# Photon energy

**Photon energy** is the energy carried by a single photon. The amount of energy is directly proportional to the photon's electromagnetic frequency and inversely proportional to the wavelength. The higher the photon's frequency, the higher its energy. Equivalently, the longer the photon's wavelength, the lower its energy.

Photon energy is solely a function of the photon's wavelength. Other factors, such as the intensity of the radiation, do not affect photon energy. In other words, two photons of light with the same color and therefore, same frequency, will have the same photon energy, even if one was emitted from a wax candle and the other from the Sun.

Photon energy can be represented by any unit of energy. Among the units commonly used to denote photon energy are the electronvolt (eV) and the joule (as well as its multiples, such as the microjoule). As one joule equals 6.24 × 10^{18} eV, the larger units may be more useful in denoting the energy of photons with higher frequency and higher energy, such as gamma rays, as opposed to lower energy photons, such as those in the radiofrequency region of the electromagnetic spectrum.

## Contents

## Formula[edit]

The equation for photon energy^{[1]} is

Where *E* is photon energy, *h* is the Planck constant, *c* is the speed of light in vacuum and *λ* is the photon's wavelength. As *h* and *c* are both constants, photon energy changes in inverse relation to wavelength *λ*.

To find the photon energy in electronvolts, using the wavelength in micrometres, the equation is approximately

Therefore, the photon energy at 1 μm wavelength, the wavelength of near infrared radiation, is approximately 1.2398 eV.

Since , where *f* is frequency, the photon energy equation can be simplified to

This equation is known as the Planck-Einstein relation. Substituting *h* with its value in J⋅s and *f* with its value in hertz gives the photon energy in joules. Therefore, the photon energy at 1 Hz frequency is 6.62606957 × 10^{−34} joules or 4.135667516 × 10^{−15} eV.

In chemistry and optical engineering,

is used where *h* is Planck's constant and the Greek letter *ν* (nu) is the photon's frequency.^{[2]}

## Examples[edit]

An FM radio station transmitting at 100 MHz emits photons with an energy of about 4.1357 × 10^{−7} eV. This minuscule amount of energy is approximately 8 × 10^{−13} times the electron's mass (via mass-energy equivalence).

The highest energy gamma rays detected to date, very-high-energy gamma rays, have photon energies of 100 GeV to 100 TeV (10^{11} to 10^{14} electronvolts) or 16 nanojoules to 16 microjoules. This corresponds to frequencies of 2.42 × 10^{25} to 2.42 × 10^{28} Hz.

A photon with a wavelength equal to the Planck length would have an energy of about 7.671 × 10^{28} eV or 1.229 × 10^{10} joules (12.29 gigajoules). This is roughly the amount of energy produced by the world's most powerful coal-fired power station, the Taichung Power Plant, during a period of 2.25 seconds.

During photosynthesis, specific chlorophyll molecules absorb red-light photons at a wavelength of 700 nm in the photosystem I, corresponding to an energy of each photon of ≈ 2 eV ≈ 3 x 10^{−19} J ≈ 75 k_{B}T, where k_{B}T denotes the thermal energy. A minimum of 48 photons is needed for the synthesis of a single glucose molecule from CO_{2} and water (chemical potential difference 5 x 10^{−17} J) with a maximal energy conversion efficiency of 35%.

## See also[edit]

- Photon
- Electromagnetic radiation
- Electromagnetic spectrum
- Planck constant and Planck units
- Planck–Einstein relation

## References[edit]

**^**"Energy of Photon". Photovoltaic Education Network, pveducation.org. Archived from the original on 2016-07-12. Retrieved 2015-06-21.**^**Andrew Liddle (27 April 2015).*An Introduction to Modern Cosmology*. John Wiley & Sons. p. 16. ISBN 978-1-118-69025-3.