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Solutions to Problem Set 12 - Quantum Field Theory | PHY 396K, Assignments of Physics

Material Type: Assignment; Class: QUANTUM FIELD THEORY I; Subject: Physics; University: University of Texas - Austin; Term: Unknown 2000;

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PHY–396 K/L. Solutions for problem set #12.
Problem 1:
Note the correct muon decay amplitude
M(µeνµ¯νe) = GF
2¯u(νµ)(1 γ5)γαu(µ)ׯu(e)(1 γ5)γαvνe).(1)
The complex conjugate of this amplitude
M=GF
2h¯u(µ)γβ(1 + γ5)u(νµ)iׯvνe)γβ(1 + γ5)u(e)(S.1)
has the opposite sign of the γ5because ¯γ5γ0(γ5)γ0=γ5. Consequently,
|M|2=1
2G2
Fh¯u(νµ)(1 γ5)γαu(µu(µ)γβ(1 + γ5)u(νµ)i(S.2)
ׯu(e)(1 γ5)γαvνe)¯vνe)γβ(1 + γ5)u(e)
and hence
1
2X
all
spins
|M|2=1
4G2
Ftr(1 γ5)γα(6pµ+Mµ)γβ(1 + γ5)(6pνµ+mνµ)
×tr(1 γ5)γα(6p¯νemνe)γβ(1 + γ5)(6pe+me)
1
4G2
Ftr(1 γ5)γα(6pµ+Mµ)γβ(1 + γ5)6pν
×tr(1 γ5)γα6p¯νγβ(1 + γ5)6pe
(S.3)
where the approximation is me0; we also make use of mνe=mνµ= 0 (which may be exactly
true or just a very good approximation, future data will tell) and simplify notations: pνpνµ
and p¯νp¯νe. Please note that here and henceforth the indices µ, ν, ¯ν , e denote the particles
to which respective momenta belong and have nothing to do with the Lorentz indices of those
momenta. For the Lorentz indices, I use here α,βand later also γ,δ,σand ρ. Thus, pµα is
the α’s component of the muon’s 4–momentum, etc.,etc.
1
pf3
pf4
pf5

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PHY–396 K/L. Solutions for problem set #12.

Problem 1 :

Note the correct muon decay amplitude

M(μ

→ e

e

G

F

[

u¯(ν

u(μ

]

×

[

u¯(e

v(¯ν

e

]

The complex conjugate of this amplitude

M

G

F

[

¯u(μ

)u(ν

]

×

[

v¯(¯ν

e

)u(e

]

(S.1)

has the opposite sign of the γ

because ¯γ

. Consequently,

|M|

G

F

[

u ¯(ν

u(μ

)¯u(μ

)u(ν

]

(S.2)

×

[

u¯(e

v(¯ν

e

)¯v(¯ν

e

)u(e

]

and hence

all

spins

|M|

G

F

tr

( 6 p

+ M

)( 6 p

+ m

× tr

( 6 p

e

− m

e

)( 6 p

e

+ m

e

G

F

tr

( 6 p

+ M

) 6 p

× tr

p

) 6 p

e

(S.3)

where the approximation is m

e

≈ 0; we also make use of m

e

= m

= 0 (which may be exactly

true or just a very good approximation, future data will tell) and simplify notations: p

≡ p

and p

≡ p

e

. Please note that here and henceforth the indices μ, ν, ν, e¯ denote the particles

to which respective momenta belong and have nothing to do with the Lorentz indices of those

momenta. For the Lorentz indices, I use here α, β and later also γ, δ, σ and ρ. Thus, p

is

the α’s component of the muon’s 4–momentum, etc., etc.

