Katana VentraIP

Muon

A muon (/ˈm(j)ɑːn/ M(Y)OO-on; from the Greek letter mu (μ) used to represent it) is an elementary particle similar to the electron, with an electric charge of −1 e and spin-1/2, but with a much greater mass. It is classified as a lepton. As with other leptons, the muon is not thought to be composed of any simpler particles.

Composition

Second


μ

Antimuon (
μ+
)

1.883531627(42)×10−28 kg[1]
0.1134289257(22) Da[2]
105.6583755(23) MeV/c2[3]

2.1969811(22)×10−6 s[4][5]


e
,
ν
e
,
ν
μ
[5] (most common)

1/2 ħ

LH: −1/2, RH: 0

LH: −1, RH: −2

The muon is an unstable subatomic particle with a mean lifetime of 2.2 μs, much longer than many other subatomic particles. As with the decay of the free neutron (with a lifetime around 15 minutes), muon decay is slow (by subatomic standards) because the decay is mediated only by the weak interaction (rather than the more powerful strong interaction or electromagnetic interaction), and because the mass difference between the muon and the set of its decay products is small, providing few kinetic degrees of freedom for decay. Muon decay almost always produces at least three particles, which must include an electron of the same charge as the muon and two types of neutrinos.


Like all elementary particles, the muon has a corresponding antiparticle of opposite charge (+1 e) but equal mass and spin: the antimuon (also called a positive muon). Muons are denoted by
μ
and antimuons by
μ+
. Formerly, muons were called mu mesons, but are not classified as mesons by modern particle physicists (see § History), and that name is no longer used by the physics community.


Muons have a mass of 105.66 MeV/c2, which is approximately 206.7682827(46)[6] times that of the electron, me. There is also a third lepton, the tau, approximately 17 times heavier than the muon.


Due to their greater mass, muons accelerate slower than electrons in electromagnetic fields, and emit less bremsstrahlung (deceleration radiation). This allows muons of a given energy to penetrate far deeper into matter because the deceleration of electrons and muons is primarily due to energy loss by the bremsstrahlung mechanism. For example, so-called secondary muons, created by cosmic rays hitting the atmosphere, can penetrate the atmosphere and reach Earth's land surface and even into deep mines.


Because muons have a greater mass and energy than the decay energy of radioactivity, they are not produced by radioactive decay. Nonetheless, they are produced in great amounts in high-energy interactions in normal matter, in certain particle accelerator experiments with hadrons, and in cosmic ray interactions with matter. These interactions usually produce pi mesons initially, which almost always decay to muons.


As with the other charged leptons, the muon has an associated muon neutrino, denoted by
ν
μ
, which differs from the electron neutrino and participates in different nuclear reactions.

Electric dipole moment[edit]

The current experimental limit on the muon electric dipole moment, |dμ| < 1.9 × 10−19 e·cm set by the E821 experiment at the Brookhaven, is orders of magnitude above the Standard Model prediction. The observation of a non-zero muon electric dipole moment would provide an additional source of CP violation. An improvement in sensitivity by two orders of magnitude over the Brookhaven limit is expected from the experiments at Fermilab.

searching for the elusive coherent neutrino-less conversion of a muon to an electron in J-PARC

Comet (experiment)

List of particles

an experiment to detect neutrinoless conversion of muons to electrons

Mu2e

Muometric navigation

Muon spin spectroscopy

Muon tomography

Media related to Muons at Wikimedia Commons

NASA Astronomy Picture of the Day: Muon anomalous magnetic moment and supersymmetry (28 August 2005)

. muon anomalous magnetic moment

"g-2 experiment"

. Archived from the original on 2 September 2006. Measurement of the Positive Muon Lifetime

"muLan experiment"

.

"The Review of Particle Physics"

.

"The TRIUMF Weak Interaction Symmetry Test"

. Archived from the original on 25 March 2002. Search for the decay Muon → Positron + Gamma

"The MEG Experiment"

King, Philip. . Backstage Science. Brady Haran.

"Making Muons"