left(\frac{V_2}{V_1}\right) = -nRT \ln\left(\frac{P_1}{P_2}\right)

Enthalpy (H): A state function defined as H=U+PVH = U + PV. It is particularly useful for processes occurring at constant pressure (common in chemistry).

ΔH=ΔU+PΔV\Delta H = \Delta U + P\Delta V
For reactions involving gases, ΔH=ΔU+ΔngRT\Delta H = \Delta U + \Delta n_g RT, where Δng\Delta n_g is the change in the number of moles of gaseous products minus gaseous reactants.

3. Second Law of Thermodynamics

This law introduces the concept of entropy and dictates the direction of spontaneous processes. It can be stated in several ways:

  • Clausius StatementHeat cannot spontaneously flow from a colder body to a hotter body.
  • Kelvin-Planck StatementIt is impossible to construct a device that operates in a cycle and produces no effect other than the extraction of heat from a reservoir and the performance of an equivalent amount of work.
  • Entropy StatementFor a spontaneous process in an isolated system, the entropy of the system always increases (ΔStotal>0\Delta S_{total} > 0). For a reversible process, ΔStotal=0\Delta S_{total} = 0.

Entropy (S): A measure of the disorder or randomness of a system. It is a state function. The change in entropy for a reversible process is given by:

ΔS=QrevT\Delta S = \frac{Q_{rev}}{T}
Units: J K1^{-1} mol1^{-1}.

Criteria for Spontaneity: For a process to be spontaneous:

  • In an isolated system: ΔSsystem>0\Delta S_{system} > 0.
  • In a non-isolated system, considering both system and surroundings:

ΔStotal=ΔSsystem+ΔSsurroundings>0\Delta S_{total} = \Delta S_{system} + \Delta S_{surroundings} > 0

Gibbs Free Energy (G): A state function defined as G=HTSG = H - TS. It is the most convenient criterion for spontaneity at constant temperature and pressure.

ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S

  • If ΔG<0\Delta G < 0: The process is spontaneous.
  • If ΔG>0\Delta G > 0: The process is non-spontaneous (the reverse process is spontaneous).
  • If ΔG=0\Delta G = 0: The system is at equilibrium.

**Relationship between ΔG\Delta G and Equilibrium Constant (K)**:

ΔG=RTlnK\Delta G^\circ = -RT \ln K
Where ΔG\Delta G^\circ is the standard Gibbs free energy change, R is the gas constant, and T is the temperature in Kelvin.

4. Third Law of Thermodynamics

It states that the entropy of a perfect crystalline substance at absolute zero temperature (0 K) is exactly zero. This law provides a reference point for determining absolute entropies.

Derivations where Relevant

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  1. Work Done in Reversible Isothermal ExpansionFor an ideal gas, Pext=Pint=nRT/VP_{ext} = P_{int} = nRT/V. Work done is W=V1V2PextdVW = -\int_{V_1}^{V_2} P_{ext} dV. Substituting PextP_{ext}, we get:

Wrev=V1V2nRTVdV=nRT[lnV]V1V2=nRTln(V2V1)W_{rev} = -\int_{V_1}^{V_2} \frac{nRT}{V} dV = -nRT [\ln V]_{V_1}^{V_2} = -nRT \ln\left(\frac{V_2}{V_1}\right)

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  1. Relationship between $\Delta H$ and $\Delta U$Starting from H=U+PVH = U + PV, for a change at constant pressure:

ΔH=ΔU+Δ(PV)\Delta H = \Delta U + \Delta(PV)
If only PV work is considered and pressure is constant:
ΔH=ΔU+PΔV\Delta H = \Delta U + P\Delta V
For reactions involving gases, using the ideal gas law PV=nRTPV = nRT, we can write PΔV=ΔngRTP\Delta V = \Delta n_g RT. Thus:
ΔH=ΔU+ΔngRT\Delta H = \Delta U + \Delta n_g RT
Where Δng=(moles of gaseous products)(moles of gaseous reactants)\Delta n_g = (\text{moles of gaseous products}) - (\text{moles of gaseous reactants}).

Real-World Applications

  • Chemical ReactionsPredicting whether a reaction will occur spontaneously and calculating the maximum yield.
  • Engines and RefrigeratorsUnderstanding the efficiency of heat engines (e.g., car engines) and refrigerators based on the Carnot cycle and thermodynamic laws.
  • Biological SystemsExplaining energy flow in living organisms (e.g., ATP hydrolysis, metabolic pathways).
  • Material ScienceDesigning new materials with desired properties by controlling synthesis conditions based on thermodynamic principles.

