Concepts of the Standard Model: renormalisation FK8022, Lecture 2 Core text: Quarks and leptons: an introductory course in modern physics, Halzen and Martin Further reading: Basics of QCD perturbation theory, D.E. Soper (hep-ph/9702203)
Feb 21, 2016
Concepts of the Standard Model: renormalisation
FK8022, Lecture 2
Core text:Quarks and leptons: an introductory course in modern physics, Halzen and MartinFurther reading:Basics of QCD perturbation theory, D.E. Soper (hep-ph/9702203)
Lecture outline
• Infinities arising from loops– Regularisation– Reparameterisation of charge – Renormalisation
finite charge, amplitude Renormalisation scaleRunning of couplings
A simple QED process
23 1 4 22
2 21 3 0.
Consider scattering. Apply Feynman rules to obtain amplitude:
where and
e
ge u p u p u p u p
Q
q p p Q q
M
We are using perturbation theory so the above Feynman diagram should give the approximately correct amplitude withhigher order processes changing the results slightly.
e e
p1
p2 p4
p3
q
2
2 23 1 4 22
2 2
2
22
2
1 ( )
1 ( )
( )
6 (1 ) ln 13
Simplify:
integral over internal loop momenta to divergent contribution of loop
m
ge u p u p I Q u p u p
Q
e I Q B
I Q
dz QI Q z z zz m
M
M
1
0
2
1
4 mass,
z dz
em e
Adding a higher order process
+e e
e e
e e
2
2
2 2
1 22
20
2
2
2
22
2
6 (1 ) ln 1 13
ln
ln ln3
Regularise divergent integral:
Can send to later. Solve first and second integrals:
m
M
m m
dz QI Q z z z z dzz m
dz dz Mz z m
M
M QI Qm
2 2
2 2
2 2
ln3
Mm Q
Q m
Renormalised charge
22
2
2 2 22 2 2 2
2 2 2
2
-4
-4 1 ( ) 4 1 ln3
1 ln 1 ln3 12
-4
,
Redefine coupling, charge:
- finite!
renormalised charge/co
r r
r
r r
B
MI q B BQ
M e MQ e Q eQ Q
Q B
e
M
M
M =
2.,
upling i.e. measured in lab, varies with unobservable "bare" charge/coupling of electron
Finite finite if is infinitesimal and cancels divergence from .r
Qe
e e M
M
Bare and renormalised charges
"bare" charge of electron whenstripped of loops : infinitesimal. The charge which would be seenfor an interaction at zero distance or infinite energy unobservable!
e
e
re2.
.
renormalised charge which is
measured in lab and varies with Divergent loops "absorbed" into the
definition of
r
r
e
Q
e
We were using the wrong charge.
Defining the coupling at a scale
22
2
2
222
2 2
2
2 22
22
2
-4 1 ( ) 4 1 ln3
1 ln3
1 ln3
4 1 ln 43
1 ln3
Define at scale
Have freedom to define at a
r
rr
rr
r
MI Q B BQ
Q
QMQQ M
Q
Q M B QQM
Q
M
M
2
22 22
2 22
2
1 ln 4 1 ln3 3
1 ln3
ny arbitrary scale
Need to rewrite in terms of finite quantities
rr
M M BQM
M
2 2
22
2
2 2 22
22
2
2 2 22
2
4 1 ln3
1 ln3
ln3
1 ln3
ln3
higher orders
higher orders
Estimate t
r
r rr
rr
M BQM
MM
M
M
2
2 22 22
2 2
2 22
2
( ) :
-4 1 ln 1 ln3 3
- 4 1 ln3
o
Finite amplitude with finite terms but depending on an arbitrary number!
r
r rr
rr
M M BQ
Q B
M
M
O
22 22
2 2
2 22 22
2 2
4 1 ln - 4 1 ln3 3
-4 1 ln ln3 3
(A) Photon exchange - no loops
(B) Photon exchange - one loop at m
rr
r rr
M QB BQ
M M BQ
M
2 2
2 2
2 2 2 2
-
,
omentum transfer =
(C) Photon exchange - one loop at momentum transfer =
Amplitude
renormalisation scale
scale at which "infinities are removed"+ charge/coupling set: r r
q
A B C
e
Renormalisation scale
[ ]- - + higher orders
2At Q 2At Q 2 2At Q
(A) (B) (C)
2 2
22 2
2
22 2
1 ( ) , -4 1 ( )
-4 1 ( ) ( ) ..
11 ...1
1-41 1
One loop.
Infinite number of loops :
Taylor expansion: +
,
r
r
I Q I Q B
I Q I Q B
X XX
Q BI Q I Q
M
M
M
Higher orders
}
Scale dependence of amplitude
renormalisation scale. It is arbitrary!No observable can depend on an arbitrary parameter ! Any scale will eventually give the right answer if all orders are calculated. Large variation at lower or
2 2.,
ders.
For QED the optimal scale is known: For QCD finding the right scale is an open question.
