particle physics particle physics chris parkes symmetries,invariances and conservation laws (or how...
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Particle Particle PhysicsPhysics
Chris Parkes
Symmetries,Invariances and Conservation laws(Or how to decide whether to shake hands with an alien!)
•Conserved quantities in QM
•Parity
•Scalars,Vectors and pseudo-S,axial-V
•CP,T
4th Handout
http://ppewww.ph.gla.ac.uk/~parkes/teaching/PP/PP.html
Symmetries and Symmetries and Conservation LawsConservation Laws
Quantum numbers are associated with the conserved observablesSome are universal laws of nature (p,E,L,CPT…), others are valid only in approximations(e.g. parity - valid for strong/EM force but not weak)
In classical physics there are a number of quantities which are conserved –momentum, energy, angular momentumConservation theorems also occur in QM
In classical physics the conservation laws tend to be the starting points(there are also more sophisticated way of deriving them)
In QM however the conservation laws are deeply related to the principle of superposition of amplitudes and the symmetry of the system.
we will deal with both continuous (e.g. displacement in space/time) and discrete symmetries (e.g. mirror like)
Emmy Noethe
rNoether’s theorem – Symmetries (invariances) naturally lead to
conserved quantities
C P
CPParity InversionSpatialmirror
Charge InversionParticle-antiparticlemirror
Conserved quantities in QMConserved quantities in QM- Revision- Revision
Any operator, Â, which is time independent (e.g. p) and commutes with the Hamiltonian is associated with a conserved quantity.
HAidt
Ad
AHHAit
A
dt
Ad
AHHAit
A
dt
Ad
Att
At
A
dt
Ad
dt
Ad
dAA
ˆ,ˆ10
ˆ
ˆˆˆˆ1ˆˆ
ˆˆˆˆ1ˆˆ
ˆˆˆ
0ˆ
)(ˆ)(ˆ
***
***
*
xxxExpectation valueOf operator
Conservation requires(e.g. momentum)
Thus if A is indep.of time the expectation value is constant, as long as A,H commute
)(ˆ1)(
)(ˆ1)(
**
tHit
t
tHit
t
Hamiltonian
Minus sign from complex conjugate
Translational InvarianceTranslational Invariance linear momentum conservation linear momentum conservation
M&S 4.1
i.e. wish to show p operator independent of time 0ˆ,ˆ1ˆˆ
Hitdt
dp
pp
Invariance: All positions in space are physically indistinguishableConsider moving a particle a small distance xxxx '
)()'(
)'()()(2
21
xx
xxx
HH
H
HHxH
m
Depends on derivatives not on position (natural units)
define operator D that performs this translation
)()ˆ1()(ˆ
....)()()()(ˆ
xpxx
xxxxxx
iD
D Higher order terms
ip̂Since in natural units
)(ˆ)(ˆ)()(ˆ)(')('ˆ
)()(ˆˆ)('ˆ
xxxxxxxxx
xxx
DHHD
HDD
)()(ˆ)(' xxx HConsider wavefunction
1)2)
Comparing 1)&2),
0]ˆ),ˆ1[(
0]ˆ,ˆ[
)(ˆ)(ˆ)()(ˆˆ
Hi
HD
DHHD
px
xxxx 1, ix just numbers so
=0
0ˆ,ˆ Hp
Hence, linear momentum is conserved and is a good quantum number
Rotational InvarianceRotational InvarianceAngular Momentum ConservationAngular Momentum Conservation
M&S 4.2
•All directions in space are physically indistinguishable•Rotating a system of particles around its CM to a new orientation
leaves its physical properties unchanged Proof is very similar to translation, see lectures
This proof considers only L, in general must also consider spinGet
SLJ 0ˆ,ˆˆ,ˆ
0ˆ,ˆ
HH
H
SL
J
Translations in timeTranslations in timeEnergy ConservationEnergy Conservation
)()()(ˆ
)()()()(ˆ
tEtt
itH
tdt
tttttA
Define an operator for time evolution, A
But wait, we already have this operator, it is the hamiltonianTISE
And H commutes with itself 0ˆ,ˆ HHSo time translation is the symmetry, H is operator, E is the conserved quantity
N.B. time translation invariance is different from time reversal operator T– discussed later
•Laws of physics independent of time
Other conserved quantitiesOther conserved quantitiesElectric Charge, Colour Charge, Baryon number, lepton number, strangeness..
