particles and deep inelastic scattering...these are spin 1/2 particles scattering through the...
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Heidi Schellman Northwestern
Particles and Deep Inelastic Scattering
Heidi Schellman
Northwestern University
HUGS - JLab - June 2010
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Heidi Schellman Northwestern
k
P
k’
P’
q
A generic scatter of a lepton off of some target. kµ and k′µ are the
4-momenta of the lepton and Pµ and P ′µ indicate the target and the final
state of the target, which may consist of many particles. qµ = kµ − k′µ is the
4-momentum transfer to the target.
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Lorentz invariants
k
P
k’
P’
q
The 5 invariant masses k2 = m2` , k′2 = m2
`′, P2 = M2, P ′2 ≡W 2, q2 ≡ −Q2
are invariants. In addition you can define 3 Mandelstam variables:
s = (k + P )2, t = (k − k′)2 and u = (P − k′)2.
s+ t+ u = m2` +M2 +m2
`′ +W 2. There are also handy variables
ν = (p · q)/M , x = Q2/2Mµ and y = (p · q)/(p · k).
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In the lab frame
k
M
k’
q
θ
P’
The beam k is going in the z direction. Confine the scatter to the x− z plane.
kµ = (Ek, 0, 0, k)
Pµ = (M, 0, 0, 0)
k′µ = (E′k, k
′ sin θ, 0, k′ cos θ)
qµ = kµ − k′µ
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In the lab frame
k
M
k’
q
θ
P’
s = E2CM = 2EkM +M2 −m2 → 2EkM
t = −Q2 = −2EkE′k + 2kk′ cos θ +m2
k +m′2k → −2kk′(1− cos θ)
ν = (p · q)/M = Ek − E′k energy transfer to target
y = (p · q)/(p · k) = (Ek − E′k)/Ek the inelasticity
P ′2 = W 2 = 2Mν +M2 −Q2 invariant mass of P ′µ
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In the CM frame
k
P
k’
q
P’
The beam k is going in the z direction. Confine the scatter to the x− z plane.
kµ = (Ek, 0, 0, k)
Pµ = (EM , 0, 0,−k)
k′µ = (E′k, k
′ sin θ, 0, k′ cos θ)
qµ = kµ − k′µ
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In the CM frame
k
P
k’
q
P’
s = E2CM = (Ek + EM )2 → 4k2
t = −Q2 = m2k +m′2
k − 2(EkE′k − kk′ cos θCM )→ −2kk′(1− cos θCM )
ν = (p · q)/M =(Ek − E′
k)EM + k(k − k′ cos θ)M
→ k2
M(1− cos θCM )
y = (p · q)/(p · k) =(Ek − E′
k)EM + k(k − k′ cos θ)EkEm + k2
→ 1− cos θCM2
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For such a two body process the cross section looks like
dσ
dt=
164π
1s
1|kCM |2
|M|2
kCM =kM√s→√s/2
dσ
dt=
164π
1k2M2
|M|2 → 116π
1s2|M|2
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e− + µ+ → e− + µ+
e
µ
e
µγ
electron muon scattering occurs through the t channel (ie the exchanged γ
has momentum qµ.).
dσ
dt= 2πα2 s
2 + u2
s2t2dσ
dy= 4πα2 s
Q4
12[1 + (1− y)2]
]
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Angular dependence
µ e
µ
eJ = 1
µ e
µ
e J = 0
What angular dependence do we expect?
These are spin 1/2 particles scattering through the exchange of a spin 1
particle so one expects to have final state with:
no angular dependence
(Jz = 0) , dσdy → 1
(Jz = 1) , dσdy → (1 + cos θcm)2 → 1
4 (1− y)2
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νµ + e−+→ µ− + νe
νµ
e
µ
W
νe
−
muon neutrino scattering also occurs through the t channel (ie the exchanged
W has momentum qµ.).
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If you do a substitution of weak interaction variables into the µe→ µe process
α →√
2πGFM
2W
1Q2
→ 1Q2 +M2
W
dσ
dy= 4πα2 s
Q4
12[1 + (1− y)2
]→ G2
FM4W
(M2W −Q2)2
s
π
Note that the weak interaction only allows one angular momentum
combination (Jz = 0) in this case.
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Now we can start studying more complexobjects
kk’
q
P’p’xPp=
If you scatter an electron off of something - you get an electron - or possibly
an electron neutrino. But when you scatter off a proton, you can either get a
proton out (elastic scattering) or a neutron (quasi-elastic scattering) or a
bunch of hadrons (inelastic scattering).
Since the proton breaks up, it must be composite. So maybe we can probe
the stuff inside using electron, muons and neutrinos.
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A quasi-elastic neutrino reaction in the Minerva neutrino detector
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kk’
q
P’p’xPp=
Imagine a quark carrying momentum fraction x of the proton momentum PµPand scatter an electron off of it. This is a t channel process. Imagine that you
only detect the incoming and outgoing scattered electrons. Assume the
electron mass is zero.
