neutron
(type of baryon that is stable and has no electric charge)
A neutron is a type of baryon
that has no electric charge.
(A baryon is a hadron, i.e., a composite particle,
that is made up of three quarks.)
Neutrons are subject to the strong force, the force
which draws together protons and neutrons to form an atomic nucleus.
Other than 1H, all nuclei include neutrons.
Neutrons can be stable when bound to protons, but
free neutrons (not so-bound) decay with a half-life
of roughly 610 seconds, i.e., mean lifetime of roughly 880 seconds,
the free neutron mean lifetime
(often shortened to neutron lifetime in context).
Neutrons were created very soon after the Big Bang when the
temperature dropped sufficiently that quarks combined into
protons and neutrons. Radioactive decay sometimes converts a
neutron within a nucleus to a proton or vice versa.
(physics,particle)
Further reading:
https://en.wikipedia.org/wiki/Neutron
https://www.britannica.com/science/neutron
http://hyperphysics.phy-astr.gsu.edu/hbase/Particles/proton.html#c3
https://scienceworld.wolfram.com/physics/Neutron.html
Referenced by pages:
1H
alpha particle
Avogadro's number (NA)
baryon
baryonic matter
Bose-Einstein statistics
Cooper pair
cosmic neutrino background (CNB)
Cryogenic Dark Matter Search (CDMS)
dalton (Da)
deuterium (D)
e-folding time
early universe
electron (e-)
element
fusion
ground state
helium (He)
isotope
lanthanide (Ln)
Lunar Reconnaissance Orbiter (LRO)
Lyman series (L)
Mars Science Laboratory (MSL)
mass
mass number (A)
mole (mol)
neutron capture
neutron degenerate matter
neutron drip
neutron rich
neutron scattering
neutron spectrometer
neutron star (NS)
neutronization
neutrons from carbon-13
nuclear statistical equilibrium (NSE)
nucleon
nuclide
p-process
pair production
particle
particle spectrometer
photodissociation
pion (π)
proton
quantum number
quark
quark matter (QM)
r-process
radioactive decay
radioactivity
relic
Rosalind Franklin
s-process
solar neutrino unit (SNU)
standard model
Vela
Index