Astrophysics (Index)About

electron

(e-)
(type of lepton that is stable and has an electric charge of -1)

An electron is a type (i.e., flavor) of lepton that has an electric charge of -1 and is stable. (A lepton is an elementary particle that is a fermion, i.e., with 1/2 integer spin, but unlike a quark, does not respond to the strong force.) Through the electromagnetic forces subject to quantum-mechanical restrictions, electrons can be bound to an atomic nucleus forming atoms and assist in binding atoms together into molecules. Electrons can exist free from atoms and such free electrons can make up some of the particles of a plasma (and most baryonic matter is in the form of plasma and most electrons in the universe are free of atoms). An electron is very light compared to protons and neutrons, on the order of 1/1800 of their mass, but the energy-equivalent of its mass (its rest energy) is considerable, 0.511 MeV, tens of thousands of times the energy needed to ionize an atom. Electrons are created by beta decay and by pair production, the latter which produces both an electron and a positron (the antimatter equivalent of an electron), requiring twice the rest energy of an electron.

The term photoelectron refers to an electron freed by the energy of a photon, from a molecule (this action being termed the photoelectric effect) or from an atom (termed photoionization).


(physics,particle)
Further reading:
https://en.wikipedia.org/wiki/Electron
https://www.britannica.com/science/electron
https://scienceworld.wolfram.com/physics/Electron.html
https://en.wiktionary.org/wiki/photoelectron

Referenced by pages:
absorption
adsorption
Advanced Composition Explorer (ACE)
AGN corona
alpha particle
AMS-02
antimatter
atomic dark matter (aDM)
atomic excitation
atomic number (Z)
Auger effect
aurora
Balmer jump (BJ)
Balmer series (H)
baryon
baryon acoustic oscillations (BAO)
baryonic matter
beta (β)
beta decay
Bethe-Heitler process
binding energy
Bohr model
Brackett series
bremsstrahlung
C+
Cassini
Cherenkov radiation
collisional broadening
column density
Compton scattering
Compton wavelength
Cooper pair
cosmic microwave background (CMB)
cosmic neutrino background (CNB)
cosmic rays (CR)
Coulomb's law
Cryogenic Dark Matter Search (CDMS)
current sheet
curvature radiation
cyclotron radiation
cyclotron radiation emission spectroscopy (CRES)
dark age
dark matter annihilation
de Broglie wavelength
Debye length
decoupling
degeneracy
dielectric
dispersion measure (DM)
ejection
electric dipole radiation
electron capture
electron degeneracy
electron degenerate matter (EDM)
electron orbital
electron pressure
electron scattering
electron screening
electron shell
electron volt (eV)
emission
energetic neutral atom (ENA)
epoch of reionization (EOR)
Faraday rotation
fast radio burst (FRB)
Fermi sea
fine structure
flavor
forbidden line
galactic electron density
galactic wind
gas pixel detector (GPD)
gravitational potential well
ground state
GZK limit
helium (He)
helium 1083 nm line
Humphreys series
hydrogen (H)
hydrogen cyanide (HCN)
hydroxyl (OH)
hyperfine structure
HZE ion
IMAP
International Cometary Explorer (ICE)
International Space Station (ISS)
inverse square law
ion
ion engine
ionization fraction
ionization potential
ionized carbon fine structure line ([CII])
ionized hydrogen (HII)
ionizing radiation
ionosphere
iron (Fe)
IXPE
KATRIN
Klein-Nishina formula
lepton
Lie transform
Lunar Prospector
Lyman alpha (Ly-α)
Lyman series (L)
Lyman-Werner photon
Magnetospheric Multiscale Mission (MMS)
Mars Global Surveyor (MGS)
Mars Observer (MO)
maser
mass number (A)
MAVEN
mean free path
metal
metallic hydrogen
metastable
microchannel array
neutral atomic hydrogen (HI)
neutrino (ν)
neutrinoless double beta decay
neutron degenerate matter
neutron scattering
neutronization
nitrite (NO2-)
nuclide
oxidation state
pair production
pair-instability supernova (PISN)
Parker Solar Probe (PSP)
partial ionization zone
particle
particle spectrometer
Paschen series
Pauli exclusion principle
Penrose Compton scattering (PCS)
Pfund series
photocathode
photochemistry
photoionization
photomultiplier tube (PMT)
photon
photon noise
Pioneer Venus Orbiter (PVO)
plasma
plasma frequency
plasma wave
plasmon
positron (e+)
potential energy (PE)
Project 8
proportional counter
proximity effect
pulsar (PSR)
quantum mechanics (QM)
quantum number
quark
r-process
radiation belt
radioactive decay
radioactivity
recombination
reduced mass
reducing atmosphere
reduction potential (Eh)
relic
Rydberg constant (RH)
Saha equation
scattering
scintillator
scintillometry
self-absorption
Solar and Heliospheric Observatory (SOHO)
solar energetic particle (SEP)
solar neutrino unit (SNU)
solar particle
solar wind
spark chamber
spectral line
spectral line designation
spectral line energy distribution (SLED)
spin (ms)
standard model
standard model of a flare
Stark effect
state of excitation
state of ionization
Strömgren sphere
Sunyaev-Zel'dovich effect (SZ effect)
supersymmetry (SUSY)
suprathermal
synchrotron radiation
synchrotron self-Compton (SSC)
tau neutrino (ντ)
temperature
thermal noise
Thomson optical depth (τT)
Thomson scattering
Urca process
Van Allen belts
wave-particle duality
weak interaction
Wigner crystal
Z+
Zeeman effect
Zeeman-Doppler imaging (ZDI)

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