Modern Physics: The Photoelectric Effect and Wave-Particle Duality Study Guide

Definition and Fundamentals of the Photoelectric Effect

  • Definition: The photoelectric effect is the phenomenon of the emission of electrons from a metal surface after absorbing photonic energy (light energy).

  • Photoelectrons: The electrons that are emitted from the metal surface during this process are specifically referred to as photoelectrons.

  • Photoelectric Current: The current that flows in a closed circuit as a result of these emitted photoelectrons is known as the photoelectric current.

Planck's Quantum Theory

  • Theoretical Basis: According to this theory, light energy is not continuous.

  • Quanta or Photons: Light energy is always available in integral multiples of small elementary energy packets called quanta or photons.

  • Energy of a Photon: Each photon carries a specific amount of energy defined by the formula:   E=h×νE = h \times \nu   - Where hh is Planck's constant (6.6×1034Js6.6 \times 10^{-34}\,J \cdot s).   - Where ν\nu is the frequency of the light.

Key Physical Quantities in Photoelectric Emission

  • Work Function (WW): This is the minimum energy of incident light required to cause photoelectric emission from a surface.   - Example: The work function of Tungsten can be increased by coating it with metal oxide.

  • Threshold Frequency (ν0\nu_0): This is the minimum frequency of incident light that can cause photoelectric emission.

  • Threshold Wavelength (λ0\lambda_0): This is the maximum wavelength of incident light that can cause photoelectric emission.

  • Material Dependence: All three of these physical quantities (WW, ν0\nu_0, and λ0\lambda_0) depend strictly on the material properties of the metal and will differ for different metals.

Einstein's Photoelectric Equation

  • General Equation: The energy of an incident photon is split between the work function and the maximum kinetic energy of the emitted electron:   E=W+KEmaxE = W + KE_{max}

  • Frequency-based Equation:   h×ν=h×ν0+KEmaxh \times \nu = h \times \nu_0 + KE_{max}

  • Wavelength-based Equation:   h×cλ=h×cλ0+KEmax\frac{h \times c}{\lambda} = \frac{h \times c}{\lambda_0} + KE_{max}

  • Conceptual Scenarios (Example with W=10eVW = 10\,eV):   - If incident energy E=15eVE = 15\,eV: Results in the "most disturbance" (significant emission).   - If incident energy E=10eVE = 10\,eV: The electron will "just pop up" (threshold reached).   - If incident energy E=7eVE = 7\,eV: Results in the "least disturbance" (no emission).

Stopping Potential (VstV_{st})

  • Definition: Stopping potential is the minimum reverse potential applied at the anode to seize or stop the photoelectric current in the circuit.

  • Mechanism: It is the point where the electron stops as it travels by depleting its kinetic energy (KE=0KE = 0).

  • Mathematical Relation:   KEmax=h×νWKE_{max} = h \times \nu - W   e×Vst=h×νWe \times V_{st} = h \times \nu - W   Vst=h×νeWeV_{st} = \frac{h \times \nu}{e} - \frac{W}{e}

  • Dependencies:   - Stopping potential depends on the frequency of the incident light.   - Stopping potential is independent of the intensity of the incident light.

Laboratory Calculation of Planck's Constant

  • Methodology: Different frequencies of incident light are used to obtain different values of stopping potential. These observations are recorded in a table (ν\nu vs VstV_{st}).

  • Graphical Analysis: A graph is plotted with frequency on the x-axis and stopping potential on the y-axis, resulting in a straight line.

  • Linear Equation: Using y=m×x+cy = m \times x + c:   Vst=(he)×νWeV_{st} = \left( \frac{h}{e} \right) \times \nu - \frac{W}{e}

  • Slope (mm): The slope of the line is defined as:   m=tan(θ)=hem = \tan(\theta) = \frac{h}{e}

  • Calculating hh: By multiplying the slope (mm) by the charge of an electron (ee), one obtains Planck's constant:   h=m×eh = m \times e   h=m×1.6×1019=6.6×1034Jsh = m \times 1.6 \times 10^{-19} = 6.6 \times 10^{-34}\,J \cdot s

Proportionality and Observed Relations

  • Photoelectric Current Relationship: Photoelectric current is directly proportional to the intensity of incident light and the number of photoelectrons (or number of photons).   Photoelectric CurrentIntensityNumber of Photons\text{Photoelectric Current} \propto \text{Intensity} \propto \text{Number of Photons}

  • Independence: Both Stopping Potential (VstV_{st}) and Maximum Kinetic Energy (KEmaxKE_{max}) are independent of the intensity of the incident light.

Wave-Particle Duality and De Broglie Relation

  • Classical Energy: According to classical mechanics, the energy of a particle of mass mm is E=m×c2E = m \times c^2.

  • Quantum Energy: Referencing Planck's theory, the energy of a wave is E=h×νE = h \times \nu.

  • Equating Energy: m×c2=h×cλm \times c^2 = \frac{h \times c}{\lambda}, which leads to m×c=hλm \times c = \frac{h}{\lambda}.

  • Momentum (pp): Since p=m×cp = m \times c, then p=hλp = \frac{h}{\lambda}.

  • De Broglie Wavelength: λ=hp\lambda = \frac{h}{p}.

  • Relation to Kinetic Energy (KK):   - Since K=12×m×v2K = \frac{1}{2} \times m \times v^2 and p=m×vp = m \times v, then p=2×K×mp = \sqrt{2 \times K \times m}.   - λ=h2×K×m\lambda = \frac{h}{\sqrt{2 \times K \times m}}.

  • Relation to Potential Difference (VmV_m):   - For a charge qq accelerated through a potential VmV_m, W=q×ΔV=KW = q \times \Delta V = K.   - λ=h2×q×Vm×m\lambda = \frac{h}{\sqrt{2 \times q \times V_m \times m}}.

  • Photon Mass Properties:   - Mass of a photon: m=h×νc2m = \frac{h \times \nu}{c^2}.   - The rest mass of a photon is 00.

Davisson-Germer Experiment and Crystallography

  • Purpose: The Davisson-Germer experiment confirms the wave nature of electrons using the phenomenon of diffraction.

  • Crystallography: For the study of crystal structures (crystallography), X-rays are typically utilized.

Practice Problems

  • Problem 1: Calculate the De Broglie wavelength of an electron with an energy of 100eV100\,eV.   - Formula: λ=h2×K×m\lambda = \frac{h}{\sqrt{2 \times K \times m}}   - Parameters: K=100×1.6×1019JK = 100 \times 1.6 \times 10^{-19}\,J, m=9.1×1031kgm = 9.1 \times 10^{-31}\,kg.

  • Problem 2: Light of wavelength 198nm198\,nm is incident on a metallic cathode with a work function of 2.5eV2.5\,eV. How much potential difference must be applied between the cathode and anode of a photocell to stop the photocurrent? Also, find the threshold wavelength for the metallic cathode.   - Parameters: λ=198×109m\lambda = 198 \times 10^{-9}\,m, W=2.5eVW = 2.5\,eV.