First three always conserved (strong,EM,weak)Last one not conserved in weak e.g. p0
Other Discrete Symmetry operatorsOther Discrete Symmetry operatorsParity (P) – spatial Inversion
Charge conjugation (C) – particles anti-particlesreverses: charge
magnetic momentsbaryon numberstrangeness
Only particles that are their own anti-particles are eigenstates of C
Time (T) - Time reversal
Discuss P,C,CP/T, particularly for the weak force
CPT – combined is a fundamental symmetry of QFTs, arising from very basic assumptions like Lorentz invariance
Q) Is there a difference in behaviour between matter and anti-matter ?
Parity - Spatial InversionParity - Spatial Inversion
P operator acts on a state |(r, t)> as
),(),(
),(),(
2 ttP
ttP P
rr
rr
Hence for eigenstates P=±1
(r, t)>= cos x has P=+1, even
(r, t)>= sin x has P=-1, odd
(r, t)>= cos x + sin x, no eigenvalue
e.g. hydrogen atom wavefn
(r,, )>=(r)Ylm(,)
Ylm(,)= Yl
m(-,+)
=(-1)l Ylm(,)
So atomic s,d +ve, p,f –ve P
Hence, Electric dipole transition l=1P=- 1
Discrete symmetry 0ˆ, HP
Parity conserved when Hamiltonian invariant under Parity transformation (strong,EM)
Parity ExamplesParity Examples
Conventions – quarks and leptons have +ve parityAnti-quarks and anti-leptons have –ve parity
•Parity multiplicative
•For a meson made from q qbar pair with orbital angular momentum l
•|> = a b, P=PaPb(-1)l
For ground state (l=0) Pmeson=-1, expect –ve parity for light mesons
-,o,K-,Ko all P=-1
For baryons:
0)1()1(
)1()1)()()((
312
312
ll
llcbaBaryon PPPP
So, expect+ve parity for low lying states
For anti-baryons:
1)1)(1(
)1)()()((
312
312
ll
ll
cbaBaryonPPPP
expect-ve parity for low lying states
l12l3
q1 q3
q2
Scalars,Vectors,Pseudo-Scalars,Axial VectorsScalars,Vectors,Pseudo-Scalars,Axial VectorsScalar – unaffected by parity (+ve parity)Vector – reverses (-ve parity) pprr ,
Can also form quantities from ‘.’ and ‘X’ products of vectors.How do the resultant scalars/vectors behave ?
Axial vector: consider cross-product of two vectors
LprL
prL
)()()(PBoth reverse under parity, so L unaltered
p
r-r
-p
Pseudo-scalar: consider dot product of two vectors
In a parity conserving theory you can’t add an axial vector to a vector
bababa )()()(P Acts like a scalar
Now, consider dot product of vector, axial vector
pLpLpL )()()(P Changes sign , a pseudo-scalar
This leads to parity violation in weak interactions
Weak Force Parity Violation Weak Force Parity Violation Discovery “Discovery “--” problem” problem
Same mass, same lifetime, Same mass, same lifetime, BUTBUT ++, , (21%)(21%) P P =+1 =+1 ++++-, -, (6%) (6%) P P =-1 =-1
Actually K+
Postulated Yang& Lee, 1956
C.S. Wu et. al., Phys. Rev. 105,
1413 (1957) B field
e- (E,p)
Co60Nuclei
spin aligned
Beta decay to Ni*60
e- (E,-p)
Parity
Spin axial vector
-> maximal violation
V-A theory, neutrino handedness
Experimental discovery
Revision
Operating with P on this reverses p, not spin, produces a right-handed neutrino.Do not observe:
Helicity and the neutrinoHelicity and the neutrinoIn angular momentum we choose the axis of quantisation to be the z axis.Lets choose this axis along the particle momentum direction.Helicity is the component of the spin along the momentum direction.•A spin ½ particle can thus have helicity +1 (ms=+ ½) or –1 (ms=- ½ ) E
pσ ˆˆ
Not so interesting for a massive particle, as not Lorentz invaraint, but consider the neutrino.