Having derived eq. (S.3), we now need to evaluate the traces. For the first trace, we have

tr

( 6 p

+ M

) 6 p

= tr

( 6 p

+ M

p

= tr

( 6 p

+ M

p

= 2 tr

( 6 p

+ M

p

〈〈using tr(γ

p

) = tr(γ

p

) = 0〉〉 (S.4)

= 2 tr

p

p

− 2 tr

p

p

[

p

p

+ p

p

− g

(p

· p

]

+ 8i

p

p

Similarly, the second trace evaluates to

tr

p

e

) 6 p

[

(p

p

+ p

p

− g

(p

e

· p

]

+ 8i

p

p

e

. (S.5)

It remains to substitute the trace formulæ (S.4) and (S.5) back into eq. (S.3) and contract

the Lorentz indices. Thus,

all

spins

|M|

= 16 G

F

([

p

p

+ p

p

− g

(p

· p

]

+ i

p

p

×

([

p

p

+ p

p

− g

(p

e

· p

]

+ i

p

p

e

〈〈using symmetry/antisymmetry of factors under α ↔ β 〉〉

= 16 G

F

[

p

p

+ p

p

− g

(p

· p

]

×

[

p

p

+ p

p

− g

(p

e

· p

]

p

p

× 

p

p

e

= 16 G

F

[

2(p

· p

e

)(p

· p

) + 2(p

· p

)(p

· p

e

− 2(p

· p

)(p

e

· p

) − 2(p

· p

)(p

e

· p

) + 4(p

· p

)(p

e

· p

]

[

2(p

· p

)(p

· p

e

) − 2(p

· p

e

)(p

· p

]

= 64 G

F

(p

· p

)(p

· p

e

(S.6)

Q.E.D.

and hence

dP =

d

×

p

p

E

E

E

dp

dp

d(cos θ

) δ(E

+ E

+ E

− E

tot

p

=−(p

+p

. (S.12)

Next, we use the cosine theorem

p

= (p

+ p

= p

+ p

+ 2p

p

cos θ

which gives

d(cos θ

p

dp

p

p

(for fixed p

, p

) and therefore

dP =

d

×

p

p

p

E

E

E

dp

dp

dp

δ(E

+ E

+ E

− E

tot

). (S.13)

Finally, we notice that for a relativistic particle of any mass, pdp = EdE and hence (S.8).

It remains to determine the limits of kinematically allowed ways to distribute the net

energy E

tot

of the process among the three final particles. Such limits follow from the triangle

inequalities for the three momenta,

p

≤ p

+ p

, p

≤ p

+ p

, p

≤ p

+ p

, (S.14)

which look simple but produce rather complicated inequalities for the energies. However, when

all three final particles are massless, the kinematic restrictions become simplify to

E

, E

, E

E

tot

, E

+ E

+ E

= E

tot

. (S.15)

Problem 2 :

We are now ready to calculate the muon decay rate and the electons’ spectrum. According to

the general rules of decay

dΓ =

|M|

2 M

dP , (S.16)

thus in light of eqs. (2) and (S.8),

dΓ(μ

→ e

e

G

F

M

(p

·p

)(p

e

·p

)×dE

e

dE

dE

d

Ω δ(E

e

+E

+E

−M

). (S.17)

In the muon’s frame,

(p

· p

) = M

E

(S.18)

while

(p

e

· p

e

) = E

e

E

− p

e

p

cos θ

= E

e

E

p

e

p

p

; (S.19)

neglecting the electron and neutrino’s masses, we may rewrite (S.19) as

(E

e

+ E

E

M

(M

− 2 E

). (S.20)

Consequently,

dΓ(μ

→ e

e

G

F

M

E

(M

− 2 E

)×dE

e

dE

dE

d

Ω δ(E

e

+E

+E

−M

). (S.21)

At this point we are ready to integrate over the final-state variables. In light of

d

and the kinematic limits (S.15), we immediately obtain

→ e

e

G

F

M

M

dE

e

dE

dE

E

(M

− 2 E

)δ(E

e

+ E

+ E

− M

G

F

M

M

dE

e

M

M

−E

e

dE

E

(M

− 2 E

G

F

M

M

dE

e

E

e

M

E

e

(S.22)

In other words, the partial muon decay rate with respect to the final electron’s energy is given