Planck-Einstein Relation: The energy () of a single photon is directly proportional to its frequency (), expressed by the formula .
Planck's Constant: The constant of proportionality, , is approximately . It defines the scale of quantization in the universe.
Wavelength Relationship: Since wave speed , the energy can also be expressed in terms of wavelength () as . This shows that energy is inversely proportional to wavelength; shorter wavelengths (like X-rays) have higher energy than longer wavelengths (like radio waves).
The Electronvolt (eV): Because the energy of a single photon is extremely small in Joules, physicists use the electronvolt. One eV is the energy gained by an electron accelerated through a potential difference of one volt.
Conversion Factor: . This value is numerically equal to the charge of an electron.
Application: When calculating photon energy using , the result is in Joules. To convert to eV, divide the result by .
| Feature | Photon Energy | Radiation Intensity |
|---|---|---|
| Determined by | Frequency () or Wavelength () | Number of photons per unit area per second |
| Effect on Electrons | Determines if an electron can be ejected | Determines the rate of electron ejection |
| Formula Context | (where is photons per second) |
Unit Consistency: Always ensure wavelength is in meters (m) and frequency is in Hertz (Hz) before using Planck's constant in Joules. Common prefixes like nanometers () must be converted immediately.
Proportionality Reasoning: If an exam question asks how energy changes when wavelength doubles, recognize the inverse relationship: the energy will be halved ().
Power and Photon Flux: To find the number of photons emitted per second, divide the total power (Watts or J/s) by the energy of a single photon ().