p
s+1 -1
p
sRight-handed Left-handed
1) Only left-handed neutrinos exist and right-handed anti-2) Helicity is a pseudo-scalar
Operating with C on this produces a left-handed anti-neutrino.Do not observe: LLC ˆ
RLP ˆ
RRC ˆ
LRP ˆ
Operating with C and P on this produces a right-handed anti-neutrino.Do observe! RRL CPC )(ˆ)ˆ(ˆ
Weak force violates Parity, but CP OK?
Measuring Helicity of the NeutrinoMeasuring Helicity of the Neutrino
152 152 * 152Eu Sm Sm (960 KeV)
J=0 1 1/2 0 1
ee
152 * 152Sm Sm
J= 1 0 1
Goldhaber et. al. 1958
Electron captureK shell, l=0
photon emission
Consider the following decay:Consider the following decay:
Eu at restSelect photons in Sm* dirn
Neutrino, SmIn opposite dirns
e-
•Momenta, p
•spin
OR
S=+ ½
S=- ½Left-handed
S=+ 1
S=- 1
right-handed
Left-handed
right-handed
•Helicities of forward photon and neutrino same•Measure photon helicity, find neutrino helicity
Neutrino Helicity ExperimentNeutrino Helicity Experiment
Tricky bit: identify forward Tricky bit: identify forward γ γ Use resonant scattering!Use resonant scattering!
Measure γ polarisation with different B-field orientationsMeasure γ polarisation with different B-field orientations
152 152 * 152Sm Sm Sm
magnetic field
Pb
NaI
PMT
152Sm152Sm
152Eu
γγ
Fe
Similar experiment with Hg carried out for anti-neutrinos
Vary magnetic field to vary photon absorbtion.Photons absorbed by e- in iron only if spins of photon and electronopposite.
)2
1()
2
1()1(
)2
1()
2
1()1(
'
ee SSS
Forward photons,(opposite p to neutrino),Have slightly higher p than backwardand cause resonant scattering
Only left-handed neutrinos exist
CP ViolationCP Violation•Parity is violated by weak force•But neutrino analysis shows CP looks OK.
History repeats itself, just as we expected parity to be conserved, we then expected CP to be conserved.Actually violated by a tiny amount – currently a hot research topic
CPT is conserved so CP violation is equivalent to T violation
QM + relativity:Gave us matter/anti-matter symmetry
So why is our world full of protons,neutrons,electronsand not anti-protons, anti-neutrons, positrons?
Historical accident that our corner of universe has more matter than anti-matter ?No, astronomical evidence tells us that observable universe is all made of matter.
CP/T violation is the key….
C P
CPParity InversionSpatialmirror
Charge InversionParticle-antiparticlemirror
Time reversal – TTime reversal – Tttt ' Leaving all position vectors x unchanged
but p,J reverse
Detailed balanceDetailed balance
),(),(),(),( ddccbbaa mdmcmbma pppp
Compare reaction
With time reversed counter-part
),(),(),(),( bbaaddcc mbmamdmc pppp
Where m are spinZ-components
Conserved for Strong,EMWe wish to test this for the weak force
Inverse experiments are difficult to do with the weak force, need to avoid strong/EM contaminatione.g. reversed would beWould be dominated by strong interaction of proton,pion.Neutrino expt. would be possible, but difficult and looking for a small effect
Particle are eigenstates of P, neutral particles can be of C, but cannot be identical to itself going backwards in time
0 p p0
Let us have a quick look at nature....Let us have a quick look at nature....
