

Thermodynamics studies the relationships between heat, work, and energy, governed by four fundamental laws. It describes energy conservation and the natural direction of energy flow.
State Function:
A state function depends only on the current state of the system, not the path taken to reach that state. Internal energy is a state function because its value at a particular state is independent of its history.First Law of Thermodynamics:
The first law, also known as the law of energy conservation, states that energy cannot be created or destroyed, only transferred or converted from one form to another. In terms of internal energy, heat, and work, it's expressed as:∆U = q – w
Where: ΔU is the change in internal energy. q is the heat added to the system. w is the work done by the system on its surroundings.
 Where:  n is the number of moles of gas.
R is the universal gas constant.
T is the constant temperature.
V
 
  f 
 
 and V
 
  i
 
  are the final and initial volumes, respectively.
 Download PDF Thermodynamics Formula
W = 0
Also Check – Charle’s Law Formula
 Where: γ is the heat capacity ratio
 
  (Cp/Cv)
 
 .
T
 
  f
 
 and T
 
  i
 
  are the final and initial temperatures, respectively.
 H = U + PV
Where: U is the internal energy of the system. P is the pressure of the system. V is the volume of the system. For a process at constant pressure, the change in enthalpy (ΔH) is related to the heat (Q) transferred as:ΔH = Q P 
Where Q P  is the heat transferred at constant pressure.Also Check – S urface Chemistry Formula
Heat Capacity at Constant Pressure (C P ) and at Constant Volume (C V ): C P is the heat capacity measured at constant pressure. C V is the heat capacity measured at constant volume.
Relation with Ideal Gas Constant:
For an ideal gas, the molar heat capacities at constant pressure (C P  ) and constant volume (C V  ) are related to the ideal gas constant C P - C V = R Furthermore, the heat capacity ratio γ (often used in adiabatic processes for ideal gases) is defined as:
Also Check – Elevation of Boiling Point Formula
 Where: q rev  is the heat transferred during the reversible process.  T is the absolute temperature at which the process occurs.
 Entropy and Phase Changes: For a phase transition (e.g., melting or vaporization) at constant temperature:
Spontaneity: The spontaneity of a process is determined by the Gibbs free energy
ΔG = ΔH − TΔS
Where: ΔG is the change in Gibbs free energy. ΔH is the change in enthalpy. ΔS is the change in entropy. T is the absolute temperature. The sign of ΔG dictates spontaneity: If ΔG<0 , the process is spontaneous. If ΔG>0 , the process is non-spontaneous. If ΔG=0 , the system is in equilibrium.Temperature Dependence: The sign of ΔH and ΔS can give insights into the temperature dependence of spontaneity:
If ΔH<0 (exothermic) and ΔS>0 (entropy increases), the process is spontaneous at all temperatures. If ΔH>0 (endothermic) and ΔS<0 (entropy decreases), the process is non-spontaneous at all temperatures. If ΔH<0 and ΔS<0 , the process is spontaneous at low temperatures. If ΔH>0 and ΔS>0 , the process is spontaneous at high temperatures. The exact temperature at which the spontaneity changes can be found using the equation ΔG=0 , which givesT = ∆H/∆S
