Photon energy
The energy carried by a single photon, set by its frequency or wavelength. The fundamental quantum unit of optical energy and the basis for all energy-wavelength conversions.
A photon of frequency (or angular frequency , or wavelength in vacuum) carries energy
where J·s is Planck's constant, , and m/s.
In practical units, with in micrometers:
The 1.24 conversion constant ( in eV·μm) is one of the most-used numbers in photonics.
Photon energies at common wavelengths:
| Wavelength | Spectral region | Photon energy |
|---|---|---|
| 100 nm | Extreme UV | 12.40 eV |
| 250 nm | UV | 4.96 eV |
| 405 nm | Violet (Blu-ray) | 3.06 eV |
| 532 nm | Green (Nd:YAG doubled) | 2.33 eV |
| 633 nm | Red (HeNe) | 1.96 eV |
| 808 nm | NIR (pump diodes) | 1.53 eV |
| 850 nm | Datacom multimode | 1.46 eV |
| 980 nm | EDFA pump | 1.265 eV |
| 1064 nm | Nd:YAG fundamental | 1.165 eV |
| 1310 nm | Telecom O-band | 0.946 eV |
| 1480 nm | EDFA pump | 0.838 eV |
| 1550 nm | Telecom C-band | 0.800 eV |
| 3 μm | Mid-IR (HF laser, OPO) | 0.413 eV |
| 10.6 μm | CO laser | 0.117 eV |
| 100 μm | Far-IR / THz | 0.0124 eV |
For optical power at wavelength , the photon flux is
A 1 mW beam at 1550 nm carries photons per second. The shot-noise floor of any photodetection scales with this number.
The quantum-limited responsivity of a photodetector is A/W at quantum efficiency . The bandgap of a photovoltaic absorber must be smaller than the photon energy for the photon to be absorbed; otherwise the semiconductor is transparent at that wavelength.
In single-photon experiments (quantum communications, low-level light detection), the energy of individual photons becomes directly observable, and photon-counting detectors (single-photon avalanche diodes, superconducting nanowire detectors) replace continuous photocurrent measurements.