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kk’
q
P’p’xPp=
in a frame where EP >> MP
kµ = (E, 0, 0, E), k′µ = (E′, E′ sin θ, 0, E′ cos θ)
PµP = (EP , 0, 0,−EP )
pµ = xP = (xEP , 0, 0,−xEP )
p′µ = kµ + pµ − k′µ = qµ + pµ
pµpµ = p′µp′µ = x2M2
P
The last expression assume the quark is still the same after the scatter.
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Observables - charged lepton scatteringYou know the target mass M
You can measure the incoming and outgoing electron or muon momenta kµ
and k′µ.
From these you can calculate the invariants s, ν, Q2.
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One can solve for x!
(p′)2 = (q + p)2 = q2 + p2 + 2(q · p)
x2M2P = −Q2 + x2M2
P + 2x(q · P )
Q2 = 2xνM
x =Q2
2Mν
You can measure x, the fraction of the total momemtum carried by an
individual parton just by measuring the incoming proton momentum and the
incoming and outgoing electron 4-vectors.
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So what would we expect to see?
u
d
u
uu
d d
Proton
A proton has 2 u quarks and a d quark. So we’d expect the electron-quark
electron center of mass energy s→ s = xs and the charge factor
α2 → α2( qi
e )2.
Naively we’d expect each quark to carry 1/3 of the momentum, so the x
probability densities would be δ(x− 1/3).
d2σ
dydx=∑i=1,3
4πα2q2isxiQ4
δ(xi − 1/3)12[1 + (1− y)2]
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What we expect to see
1/3x
σ
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The u quarks have charge 23e while the d quarks have charge − 1
3e.
We’d also predict that a neutron would have a scattering cross section which
is smaller by a factor of:
σnσp
=(− 1
3 )2 + (− 13 )2 + ( 2
3 )2
( 23 )2 + (− 1
3 )2 + ( 23 )2
=23
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What we actually see
What we actually see when we plot cross sections vs x. There are no little
spikes at (1/3)!
(this is e+ p→ e+X data from the Zeus experiment at HERA)
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n/p
Observed n/p ratio as a function of x.
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New model of the proton
u
d
u
uu
d d
Proton
Our new model has the proton containing the 3 ”valence” u and d quarks but
a whole sea of quark anti-quark pairs.
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We can measure the momentum fractionx carried by these quarks!
At each x the total cross section will be depend on the probability of there
being a quark of fraction x around and on the rate for hard electron-quark
scattering.
These probability density functions are called ”Parton Distribution Functions”
or PDF’s.
dσ
dx(e+ p→ e′ +X) =
∑i
dσ
dx(e+ i→ e+ i; s, t, u)fi(x)
By measuring dσdx on different targets and using the simple predictions for the
σ(e+ qi → e+ qi;xs) one can measure the different fi(x).
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quark kinematics compared to protonkinematics
In all frames:
s = (k + xp)2 = k2 + 2xkp+ x2M2 ' 2xkµpµ = xs (1)
t = t = (k − k′)2 (2)
u = = (p− k′)2 ' xu (3)
In the cm frame
s = xs (4)
t = −xQ2 = −xs sin2 θcm2
(5)
u = −xs cos2θcm2
(6)
(7)
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If we substitute s/x and Q2 for s and t we end up with:
dσ
dxdy(e+ P → e+X) =
4πα2s
Q4×
12[1 + (1− y)2]×
x[49(u(x) + u(x)) +
19(d(x) + d(x))
+19(s(x) + s(x))] + ...
Note: this is an approximation - we’ve neglected quark and lepton masses in
assuming s = xs.
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What can neutrons tell usEarly in the history of particle physics Heisenberg noticed that the strong
interactions didn’t care if particle was a neutron or a proton. In modern
language this means that the strong interaction is flavor blind. This leads to
an approximate symmetry called Isospin where the proton and neutron are the
+1/2 and −1/2 eigenstates and the symmetry acts like spin.
The u and d quarks have the same relation under isospin as the proton and
neutron and it has been argued that the u content of the neutron un(x)should be the same as the d content of the proton dp(x)
ie applying an isospin rotation to a neutron changes it to a proton and also
exchanges all the u and d quarks.
We’re not certain this is perfectly so (after all the neutron and proton do
differ a bit).
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But it does mean that scattering from neutrons should be like:
dσ
dydx(e+ n) =
4πα2s
Q4× 1
2[1 + (1− y)2]×
x[49(un(x) + un(x)) +
19(dn(x) + dn(x)) +
19(sn(x) + sn(x))] + ...
=4πα2s
Q4× 1
2[1 + (1− y)2]×
x[49(dp(x) + dp(x)) +
19(up(x) + up(x)) +
19(sn(x) + sn(x))] + ...
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And if you assume that the s quarks are the same for protons and neutrons
you can look at the difference.
1x
[dσ
dx(e+ p)− dσ
dx(e+ n)
]∝ 1
3[u(x) + u(x)− d(x)− d(x)]
You can use this to check to see if there really is one more u than d quark in
the proton.
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