Common Misconceptions

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  1. Heat vs. TemperatureHeat is energy transfer due to temperature difference (path function); temperature is a measure of the average kinetic energy of particles (intensive property, state function).
  2. 2
  3. Spontaneity vs. SpeedThermodynamics predicts if a process can occur spontaneously, not how fast it will occur. A spontaneous reaction can be very slow (e.g., diamond converting to graphite).
  4. 3
  5. Isolated System vs. Closed SystemAn isolated system exchanges neither matter nor energy, while a closed system exchanges energy but not matter.
  6. 4
  7. Work Sign ConventionOften confused. Remember: work done by the system (expansion) is negative; work done on the system (compression) is positive.

NEET-Specific Angle

For NEET, the focus is heavily on:

  • CalculationsApplying the First Law (ΔU=Q+W\Delta U = Q + W), calculating work done in various processes, using ΔH=ΔU+ΔngRT\Delta H = \Delta U + \Delta n_g RT, and applying ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S.
  • Conceptual UnderstandingGrasping the definitions of state functions, path functions, types of systems, and the implications of the three laws.
  • Spontaneity CriteriaBeing able to predict spontaneity based on ΔG\Delta G and its dependence on ΔH\Delta H, ΔS\Delta S, and T.
  • Standard Thermodynamic ValuesUnderstanding standard enthalpy of formation, combustion, bond enthalpy, and their use in calculating reaction enthalpies.
  • Entropy ChangesPredicting the sign of ΔS\Delta S for various physical and chemical changes (e.g., gas formation, phase transitions, dissolution).

Mastering these aspects will ensure a strong performance in thermodynamics questions in the NEET exam.

Key Concepts

First Law of Thermodynamics (Energy Conservation)

The First Law states that energy cannot be created or destroyed, only converted from one form to another. For…

Spontaneity and Gibbs Free Energy

Spontaneity refers to whether a process will occur on its own without continuous external intervention. The…

Relationship between ΔH\Delta H and ΔU\Delta U

Enthalpy (H) is defined as H=U+PVH = U + PV. For a chemical reaction or physical change occurring at constant…

Often confused with

Side-by-side differences the NEET paper likes to test.

Thermodynamics vs State Functions vs. Path Functions
AspectThermodynamicsState Functions vs. Path Functions
DefinitionProperties whose values depend only on the initial and final states of the system, irrespective of the path taken.Properties whose values depend on the specific path or manner in which a change of state occurs.
DependenceIndependent of the process path.Dependent on the process path.
Mathematical RepresentationExact differentials (e.g., $dU$, $dH$). Change denoted by $\Delta$ (e.g., $\Delta U$).Inexact differentials (e.g., $\delta Q$, $\delta W$). Not denoted by $\Delta$ for total change.
ExamplesPressure (P), Volume (V), Temperature (T), Internal Energy (U), Enthalpy (H), Entropy (S), Gibbs Free Energy (G).Heat (Q), Work (W).
Cyclic ProcessFor a cyclic process, the net change in a state function is zero.For a cyclic process, the net heat or work exchanged is generally non-zero.

The distinction between state functions and path functions is fundamental in thermodynamics. State functions provide a snapshot of the system's condition, with their changes being independent of how the change occurred.

This makes them extremely useful for defining the thermodynamic state. Path functions, conversely, describe the energy transfer during a process and are entirely dependent on the specific sequence of steps taken.

Understanding this difference is critical for correctly applying thermodynamic laws and performing calculations, especially concerning internal energy, enthalpy, heat, and work.

Why it is tested: For NEET, this distinction is frequently tested conceptually and is vital for correctly interpreting and applying the First Law of Thermodynamics. Students must know which quantities are state functions (e.g., $\Delta U$, $\Delta H$) and which are path functions (Q, W) to avoid common calculation errors and to understand the theoretical underpinnings of thermodynamic processes.

Questions students ask

5 answered on this topic.

What is the difference between an extensive and an intensive property?

Extensive properties depend on the amount of matter present in the system. Examples include mass, volume, internal energy, enthalpy, and entropy. If you double the amount of substance, these properties will also double.

Intensive properties, on the other hand, are independent of the amount of matter. Examples are temperature, pressure, density, and specific heat capacity. A small drop of water has the same temperature and density as a large bucket of water at the same conditions.

This distinction is crucial for understanding how system properties change.

