Photon energy

 ( Foundational Quantum Physics ) 

Photon energy is the energy carried by a single photon. The amount of energy is directly proportional to the photon's electromagnetic frequency and thus, equivalently, is 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 can be expressed using any energy unit. 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 , the larger units may be more useful in denoting the energy of photons with higher frequency and higher energy, such as , as opposed to lower energy photons as in the optical and radio frequency regions of the electromagnetic spectrum.

---

Formulas

---

Physics Photon energy is directly proportional to frequency. $$E\; =\; hf$$ where

• $E$ is energy (Joule in the SI system)
• $h$ is the Planck constant
• $f$ is frequency

This equation is known as the Planck relation.

Additionally, using equation f = c/ λ, $$E\; =\; \backslash frac\{hc\}\{\backslash lambda\}$$ where

• E is the photon's energy
• λ is the photon's wavelength
• c is the speed of light in vacuum
• h is the Planck constant

The photon energy at 1 Hz is equal to , which is equal to .

---

Electronvolt Photon energy is often measured in electronvolts. One electronvolt (eV) is exactly or, using the atto prefix, , in the SI system. To find the photon energy in electronvolt using the wavelength in , the equation is approximately

$E\backslash text\{\; (eV)\}\; =\; \backslash frac\{1.2398\}\{\backslash lambda\backslash text\{\; (\mu m)\}\}$

since $hc/e$ = where h is the Planck constant, c is the speed of light, and e is the elementary charge.

The photon energy of near infrared radiation at 1 μm wavelength is approximately 1.2398 eV.

---

Examples An FM broadcasting radio station transmitting at 100 megahertz emits photons with an energy of about . This minuscule amount of energy is approximately times the electron's mass (via mass–energy equivalence).

Very-high-energy gamma rays have photon energies of 100 GeV to over 1 PeV (10¹¹ to 10¹⁵ electronvolts) or 16 nJ to 160 μJ. This corresponds to frequencies of to .

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 ≈ ≈ 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 CO₂ and water (chemical potential difference ) with a maximal energy conversion efficiency of 35%.

---

See also

• Electromagnetic radiation
• Electromagnetic spectrum
• Planck relation
• Soft photon

Post Comment