Q
r(Q2)2 20 Q
2 21 Q 2 21 2 2 22 3
Order of calculation
e scatteringSingle photon exchange
22
22
2
22 2
2 2
2 2
2 22 2
1
1 ln3
11 11 ln ln
3 3
1 1 1 1 1 1ln ln3 3
At scale :
;
r
r
r
r r
QI Q
QMQ
c cM Mc c
M MQ cQ c
Running coupling
2 2 2
2 2 22 2
22
2 2 2
22 2
1 1 1 1ln ln ln3 3
11 1 ln 1 ln3 3
We can't predict from first principles but we can predict
it's value at one momen
r r
rr
r
r
r
M M QQ c cQ c
cQ
Q c Qcc c
2 2 !tum scale if we know it another value
The coupling changes with momentum transfer scale.
The above is an approximation. Loops from other particles, eg muons,will also play some role.
q c
Consistency check
2
2 22
2
2 2 2
2 22 2
2
-4 1 ln3
-4
1 ln3
Consider scattering.
At renormalisation scale
At "correct" QED scale
Amplitude must be independent of scale.
rr
r
rr r
e
Q B
Q B Q
M
M
2 2 2
2 222 2
2
1 ln3
1 ln3
Check consistency with formula for running:
The "running" of ensures that an observable does not depend on the choice of
r
r rr r
r
r
QQQ
renormalisation scale.
Divergence in amplitude from
higher order loop
Make finite by redefining coupling/charge and remove infinity
For a complete expansion the amplitude is independent of r
Renormalisation
Finite expression for running of coupling/charge with r
Coupling/charge depends on an arbitrary kinematic scale r for a given interaction
Renormalisation works: electromagnetic coupling running
Interaction distance
(momentum transfer)2 /GeV2
, , , , , , , ,e u d s c b t
(5)
2
2
(5) 2
01
0.031497686
0.00007
0.0275 0.0
emem
e top had
e Z
top Z
had Z
M
M
M
Vacuum polarisation contributions from all leptons and quarks.
Calculable:
Not calculable (pQCD not valid):03 e e - from data.
Large uncertainty - affects precision measurements.
Tiny shift
Physical interpretation of the running coupling
+
e-
The "vacuum" consists of virtual particles fluctuating into and out of existence.An electron is surrounded by virtual particles which act to shield the charge asin a polarised dielectric.
e-e-
e- e-
e- e-
e+,e-
e+,e-
e+,e-
Distance scale
Coupling
Renormalisation of other quantities• Different loop diagrams cause other physical
quantities to be renormalised.• Eg mass
• Masses also run:
What about the strong force ?
q q
q q
q q
q q
q q
q qq q
q q
q,q
Similar story as for electromagnetism except that gluonscan self-interact (they carry colour - the photon carries no charge!)This turns out to be critical.....
q,q
q,q + other higher order diagrams
Asymptotic freedom
s
Momentum transfer /GeV
Interaction distance
12
2 2 22
33 21 ln
6
0.118 0.002
number of quark flavours
Varies strongly with momentum!!
fs s s
f
s Z
N QQ
N
M
Electromagnetic force (QED)Electric charge screened: distance > Compton wavelength
Strong force (Quantum chromodynamics: QCD)Effective colour charge grows at larger distances.Distances < fm quasi
c
-free quarks Asymptotic freedom! Nobel prize (2004) for Gross, Politzer and Wilczek.
Renormalisation scale setting
-
22
2
2
Process:
4 1
centre-of-mass energy ; 3 (no. of colours)
sum over squared charges of quarks which can be produced.
= contribution from pQCD proces
c i QCDi
c
ii
QCD
e e hadrons
N es
s N
e
ses
22
222 2
1.4092 1.9167 ln
12.805 7.18179ln 3.674 ln ...
s sQCD
s
s
s s
2
ln
Coefficients and depend on renormalisation scale.
Scales usually chosen to have a value close to the kinematic hard
scattering scale (eg ). This avoids large logs and
ensures faster
s
ss
convergence in a perturbative series.
Renormalisation scale setting
Scale variation
1
12
2 2 22
22 2 2
2
21 1
Change in scale from ' for leading order calculation:
33 2 '' 1 ln 6
33 2 ' ln 6
33 2
6
s
fs s s
fs s
fs s
c
N
N
Nc c
M
M 2
2 22
'ln
scale variations higher orders in . scale variations offer some sensitivity to missing higher orders.
Typical choices , 22
(More in lecture 13 - simulation technique
s
s
s).
Summary and discussion (1)
General:When including loops the Feynman diagram machinery can break down owing to divergences related to unknown physicsat high energy (short distance). The divergences can be removed by absorbing th
2
2
.
em into thedefinition of a renormalised physical quantity.
Specific for our example process:
The divergent term ln emerges and is cancelled by the
"bare" charge This gives the renormalise
Mm
e
d coupling .
re
Summary and discussion (2)
General:The physical quantity receives a finite correction in addition to the divergence removal.
Specific for our example process:The renormalised coupling/charge varies with the momentum transfer/scale.
Summary and discussion (3)
Renormalisation originally seen as a mysterious stop-gap measure.It is now better understood Nobel prizes (eg Wilson, 't Hooft).
SM integrals with shouldn't necessarily be problem-free !We know th
p
e SM must break down eg, at .
Short distance stuff beyond the SM *should* be absorbed away. Successful theories do not couple short and long distance scales.Eg planetary motion with Newton's l
PlanckM
aws does not need quarks. QCD generates visible mass : absorbed in the planets' masses.