طاقة الفوتون

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 6.24×10¹⁸ 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 as in the optical and radio frequency regions of the electromagnetic spectrum.

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صِيَغ

الفيزياء

Photon energy is directly proportional to frequency.^[1]

E=hf

where

$E$ is energy (typically in joules)^[2]
$h$ is the Planck constant
$f$ is frequency (typically in hertz)^[2]

This equation is known as the Planck–Einstein relation.

Additionally, using equation f = c/λ,

E={\frac {hc}{\lambda }}

where

E is photon 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 6.62607015×10⁻³⁴ J, which is equal to 4.135667697×10⁻¹⁵ eV.

إلكترون‌ڤولت

Photon energy is often measured in electronvolts. To find the photon energy in electronvolt using the wavelength in micrometres, the equation is approximately

E{\text{ (eV)}}={\frac {1.2398}{\lambda {\text{ (μm)}}}}

since $hc/e$ = 1.239841984...×10⁻⁶ eV⋅m^[3] 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.

أمثلة

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).

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.^[4] This corresponds to frequencies of 2.42×10²⁵ Hz to 2.42×10²⁹ Hz.

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 ≈ 3×10⁻¹⁹ J ≈ 75 k_BT, where k_BT 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 5×10⁻¹⁸ J) with a maximal energy conversion efficiency of 35%.

انظر أيضاً

المراجع

^ "Energy of Photon". Photovoltaic Education Network, pveducation.org.
^ ^أ ^ب "6.3 How is energy related to the wavelength of radiation? | METEO 300: Fundamentals of Atmospheric Science".
^ "NIST table of fundamental physical constants". Retrieved 27 June 2023.
^ Sciences, Chinese Academy of. "Observatory discovers a dozen PeVatrons and photons exceeding 1 PeV, launches ultra-high-energy gamma astronomy era". phys.org (in الإنجليزية). Retrieved 2021-11-25.

[:0-1] "Energy of Photon". Photovoltaic Education Network, pveducation.org.

[psu-2] أ ^ب "6.3 How is energy related to the wavelength of radiation? | METEO 300: Fundamentals of Atmospheric Science".

[3] "NIST table of fundamental physical constants". Retrieved 27 June 2023.

[4] Sciences, Chinese Academy of. "Observatory discovers a dozen PeVatrons and photons exceeding 1 PeV, launches ultra-high-energy gamma astronomy era". phys.org (in الإنجليزية). Retrieved 2021-11-25.

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