Why is Gibbs Free Energy ($\Delta G$) a more practical criterion for spontaneity than entropy ($\Delta S_{total}$)?

While the Second Law states that a process is spontaneous if ΔStotal>0\Delta S_{total} > 0 (where ΔStotal=ΔSsystem+ΔSsurroundings\Delta S_{total} = \Delta S_{system} + \Delta S_{surroundings}), calculating ΔSsurroundings\Delta S_{surroundings} can be challenging as it requires knowing the heat exchanged with the surroundings.

Gibbs Free Energy, ΔG=ΔHTΔSsystem\Delta G = \Delta H - T\Delta S_{system}, provides a direct criterion for spontaneity that only depends on the properties of the system itself (ΔHsystem\Delta H_{system} and ΔSsystem\Delta S_{system}) at constant temperature and pressure, which are common experimental conditions.

Thus, it's much more convenient to use.

What is the significance of the sign conventions for heat (Q) and work (W) in the First Law of Thermodynamics?

The sign conventions are crucial for correctly applying the First Law, ΔU=Q+W\Delta U = Q + W. For heat (Q), a positive sign means heat is absorbed by the system from the surroundings (endothermic process), increasing its internal energy.

A negative sign means heat is released from the system to the surroundings (exothermic process). For work (W), a positive sign means work is done on the system by the surroundings (e.g., compression), increasing its internal energy.

A negative sign means work is done by the system on the surroundings (e.g., expansion), decreasing its internal energy. Consistent application of these conventions is vital for accurate calculations.

Can a non-spontaneous reaction occur?

Yes, a non-spontaneous reaction can occur, but it requires continuous input of energy from the surroundings. Thermodynamics predicts that such a reaction will not proceed on its own. For example, charging a battery is a non-spontaneous process that requires electrical energy input.

Similarly, many biological processes that build complex molecules from simpler ones are non-spontaneous and are driven by the energy released from spontaneous processes like ATP hydrolysis. The term 'spontaneous' in thermodynamics simply means 'energetically favorable' or 'happens without external intervention'.

What is the difference between reversible and irreversible processes?

A reversible process is an idealized process that can be reversed by an infinitesimal change in conditions, returning the system and surroundings to their initial states without any net change in the universe.

It occurs infinitely slowly and involves a series of equilibrium states. Work done in a reversible process is maximum. An irreversible process, on the other hand, is a real-world process that cannot be reversed without leaving some permanent change in the surroundings.

It occurs at a finite rate and involves non-equilibrium states. Most natural processes are irreversible, and the work done is always less than the maximum possible reversible work.

Revise in 30 seconds

  • First LawΔU=Q+W\Delta U = Q + W (Energy Conservation) \n- Work (Constant P): W=PextΔVW = -P_{ext}\Delta V \n- Work (Reversible Isothermal): Wrev=nRTln(V2/V1)W_{rev} = -nRT \ln(V_2/V_1) \n- Enthalpy: H=U+PVH = U + PV, ΔH=ΔU+ΔngRT\Delta H = \Delta U + \Delta n_g RT \n- Second Law: ΔStotal>0\Delta S_{total} > 0 (Spontaneous) \n- Entropy Change: ΔS=Qrev/T\Delta S = Q_{rev}/T \n- Gibbs Free Energy: ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S \n- Spontaneity: ΔG<0\Delta G < 0 (Spontaneous), ΔG=0\Delta G = 0 (Equilibrium), ΔG>0\Delta G > 0 (Non-spontaneous) \n- Equilibrium Constant: ΔG=RTlnK\Delta G^\circ = -RT \ln K \n- Third Law: S=0S = 0 at 0K0\,\text{K} for perfect crystal \n- Sign Conventions: Q (+ve absorbed, -ve released); W (+ve on system, -ve by system)

To remember the spontaneity conditions based on ΔH\Delta H and ΔS\Delta S: \n\n'Happy Students Get To Succeed' \nΔH\Delta H (Happy) and ΔS\Delta S (Students) determine ΔG\Delta G (Get) at Temperature (To) for Spontaneity (Succeed).

\n\n* H-ve, S+ve: Always spontaneous (Happy, Succeed). \n* H+ve, S-ve: Never spontaneous (Sad, Fail). \n* H-ve, S-ve: Spontaneous at Low T (Happy, but messy, so needs cool head). \n* H+ve, S+ve: Spontaneous at High T (Needs energy, but loves freedom, so needs hot environment).