Particle Physics 6, Exercises - Physics, Exercises of Particle Physics

Particle Physics 6, Exercises - Physics - Prof. Hitoshi MurayamaUniversity of California (CA) - UCLA, United States of America (USA), Prof. Hitoshi Murayama, Physics, Particle Physics, exercise, solution

Typology: Exercises

2010/2011

Uploaded on 10/31/2011

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HW #6 (129A), due Dec 6 , 4pm
1. Calculate the branching fraction of Zboson into ν¯ν,e+e,µ+µ,τ+τ,
and all hadrons (u¯u,d¯
d,s¯s,c¯c,b¯
b) together with the correction factor due to
the additional gluon emission, and compare them to the values in the PDG
booklet.
2. Work out vfrom GF= 1/2v2,g=e/ sin θW,gZ=e/sin θWcos θW,
and show that the formulae mW=1
2gv,mZ=1
2gZvdo not quite work. On
the other hand, using α(mZ) = e2(mZ)/4π= 1/129 instead of 1/137, show
that they work much better.
3. Show that the relation m2
W=m2
Zcos2θWdoes not quite work. Instead,
one has to take the effect of virtual top quark into consideration, and the
correct relation is m2
W=m2
Zρcos2θW, with ρ= 1 + 3GFm2
t/(82π2). Here,
the factor of three comes from the number of colors. Show that this relation
works much better.
4. Plot the survival probability in the neutrino oscillation
Psurv = 1 sin22θsin2m2
4EL, (1)
as a function of the cosine zenith angle for atmospheric neutrinos. Assume
that the neutrinos are produced at the altitude of 20 km. Take the parameters
sin22θ= 1, m2= 3 ×103eV2, and E= 1 GeV.

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HW #6 (129A), due Dec 6 , 4pm

  1. Calculate the branching fraction of Z boson into ν ν¯, e+e−, μ+μ−, τ +τ −, and all hadrons (uu¯, d d¯, s¯s, c¯c, b¯b) together with the correction factor due to the additional gluon emission, and compare them to the values in the PDG booklet.
  2. Work out v from GF = 1/

2 v^2 , g = e/ sin θW , gZ = e/ sin θW cos θW , and show that the formulae mW = 12 gv, mZ = 12 gZ v do not quite work. On the other hand, using α(mZ ) = e^2 (mZ )/ 4 π = 1/129 instead of 1/137, show that they work much better.

  1. Show that the relation m^2 W = m^2 Z cos^2 θW does not quite work. Instead, one has to take the effect of virtual top quark into consideration, and the correct relation is m^2 W = m^2 Z ρ cos^2 θW , with ρ = 1 + 3GF m^2 t /(

2 π^2 ). Here, the factor of three comes from the number of colors. Show that this relation works much better.

  1. Plot the survival probability in the neutrino oscillation

Psurv = 1 − sin^2 2 θ sin^2

∆m^2 4 E

L, (1)

as a function of the cosine zenith angle for atmospheric neutrinos. Assume that the neutrinos are produced at the altitude of 20 km. Take the parameters sin^2 2 θ = 1, ∆m^2 = 3 × 10 −^3 eV^2 , and E = 1 GeV.