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Physics class 12th Photoelectric effect

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The photoelectric effect occurs when light strikes a metal surface, causing the emission of electrons. Albert Einstein explained it using quantum theory, proposing that light consists of photons, each carrying energy proportional to its frequency. If a photon’s energy exceeds the work function of the metal, it ejects an electron. Increasing light intensity increases the number of emitted electrons, while increasing frequency boosts their kinetic energy. This effect supports the particle nature of light and helped develop quantum mechanics. It has practical applications in solar cells, photodetectors, and imaging devices, shaping modern physics and technology.

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The Photoelectric Effect




The photoelectric effect is a phenomenon where electrons are emitted from a material
(usually a metal) when it is exposed to light of a certain frequency. It played a crucial
role in the development of quantum mechanics and was explained by Albert Einstein in 1905,
earning him the Nobel Prize in Physics in 1921.


1. Discovery and Observation:
- First observed by Heinrich Hertz in 1887, studied by Philipp Lenard.
- Shining light on certain metals caused electron emission, contradicting classical physics.


2. Experimental Setup:
- A light source is directed onto a metal surface.
- A vacuum tube contains the metal surface (cathode) and another electrode (anode).
- A voltmeter and ammeter measure the emitted electron current.


3. Observations:
- Electrons are emitted instantly when light is shone on metal.
- Increasing light intensity increases the number of electrons but not their energy.
- There is a threshold frequency; below it, no electrons are emitted.
- Kinetic energy of electrons depends on frequency, not intensity.


4. Einstein's Explanation:
- Light consists of particles called photons.
- Photon energy: E = h f (h = Planck's constant, f = frequency of light).
- If E is greater than the work function (W) of the metal, an electron is ejected.
- Kinetic Energy of the electron: K_max = h f - W.
- If h f < W, no electron is emitted.


5. Applications:
- Solar cells, photodiodes, night vision devices, electron microscopes, etc.
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