Photons3 concepts
- Visible light is about 400–700 nm, i.e. 3.1–1.8 eV. Shorter than 400 nm is UV (more energy per photon), longer than 700 nm is IR; X-rays are near 1 Å.
- Not = the number in . That number is , so . Sum of sines: the highest sets ; a product such as has highest .
- Not less momentum at shorter . and both rise as falls. Two photons with equal momentum have equal wavelength.
- Point source of power : photons per second per m² at distance . Pressure and force of light: EM Waves sheet.
- Not . That is the energy per photon. At the same power, longer-wavelength photons are weaker, so more of them are emitted each second.
- Quick method. Convert first: mW to W, nm to m, cm² to m² (). Or find in eV from and multiply by for joules.
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16 more concepts in 5 topics
Photoelectric effect: observations, Einstein's photoelectric equation, Photoelectric graphs, de Broglie waves and Matter waves: links and evidence. Read the first part free. Sign in free with Google to read the rest and download the PDF.
Photoelectric effect: observations2 concepts
- Hertz and Lenard observations10×
- Why wave theory fails4×
Einstein's photoelectric equation5 concepts
- Einstein's equation23×
- Threshold frequency and wavelength13×
- Two lights on one metal17×
- Speeds of photoelectrons6×
- Photoelectrons in a magnetic field4×
Photoelectric graphs2 concepts
- Stopping potential vs frequency10×
- Photocurrent vs anode potential4×
de Broglie waves5 concepts
- de Broglie relation16×
- Charge accelerated through V14×
- Comparing particles28×
- Thermal particles5×
- Charge moving in a field7×
Matter waves: links and evidence2 concepts
- Photon vs material particle7×
- Photoelectron wavelength2×
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