photon energy
(the energy carried by a single photon)
The term photon energy is used for the energy carried
by a single photon of electromagnetic radiation (EMR) . A particular photon's
energy is directly related to its wave frequency , i.e.,
the photon is part of an EMR wave such that:
E = h × f
E - energy of a single photon of the wave.
h - Planck constant .
f - wave's frequency.
A typical unit of measurement is the electron volt (eV) .
For short-wavelength , high-frequency EMR
(gamma rays , X-rays , and often the shorter-wavelength
portion of ultraviolet ),
the photon energy (in eV) is generally used to describe the EMR,
whereas wavelength or frequency is more often used for
longer-wavelength EMR.
(EMR,measure,waves )
Further reading:
https://en.wikipedia.org/wiki/Photon_energy
https://www.pveducation.org/pvcdrom/properties-of-sunlight/energy-of-photon
https://www.e-education.psu.edu/meteo300/node/682
http://electron6.phys.utk.edu/phys250/modules/module%201/photons.htm
https://energywavetheory.com/photons/photon-energies/
https://www.brown.edu/research/labs/mittleman/sites/brown.edu.research.labs.mittleman/files/uploads/lecture04.pdf
Referenced by pages:
absorption line
ACIS
ALEXIS
Auger effect
Balmer jump (BJ)
bolometer
Cherenkov detector
Cherenkov Telescope Array (CTA)
Colibrì
Compton scattering
Compton telescope
cosmic gamma ray background (CGB)
cosmic neutrino background (CNB)
cosmic rays (CR)
diffusion damping
electromagnetic spectrum
electron orbital
electron volt (eV)
emission line
eROSITA
FACT
frequency (ν)
gamma rays (GR)
GRB 190114C
hardness
HEGRA
HXMT
imaging atmospheric Cherenkov telescope (IACT)
imaging spectrometer
intergalactic medium (IGM)
ionizing radiation
K correction
K-line
Lyman continuum (LyC)
Lyman-Werner photon
MAGIC
microcalorimeter
neon burning
NICER
nuclear spectral line
pair production
pair telescope
photodisintegration
photoionization
photon
positron (e+ )
proportional counter
relativistic beaming
spectral energy distribution (SED)
stimulated emission
Thomson scattering
Uhuru
ultra-high-energy gamma rays (UHEGR)
vegetation red edge (VRE)
very-high-energy gamma rays (VHEGR)
VHE
wavelength (λ)
Wien's displacement law
X-ray
Notes to myself regarding this page
Index