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Violations of the lepton number conservation laws: The muon decay was described as 'rare' - and it's a pretty common one - I've tweaked some wording elsewhere in the paragraph
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==Violations of the lepton number conservation laws==
==Violations of the lepton number conservation laws==
In the [[Standard Model]], leptonic family numbers (LF numbers) would be preserved if neutrinos were massless. Since [[neutrino oscillations]] have been observed, neutrinos do have a tiny nonzero mass and conservation laws for LF numbers are therefore only approximate. This means the conservation laws are violated, although because of the smallness of the neutrino mass they still hold to a very large degree for interactions containing charged leptons. The (total) lepton number conservation law still holds for most practical purposes (under the Standard Model). So, when dealing with lepton interactions, we can use the constancy of Lepton numbers to predict possible outcomes of interactions, such as:
In the [[Standard Model]], leptonic family numbers (LF numbers) would be preserved if neutrinos were massless. Since [[neutrino oscillations]] have been observed, neutrinos do have a tiny nonzero mass and conservation laws for LF numbers are therefore only approximate. This means the conservation laws are violated, although because of the smallness of the neutrino mass they still hold to a very large degree for interactions containing charged leptons. However, the (total) lepton number conservation law must still hold (under the Standard Model). Thus, it is possible to see rare muon decays such as:
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Revision as of 09:34, 10 February 2015

In particle physics, the lepton number is the number of leptons minus the number of antileptons.

In equation form,

so all leptons have assigned a value of +1, antileptons −1, and non-leptonic particles 0. Lepton number (sometimes also called lepton charge) is an additive quantum number, which means that its sum is preserved in interactions (as opposed to multiplicative quantum numbers such as parity, where the product is preserved instead).

Beside the leptonic number, leptonic family numbers are also defined:

with the same assigning scheme as the leptonic number: +1 for particles of the corresponding family, −1 for the antiparticles, and 0 for leptons of other families or non-leptonic particles.

Violations of the lepton number conservation laws

In the Standard Model, leptonic family numbers (LF numbers) would be preserved if neutrinos were massless. Since neutrino oscillations have been observed, neutrinos do have a tiny nonzero mass and conservation laws for LF numbers are therefore only approximate. This means the conservation laws are violated, although because of the smallness of the neutrino mass they still hold to a very large degree for interactions containing charged leptons. However, the (total) lepton number conservation law must still hold (under the Standard Model). Thus, it is possible to see rare muon decays such as:

 
μ
 → 
e
+
ν
e
+
ν
μ
L:    1 = 1 + 1 1
Le:   0 1 + 1 + 0
Lμ:   1 0 + 0 1

Because the lepton number conservation law in fact is violated by chiral anomalies, there are problems applying this symmetry universally over all energy scales. However, the quantum number BL is much more likely to work and is seen in different models such as the Pati–Salam model.

Experiments such as MEGA have searched for lepton number violation in muon decays to electrons; MEG set the current branching limit of order 10−13. Some BSM theories predict branching ratios of order 10-12 to 10−14.[1]

References

  1. ^ "New Limit on the Lepton-Flavor-Violating Decay mu to e+gamma". PRL. 21 Oct 2011. doi:10.1103/PhysRevLett.107.171801.
  • Griffiths, David J. (1987). Introduction to Elementary Particles. Wiley, John & Sons, Inc. ISBN 0-471-60386-4.
  • Tipler, Paul; Llewellyn, Ralph (2002). Modern Physics (4th ed.). W. H. Freeman. ISBN 0-7167-4345-0.{{cite book}}: CS1 maint: multiple names: authors list (link)
  • M. Raidal; et al. (2008). Eur. Phys. J. C 57, 13. {{cite journal}}: Explicit use of et al. in: |author= (help); Missing or empty |title= (help)