Thermodynamics Chemistry Class 11 PDF: Complete NEET Revision Notes & Formulas

Searching for thermodynamics chemistry class 11 pdf notes? Look no further. This comprehensive guide covers the transformation of heat into other forms of energy, providing essential concepts for NEET aspirants. Thermodynamics is a high-yield chapter that bridges the gap between physical and chemical processes.

01
Introduction to Thermodynamics

Thermodynamics is the branch of science that deals with the relationship between heat and other forms of energy. In chemistry, it helps us predict whether a reaction will occur spontaneously under a given set of conditions. Understanding the interaction between the system and its surroundings is fundamental.

SYSTEM The specific part of the universe being studied (e.g., chemicals in a beaker).
SURROUNDINGS Everything in the universe outside the system boundaries.

Types of Thermodynamic Systems

  • Open System: Exchanges both matter and energy with surroundings (e.g., an open beaker of boiling water).
  • Closed System: Exchanges only energy, not matter (e.g., a sealed cylinder).
  • Isolated System: Exchanges neither matter nor energy (e.g., an ideal thermos flask).

02
Types of Processes in Thermodynamics

The path by which a system changes its state is called a process. Recognizing these processes is key to solving numericals in any thermodynamics chemistry class 11 pdf resource.

Process Type Condition Key Characteristic
Isothermal ΔT = 0 Temperature remains constant.
Adiabatic q = 0 No heat exchange with surroundings.
Isobaric ΔP = 0 Pressure remains constant.
Isochoric ΔV = 0 Volume remains constant (Work = 0).
TIP
In a cyclic process, the system returns to its initial state, meaning the change in all state functions (like ΔU and ΔH) is exactly zero.

03
State Variables and State Functions

State functions depend only on the initial and final states of the system, not on the path taken. Path functions, like work and heat, depend entirely on how the change was achieved.

INTENSIVE PROPERTIES Independent of the amount of matter present (e.g., Temperature, Pressure, Density).
EXTENSIVE PROPERTIES Dependent on the amount of matter present (e.g., Mass, Volume, Enthalpy).
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04
First Law of Thermodynamics

The First Law is essentially the law of conservation of energy. It states that energy can neither be created nor destroyed, only transformed from one form to another.

MATHEMATICAL EXPRESSION
ΔU = q + w
WARN
Sign Convention: Heat added TO the system is +q. Work done ON the system is +w. Work done BY the system is −w.

05
Enthalpy (H) and Thermochemistry

Enthalpy is the total heat content of a system at constant pressure. It is defined as the sum of internal energy and the product of pressure and volume.

H = U + PV
ΔH = ΔU + PΔV (at constant P)
ΔH = ΔU + ΔngRT

Hess’s Law of Constant Heat Summation

Hess’s Law states that the total enthalpy change for a reaction is the same regardless of whether the reaction occurs in one step or several steps. This is a crucial topic in any thermodynamics chemistry class 11 pdf guide for calculating enthalpies of formation.

06
Entropy and the Second Law

The Second Law of Thermodynamics introduces the concept of Entropy (S), which is a measure of the degree of randomness or disorder in a system. It explains why certain processes are spontaneous.

ENTROPY CHANGE
ΔS = qrev / T
SPONTANEITY For a spontaneous process in an isolated system, ΔStotal > 0.
EQUILIBRIUM At equilibrium, ΔStotal = 0.
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07
Gibbs Free Energy (G)

Gibbs Free Energy is the most important criterion for spontaneity in chemical reactions. It combines enthalpy and entropy into a single state function.

ΔG = ΔH − TΔS
ΔG Value Meaning / Spontaneity
ΔG < 0 Spontaneous Process (Exergonic)
ΔG > 0 Non-spontaneous Process (Endergonic)
ΔG = 0 System is at Equilibrium

Quick Revision Summary

  • ΔU = q + w (First Law of Thermodynamics).
  • w = −PextΔV (Irreversible expansion work).
  • ΔH = ΔU + ΔngRT (Relationship between H and U).
  • ΔH is positive for Endothermic; negative for Exothermic.
  • Hess’s Law: ΔHtotal = ΔH1 + ΔH2 + …
  • Bond Enthalpy: ΔH = ΣB.E.(Reactants) − ΣB.E.(Products).
  • Entropy increases with Temperature and Volume.
  • ΔG = ΔH − TΔS (Gibbs-Helmholtz Equation).
  • At Equilibrium, ΔG° = −2.303 RT log K.
  • The Third Law states S = 0 for a perfect crystal at 0 K.
Download Formula Sheet (PDF)

08
Frequently Asked Questions

What is the difference between ΔU and ΔH?
ΔU (Internal Energy) is the heat change at constant volume (qv), while ΔH (Enthalpy) is the heat change at constant pressure (qp). They are related by ΔH = ΔU + PΔV.
Can ΔG be zero for a spontaneous process?
No. For a process to be spontaneous, ΔG must be negative. When ΔG is zero, the system has reached chemical equilibrium and there is no net change in either direction.
Why is entropy of a gas higher than that of a liquid?
Gas molecules move randomly in all directions and have much higher disorder compared to liquid molecules which are relatively constrained. Higher disorder leads to higher entropy.
What does Hess’s Law essentially prove?
It proves that enthalpy is a state function. Since it depends only on the start and end points, the path (steps) taken does not affect the total enthalpy change.
What is an intensive property? Give examples.
Intensive properties are those that do not depend on the quantity of matter. Examples include density, temperature, pressure, and molar heat capacity.
Under what condition does ΔH equal ΔU?
ΔH equals ΔU when the change in number of gaseous moles (Δng) is zero, or when the process occurs at constant volume (ΔV = 0).

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Table of Contents — Chemistry Class 11

Table of Contents

Chemistry — Class 11

01Some Basic Concepts of ChemistryGo to page
02Structure of AtomGo to page
03Classification of Elements and PeriodicityGo to page
04Chemical Bonding and Molecular StructureGo to page
05ThermodynamicsGo to page
06EquilibriumGo to page
07Redox ReactionsGo to page
08Organic Chemistry — Basic PrinciplesGo to page
09HydrocarbonsGo to page

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