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Law Thermodynamics

Reference data and engineering information about law thermodynamics for thermodynamics applications.

lawthermodynamics

Overview

The laws of thermodynamics are fundamental principles governing energy, heat, and work in physical systems.

Key Formulas

Zeroth Law

TA=TB and TB=TCTA=TCT_A = T_B \text{ and } T_B = T_C \Rightarrow T_A = T_C

If two systems are each in thermal equilibrium with a third, they are in equilibrium with each other.

First Law

ΔU=QW\Delta U = Q - W

Change in internal energy = heat added − work done by the system.

Second Law (Clausius)

ΔSQT\Delta S \geq \frac{Q}{T}

Entropy of an isolated system never decreases.

Third Law

limT0S=0\lim_{T \to 0} S = 0

Entropy approaches zero as temperature approaches absolute zero (perfect crystal).

Variables

SymbolDescriptionUnit
UUInternal energyJ
QQHeat added to systemJ
WWWork done by systemJ
SSEntropyJ/K
TTAbsolute temperatureK

Entropy and the Second Law

Entropy quantifies the unavailable energy in a system and its relative ability to perform work. Key properties derived from the Second Law include:

  • Entropy change conditions:

    • ΔS>0\Delta S > 0: irreversible process
    • ΔS=0\Delta S = 0: reversible process
    • ΔS<0\Delta S < 0: impossible process
  • Entropy is not conserved like energy; it is produced by all real processes and associated with energy degradation.

  • The entropy of the universe tends to increase as energy flows towards lower availability.

For a thermodynamic process, the entropy change is given by:

dS=dHTadS = \frac{dH}{T_a}

where dSdS is entropy change (kJ/kg·K), dHdH is change in enthalpy or internal energy (kJ/kg), and TaT_a is average temperature (K).

Carnot Heat Cycle Analysis

The Carnot cycle models an ideal heat engine with four reversible stages:

  1. Isothermal expansion at ThT_h: ΔE1=0\Delta E_1 = 0, w1=H1w_1 = -H_1
  2. Adiabatic expansion from ThT_h to TcT_c: H2=0H_2 = 0, ΔE2=w2\Delta E_2 = w_2
  3. Isothermal compression at TcT_c: ΔE3=0\Delta E_3 = 0, w3=H3w_3 = -H_3
  4. Adiabatic compression back to ThT_h: H4=0H_4 = 0, ΔE4=w4\Delta E_4 = w_4

Net work and heat relationships: w=H=H1+H2+H3+H4-w = H = H_1 + H_2 + H_3 + H_4 dHT=0\oint \frac{dH}{T} = 0

The cycle's thermodynamic efficiency is: η=ThTcTh=1TcTh\eta = \frac{T_h - T_c}{T_h} = 1 - \frac{T_c}{T_h}

Entropy Change Examples

Heating Water

  • Mass: 1 kg, from 0°C (273 K) to 100°C (373 K)
  • Specific enthalpy: h1=0h_1 = 0 kJ/kg, h2=419h_2 = 419 kJ/kg
  • Average temperature: Ta=(273+373)/2=323T_a = (273 + 373)/2 = 323 K
  • Entropy change: ΔS=4190323=1.297kJ/kg⋅K\Delta S = \frac{419 - 0}{323} = 1.297 \, \text{kJ/kg·K}

Evaporation of Water

  • Phase change at 100°C (373 K)
  • Specific enthalpy: liquid h1=418h_1 = 418 kJ/kg, vapor h2=2675h_2 = 2675 kJ/kg
  • Temperature: Ta=373T_a = 373 K
  • Entropy change: ΔS=2675418373=6.054kJ/kg⋅K\Delta S = \frac{2675 - 418}{373} = 6.054 \, \text{kJ/kg·K}

These examples illustrate entropy increase during heating and phase change, highlighting energy dispersal at constant temperature.

References