Unit 1: Introductory Quantum Mechanics – Study Material (Part 1)



📘 Unit 1: Introductory Quantum Mechanics – Study Material (Part 1)


🔶 1. Planck’s Radiation Law

🔹 Introduction

In the late 19th century, classical physics could not explain the nature of blackbody radiation. According to classical theory (Rayleigh-Jeans law), the energy radiated at short wavelengths (UV region) should be infinite—this problem is known as the Ultraviolet Catastrophe.

Max Planck, in 1900, proposed a new theory stating that energy is not continuous but quantized, meaning it exists in discrete packets called quanta.


🔹 Key Postulates by Planck

  1. Energy is emitted or absorbed in discrete packets:

   E = nh\nu

= energy,
= integer (1, 2, 3...),
= Planck’s constant = J·s,
= frequency of radiation.

  1. Oscillators can only have energies that are multiples of .

🔹 Planck’s Radiation Formula


E(\nu, T) = \frac{8\pi h \nu^3}{c^3} \cdot \frac{1}{e^{\frac{h\nu}{kT}} - 1}

Where:

  • = energy density at frequency and temperature
  • = Planck’s constant
  • = speed of light
  • = Boltzmann constant = J/K

🔹 Importance of Planck’s Law

  • Explained blackbody radiation curve.
  • Marked the beginning of quantum theory.
  • Accurate for all wavelengths, unlike classical theories.

🔹 Blackbody Radiation Curve

  • Low wavelengths (UV): Energy increases then drops (explained only by Planck).
  • Classical theory fails at short wavelengths.

🔶 2. Photoelectric Effect

🔹 Definition

The emission of electrons from a metal surface when light of suitable frequency falls on it.

Discovered by: Heinrich Hertz
Explained by: Albert Einstein (1905)


🔹 Observations That Couldn’t Be Explained Classically

  1. No electrons are emitted below a certain threshold frequency, regardless of intensity.
  2. Number of electrons depends on intensity of light.
  3. Kinetic energy of emitted electrons depends on frequency, not intensity.

🔹 Einstein’s Photoelectric Equation


K.E. = h\nu - \phi
  • = Kinetic energy of emitted electron
  • = Planck’s constant
  • = frequency of light
  • = work function (minimum energy needed to eject an electron)

🔹 Threshold Frequency ()


\phi = h\nu_0

Below this frequency, no electrons are emitted.


🔹 Applications

  • Solar panels
  • Photodiodes and photomultiplier tubes
  • Einstein received the Nobel Prize in Physics (1921) for this.

🔹 Experiment Setup Diagram

(You can draw or visualize this for your notes)

  • Light source → falls on metal plate in vacuum tube
  • Electrons are emitted → collected by collector
  • Current is measured by galvanometer

🔶 3. Optical Activity

🔹 Definition

A compound is said to be optically active if it can rotate the plane of plane-polarized light.


🔹 Plane-Polarized Light

  • Ordinary light vibrates in all directions.
  • Plane-polarized light vibrates in one plane.
  • Optical rotation occurs when this light passes through a chiral (asymmetric) substance.

🔹 Types of Optical Rotation

  1. Dextrorotatory (+): Rotates light clockwise (e.g., (+)-glucose)
  2. Levorotatory (−): Rotates light anticlockwise (e.g., (−)-fructose)

🔹 Specific Rotation


[\alpha] = \frac{\alpha}{l \cdot c}

Where:

  • = specific rotation (°·dm⁻¹·g⁻¹·mL)
  • = observed angle of rotation
  • = path length in dm
  • = concentration in g/mL

🔹 Measurement – Polarimeter

  • Uses a monochromatic light source
  • Light passes through polarizersample tubeanalyzer
  • Angle of rotation is measured

🔹 Causes of Optical Activity

  • Molecules with chiral centers (asymmetric carbon atoms)
  • No plane of symmetry in molecule

🔹 Examples of Optically Active Compounds

Compound Rotation Nature
Glucose +52.7° Dextrorotatory
Fructose –92.4° Levorotatory
Tartaric Acid ± Can exist as optically active and inactive (racemic) mixtures

🔹 Applications

  • Determining purity of enantiomers
  • Identifying sugar types in food and biochemistry
  • Pharmaceutical analysis

Quick Summary – Part 1

Topic Formula Key Point
Planck's Law Energy is quantized
Photoelectric Effect Light ejects electrons
Optical Activity Measures rotation of polarized light

Would you like me to now continue with Part 2, which will cover:

✅ Polarization (Clausius-Mossotti Equation)
✅ Orientation of Dipoles in Electric Field
✅ Dipole Moment & Induced Dipole Moment
✅ Measurement of Dipole Moment

Let me know and I’ll prepare it next!

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