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First, UNMSplit is used to expand NM products of U matrices into meson fields:
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Redundant terms are discarded:
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Remaining 'raw' quantites are given arguments:
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Calculation of the Feynman rule:
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A couple of checks:
![massshellrules = {Pair[Momentum[p1], Momentum[p2]] -> (Pair[Momentum[p3], Momentum[p3]] - Pair[Momentum[p1], Momentum[p1]])/2, Pair[Momentum[p2], Momentum[p3]] -> (Pair[Momentum[p1], Momentum[p1]] - Pair[Momentum[p3], Momentum[p3]])/2, Pair[Momentum[p1], Momentum[p3]] -> -(Pair[Momentum[p3], Momentum[p3]] + Pair[Momentum[p1], Momentum[p1]])/2, Pair[Momentum[p2], Momentum[p2]] -> 0} ;](../HTMLFiles/index_536.gif)
![subpar = Table[(ParticleMass[PhiMeson, SUNIndex[i], r___] -> ParticleMass[Select[$IsoSpinProjectionRules, (! FreeQ[#, {i}] &)][[1]][[1]], r]), {i, 8}] ;](../HTMLFiles/index_537.gif)
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Converted by Mathematica (July 10, 2003)