G parity

From testwiki
Jump to navigation Jump to search

Template:Short description In particle physics, G parity is a multiplicative quantum number that results from the generalization of C parity (charge conjugation) to multiplets of particles.

It was introduced by Louis Michel in 1953 as isotopic parity,[1] and later introduced as G parity by T.D. Lee and C.N. Yang in 1956.[2][3]

Description

Charge conjugation or C parity applies only to neutral systems. For example, in the pion triplet, only the neutral pion π0 has C parity. On the other hand, strong interaction does not see electrical charge, so it cannot distinguish amongst π+, π0 and π−. We can generalize the C parity so it applies to all charge states of a given multiplet:

𝒢:(π+π0π−)=ηG(π+π0π−)

where ηG = ±1 are the eigenvalues of G parity. The G parity operator is defined as

𝒢̂=𝒞̂e(iπÎ2)

where 𝒞̂ is the C parity operator, and Î2 is the operator associated with the 2nd component of the isospin "vector", which in case of isospin I=1/2 takes the form Î2=σ2/2, where σ2 is the second Pauli matrix. G-parity is a combination of charge conjugation and a π radians (180°) rotation around the 2nd axis of isospin space. Given that charge and isospin are preserved by strong interactions, so is G. Weak and electromagnetic interactions, though, does not conserve G parity.

Since G parity is applied on a whole multiplet, charge conjugation has to see the multiplet as a neutral entity. Thus, only multiplets with an average charge of 0 will be eigenstates of G, that is

Q¯=B¯=Y¯=0,

where Q is the electric charge of the multiplet, B is the baryon number and Y of the hypercharge.

In general

ηG=ηC(−1)I

where ηC is a C parity eigenvalue, and I is the isospin.

Since no matter whether the system is fermion–antifermion or boson–antiboson, ηC always equals to (−1)L+S, we have

ηG=(−1)S+L+I.

See also

References

Template:Reflist

Template:Particle-stub