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Important Formulas: Thermodynamics

Thermodynamic processes :

  • Isothermal process: T = constant
    dT = 0
    ΔT = 0
  • Isochoric process: V = constant
    dV = 0
    ΔV = 0
  • Isobaric process: P = constant
    dP = 0
    ΔP = 0
  • Adiabatic process: q = 0
    or heat exchange with the surrounding = O(zero)

IUPAC Sign convention about Heat and Work :
Work done on the system = Positive
Work done by the system = Negative 

1st Law of Thermodynamics
ΔU = (U- U1) = q + w

Law of equipartion of energy :
Important Formulas: Thermodynamics (only for ideal gas)

Important Formulas: Thermodynamics
where f= degrees of freedom for that gas. (Translational + Rotational)
f = 3 formonoatomic
= 5 for diatomic or linear polyatmic
= 6 for non - linear polyatmic

Calculation of heat (q): 
Total heat capacity:

Important Formulas: Thermodynamics

Molar heat capacity :

Important Formulas: Thermodynamics

Specific heat capacity (s):

Important Formulas: Thermodynamics

WORK DONE (w) :
Isothermal Reversible expansion/compression of an ideal gas :

W = - nRT In (Vf/Vi)

Reversible and irreversible isochoric processes.
Since dV = 0
So dW = - Pext . dV = 0.

Reversible isobaric process:
W = P (Vf - Vi)
Adiabatic reversible expansion :
Important Formulas: Thermodynamics

Reversible Work:
Important Formulas: Thermodynamics

Irreversible Work :
Important Formulas: Thermodynamics

Free expansion - Always going to be irrerversible and since Pext = 0
so dW = -Pext..dV = 0
If no. heat is supplied q = 0
then ΔE = 0 so ΔT = 0.

Application of 1st Law :
ΔU = ΔQ + ΔW ⇒ ΔW = -P ΔV
∴ ΔU = ΔQ -PΔV

Constant volume process
Heat given at constant volume = change in internal energy
∴du = (dq)v
du = nCvdT
Important Formulas: Thermodynamics

Constant pressure process:
H ≡ Enthalpy (state function and extensive property)
H = U + PV

⇒ Cp - Cv = R (only for ideal gas)

Second Law Of Thermodynamics :
Important Formulas: Thermodynamics fo r a spontaneous process.

Entropy (S):
Important Formulas: Thermodynamics

Entropy calculation for an ideal gas undergoin a process :

Important Formulas: Thermodynamics

Important Formulas: Thermodynamics (only for an ideal gas)

Third Law Of Thermodynamics :
The entropy of perfect crystals of all pure elements & compounds is zero at the absolute zero of temperature.

Gibb's free energy (G) : (State function and an extensive property)
Important Formulas: Thermodynamics

Criteria of spontaneity:
(i) If ΔGsystem is (-ve) < 0 ⇒ process is spontaneous
(ii) If ΔGsystem is > 0 ⇒ process is non spontaneous
(iii) lf ΔGsystem  = 0 = 3 system is at equilibrium.

Physical interpretation of ΔG :
 The maximum amount of non-expansional (compression) work which can be performed.
Important Formulas: Thermodynamics

Standard Free Energy Change (ΔG°) :
1. ΔG° = -2.303 RTIog10K
2. At equilibrium ΔG = 0.
3. The decrease in free energy (-ΔG) is given as :
Important Formulas: Thermodynamics
4. Important Formulas: Thermodynamicsfor elemental state = 0

5. Important Formulas: Thermodynamics

Thermochemistry:
Change in standard enthalpy Important Formulas: Thermodynamics

= heat added at constant pressure. =  CPΔT.
If Hproducts > Hreactants

  • Reaction should be end other micas we have to give extra heat to reactants to get these converted into products and if
    Hproducts > Hreactants
  • Reaction will be exothermic as extra heat content of reactants will be released during the reaction. Enthalpy change of a reaction :
    Important Formulas: Thermodynamics
    Important Formulas: Thermodynamics
    = positive - endothermic
    = negative - exothermic

Temperature Dependence Of ΔH : (Kirchoff's equation):
For a constant volume reaction
Important Formulas: Thermodynamics

where ΔCP = Cp (products) - Cp (reactants).
For a constant volume reaction
Important Formulas: Thermodynamics

Enthalpy of Reaction from Enthalpies of Formation :
The enthalpy of reaction can be calculated by
Important Formulas: Thermodynamics  is the stoichiometric coefficient.

Estimation of Enthalpy of a reaction from bond Enthalpies :
Important Formulas: Thermodynamics

Resonance Energy:
Important Formulas: Thermodynamics

The document Important Formulas: Thermodynamics is a part of the NEET Course Chemistry Class 12.
All you need of NEET at this link: NEET

FAQs on Important Formulas: Thermodynamics

1. What are the main thermodynamics formulas I need to memorise for NEET Chemistry?
Ans. Key NEET thermodynamics formulas include ΔG = ΔH - TΔS (Gibbs free energy), ΔH = ΔU + PΔV (enthalpy change), q = mcΔT (heat capacity), and ΔS = q/T (entropy). Additionally, students should memorise W = -PΔV (work done), ΔU = q + W (first law), and relationship between Cp and Cv. Practising these formulas through flashcards and mind maps helps retention for exam success.
2. How do I calculate change in enthalpy using Hess's Law for thermochemistry problems?
Ans. Hess's Law states that enthalpy change depends only on initial and final states, not reaction pathway. To solve problems, arrange given chemical equations so their sum produces the target equation, then add their ΔH values algebraically. Reverse equations flip ΔH sign; multiply equations multiply ΔH accordingly. This constant enthalpy principle is fundamental for solving complex thermochemical calculations on NEET.
3. What's the difference between ΔH and ΔU in thermodynamics, and when do I use each?
Ans. ΔH (enthalpy change) measures total heat exchanged at constant pressure, while ΔU (internal energy change) measures energy change within the system. The relationship ΔH = ΔU + PΔV links them. For most chemistry reactions at constant pressure (like lab conditions), use ΔH. ΔU applies in constant-volume processes. Understanding this distinction prevents marking errors in NEET thermodynamics questions.
4. Why is Gibbs free energy important, and what does a negative ΔG value actually mean?
Ans. Gibbs free energy (ΔG) predicts reaction spontaneity at given temperature using ΔG = ΔH - TΔS. Negative ΔG indicates spontaneous reactions occurring naturally; positive ΔG means non-spontaneous reactions requiring external work. ΔG = 0 represents equilibrium state. This concept links thermodynamics to reaction feasibility, making it crucial for understanding why certain reactions proceed while others don't in NEET exams.
5. How do entropy and enthalpy together determine whether a reaction will happen spontaneously?
Ans. Spontaneity depends on both enthalpy (ΔH) and entropy (ΔS) through Gibbs equation ΔG = ΔH - TΔS. Exothermic, entropy-increasing reactions (negative ΔH, positive ΔS) are always spontaneous. Endothermic reactions become spontaneous only at high temperatures when TΔS exceeds ΔH. Temperature's role in spontaneity decisions is vital for solving thermodynamic feasibility questions in NEET Chemistry.
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