Neutral kaon system sdK0 sdK0 flavour eigenstates CP conjugated
m
cm
6.15c
s1004.017.51
7.2c
s100008.08934.01
L
8
LL
S
10
SS
mass eigenstatesKS
KL
Short lifetime
Long lifetime
are a mixture of flavour eigenstates
Time dilation - factor needed for actual flight distance in lab
Mainly Decays to three pions (34%)3 x m(pion) ~ m(Kaon)
Mainly Decays to two pions (99.9%)
CPLEAR- some parametersCPLEAR- some parameters•Beam – 106 anti-protons /s into Hydrogen target•Fast online trigger selection of events ~ 103/s•Ability to separate charged pions / kaons using Cherenkov, dE/dx, Time of flight
discriminate in momentum range 350-700 MeV/c•Can detect and reconstruct Ks vertex to ~ 60 lifetimes c~2.6 cm•Observe events over ~ 4•Magnetic field (0.4T) and tracking leads to particle momentum determination• (~5% accuracy)
Kaon OscillationKaon Oscillation
Rate difference Ko Ko Ko Ko is T violation
Particle can turn into anti-particle. So say at t=0, pure Ko, later a superposition of states
d
su, c, t W
W_
s
d_u, c, t
ds
u, c, tW W
_ sd_
u, c, t___
K0K0
1) Identify Ko / Ko at production:produced in association with K+/K-
2) Identify Ko / Ko at decay:observe leptonic decay
CPLEAR T invariance testCPLEAR T invariance test
Initial state at t = 0
KK
KKpp
0
0
S = 0 S = 0)su(K
)su(K
Get positron: Or electron:
Experiment at LEAR ring
at CERN 1990-1996
Pions from kaon decay
Discovery of T violationDiscovery of T violation Currently the only direct observation of T violationCurrently the only direct observation of T violation
Measure asymmetry in rates
3106.16.6 TA
CPLEAR,1998
)()(
)()(0000
0000
KKRKKR
KKRKKRAT
Number of lifetimes
•T, or equivalently CP, violated by this tiny amount
CP Violation:CP Violation:Why is it interesting ?Why is it interesting ?
Fundamental:Fundamental: The Alien test The Alien test C violation does not distinguish between matter/anti-matter
Left-handed / right-handed are simply conventions
We cannot define what we mean by Co60 e- emission asymmetry unless we can define difference from anti-Co60 (or charge)
CP violaton says preferred decay KLe+ve-
Never shake hands with an alien whose `electrons’ are the preferred decay state of the long lived kaon!
Hence, it allows us to unambiguously distinguish between matter and anti-matter.
Least UnderstoodLeast Understood: CP Violation is ‘add-on’ in SM: CP Violation is ‘add-on’ in SM Parity violation naturally imbedded from coupling structure
Left-handed and right-handed couplings There is a matrix (CKM matrix) that tells us how likely transitions are from one
quark generation to another e.g. b quark to decay to a c quark or a u quark. CP violation can be accommodated in this matrix by adding a complex phase.
It is an ‘add-on’ justified only by the observation of CP violation.
CP: Why ? CP: Why ? Powerful: Powerful: delicately broken symmetrydelicately broken symmetry
Very sensitive to New Physics models Historical: Predicted 3rd generation !
Baryogenesis: Baryogenesis: there is more matter !there is more matter ! N(antibaryon) << N(baryon) << N(photons) N(antibaryon) << N(baryon) << N(photons)
Fortunately! 1 : 109
Sakharov (1968) Conditions for matter dominated universeSakharov (1968) Conditions for matter dominated universe Baryon number violation CP violation Not in thermal equilibrium
Assuming not initial conditions, but dynamic.Cannot allow all inverse
reactions to have happened
CP Violation key datesCP Violation key dates
19641964 CP Violation CP Violation discovery in Kaonsdiscovery in Kaons
19731973 KM predict 3 or more KM predict 3 or more familiesfamilies
… ….... … …..erm…not…much…..erm…not…much… …….. 19991999 Direct CP Violation Direct CP Violation
NA48/KTeVNA48/KTeV 20012001 BaBar/Belle CP BaBar/Belle CP
Violation in B mesonsViolation in B mesons
200?200? LHCb physics LHCb physics beyond the SM?beyond the SM?
Are we just the left over matter after CP violating matter/ anti-matter annihilation processes?