The Photoelectric Effect: Einstein's Equation, Graphs & Numericals
In 1887, Heinrich Hertz made a fascinating observation: when a clean metal surface is illuminated by light of a certain frequency, it emits electrons. This phenomenon came to be known as the Photoelectric Effect, and the ejected electrons were termed photoelectrons.
However, classical wave theory completely failed to explain why this was happening. It took the genius of Albert Einstein, using Max Planck's quantum theory, to finally decode the mystery.
Salient Features of the Photoelectric Effect
- No Time Lag: The emission of electrons happens instantaneously. The moment light hits the metal, electrons are ejected (10-9 seconds).
- Effect of Intensity: Increasing the intensity (brightness) of light increases the number of photoelectrons emitted per second, but it does not change their kinetic energy.
- Effect of Frequency: The kinetic energy of the ejected electrons depends entirely on the frequency of the incident light.
Conditions for the Photoelectric Effect
The Two Critical Requirements
Electrons are bound to the metal nucleus by attractive forces. To pull them out, a specific minimum amount of energy is required.
- Threshold Frequency (ν0): The minimum frequency of light required to eject an electron. If the incident light's frequency (ν) is less than ν0, no electrons will be ejected, regardless of how intense the light is!
- Work Function (Φ or W0): The minimum energy required to eject an electron. It is directly related to the threshold frequency: W0 = hν0.
Einstein’s Photoelectric Equation
Einstein proposed that light consists of energy packets called photons. When a photon strikes an electron, its total energy (E) is split into two parts: one part overcomes the work function (to free the electron), and the remaining energy becomes the kinetic energy of the moving electron.
Graphical Analysis
If we plot the maximum Kinetic Energy of the emitted electrons on the y-axis against the Frequency (ν) of incident light on the x-axis, we get a straight line graph. By comparing Einstein's equation to the equation of a line (y = mx + c):
- The x-intercept represents the Threshold Frequency (ν0).
- The slope of the line represents Planck's constant (h).
Solved Numerical
Competitive exams heavily feature numerical problems based on Einstein's equation. Review the step-by-step solved example below to understand how to apply the formula.
Frequently Asked Questions (FAQs)
What is the Photoelectric Effect?
What does the intensity of light affect in the photoelectric effect?
What is Threshold Frequency?
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