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Chiral DynamicsChiral DynamicsHowHowss and Why and Whyss
2nd lecture: Goldstone bosons
Martin Mojžiš, Comenius University23rd Students’ Workshop, Bosen, 3-8.IX.2006
a brief history of strong interactions
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
|exp T| S 4int i}xdH{-iffi
pre-QCD
< < ff | | ...HHintint... | i >| i >
| f , i >| f , i >known hadronic states
HHint int
unknown Hamiltonian(in terms of hadrons)
QCD
< < ff | | ...HHintint... | i >| i >
HHintint
known Hamiltonian
| f , i >| f , i >unknown hadronic states
(in terms of quarks)
ChPT
< < ff | | ...HHintint... | i >| i >
| f , i >| f , i >known hadronic states
HHintint
effective Hamiltonian(in terms of hadrons)
from the QCD to the ChPT
• the ChPT not derived, but constructed
• the procedure based on the symmetries
ChPT shares all the symmetries of QCD
• the symmetries were identified in the pre-QCD period
• then incorporated into and understood within the QCD
• the most prominent: the chiral symmetry
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
SU(2) isospin symmetry
... qMDiqQCDL
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U )2(
)1()2()2( USUU
the symmetry
Why linear and unitary? So it happened.
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
Nothing to do with the superposition principle or probability conservation.
classical conservation laws
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
(Noether’s theorem)
)( )()( xxx
symmetry conservation law current or charge
δ = 0 μ jμ(x) = 0 jμ = δφ /(μφ )
δ = ε μ μ(x) μ jμ(x) = 0 jμ = δφ /(μφ ) – μ
δL = 0 dt Q(t) = 0 Q = d3x δφ /(0φ )
δL = ε dt (t) dt Q(t) = 0 Q = d3x δφ /(0φ ) –
δS = 0 μ Iμ(x) = 0 Iμ not known explicitly
the generators
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• linear field transformation φi Tij φj
• infinitesimal transformation φi φi – i εa (ta)ij φj
δaφi = – i (ta)ij φj
• Lie algebra [ta ,tb] = i fabc tc
• SU(2) as a special case ta = ½ τa (Pauli matrices)
• conserved charges Qa = – i d3x 0φi (τa)ij φj
the generators – another incarnation
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• quantization: linear operators φi H Qa
• quantum conservation laws [H , Qa] = 0
[Pμ , Qa] = 0
• Qk’s form the Lie algebra [Qa , Qb] = i fabc Qc
• realization of the original symmetry in the Fock space
• in the QCD the knowledge of Qk is not sufficient for the knowledge of hadronic states transformations
transformations of states
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• Qa known explicitly in terms of quark fields
• |h(adron) not known explicitly in terms of quark fields
• Qa | h explicitly unknown, with the same energy
• eiαaQa representation of the symmetry group
• eiαaQa | h multiplet of states with the same energy
• observed in the hadronic spectrum
questions and comments
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• why to bother with charges if they are of no explicit use?we are going to see some use of them shortly
• what about SU(3)?the same story with Pauli matrices Gell-Mann ones
• what was the historical development?patterns in hadronic masses approximate symmetriesLie groups with pertinent irreducible representationswere postulated as the symmetries of strong interactions
SU(2) SU(2) chiral symmetry
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the symmetry
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
)1 ( 521
, LR
L
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chirality
the generators
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• formally: isospin + L,R tLa, tR
a
• the Lie algebra [tLa ,tL
b] = i f abc tL
c
[tRa ,tR
b] = i f abctRc
[tLa ,tR
b] = 0
• useful combinations tVa =tR
a+tLa tA
a=tRa –tL
a
• the Lie algebra [tVa ,tV
b] = i f abc tV
c
[tAa ,tA
b] = i f abctVc
[tVa ,tA
b] = i f abc tA
c
the generators – another incarnation
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• charges QVa , QV , QA
a , QA
• conservation laws [H , Q] = 0 , [Pμ , Q] = 0
• the Lie algebra [QVa
, , QVb] = i f abc
QVc etc.
• realization of the original symmetry in the Fock space
• again, the knowledge of charges is not sufficient
for the knowledge of hadronic states transformations
transformations of states
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• even without the explicit knowledge of Qa | h
quite a lot can be said about the hadronic multiplets• to each isospin multiplet there should be
a mirror multiplet with same masses and opposite parity• no trace of this in the particle spectrum!• could be that axial generators just annihilate | h states?
NO! [QAa
,QAb] = i f abcQV
c
isospin generators would also annihilate those states
spontaneous symmetry breakdown
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• Nambu (60’s)• if Qa | h = 0 does not help
what about trying Qa | 0 0 (SSB)• Goldstone (prior to Nambu): this leads to the
existence of spinless massless particles in the theory (with the precisely given quantum numbers)
• this is (in a sense) observed in the hadronic spectrum• the spectrum does not overrule the chiral symmetry it
rather supports the symmetry (in the SSB form)
questions and comments
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• are there really any massless hadrons?pions are almost massless, with right quantum numbersthe mass splitting within the flavor multiplets tells us that for strong interactions 150 MeV is a small number so the pions are close enough to masslessness
• what are the axial generators doing with states?they should in a sense create the Goldstone bosonsbut we are not able to write this down explicitlyreason: not only | h but also | 0 became complicated
even some more
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• what about U(1)V and U(1)A?
U(1)V happens to be the baryon number symmetry (easy)
U(1)A happens not to survive in quantum worlds (difficult)
• what is the precise formulation of the Goldstone theorem?if for a Noether charge Q there is an operator A for which 0|[Q,A]|0 0 then there is a massless state |G
for which 0|j0|G G|A|0 0
• a simple choice of A leads to 0|[Q,A]|0 = 0|qq|0 famous condensate (here it pays off to know Q explicitly)
(almost) do it yourself ChPT
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• we have identified the symmetries of the QCDas well as the lightest particles
• low-energy effective theory should start as a theory of fields of these particles sharing all the symmetries with the QCD
• one should start with the transformation properties of these fields and to construct the invariant ChPT
• the transformation properties of Goldstone boson fields are not known explicitly!
transformations of fields
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• so far we have considered either transformations of fields or of states
• both were linear, for different reasons• for the states the reason is the superposition principle• for the quantum fields: creation operators transformed
to linear combinations of the creation operatorsi.e. transformations do not change number of particles
• this is inconvenient for the axial generators Qa
they should change the number of Goldstone bosons
how do the GB fields transform?
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• according to a non-linear realization of the group• as to the unbroken isospin subgroup
the pion triplet behaves quite ordinary• so for the unbroken isospin subgroup
the realization should become a linear representation • there is an infinite number of such realizations
becoming representation when restricted to the subgroup• which one is the one?
which choice is the right one?
23rd Students’ Workshop, Bosen, 3-8.IX.2006 Martin Mojžiš, Comenius University
• any will do!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
• they are all equivalent as to the S-matrix elements• the off-shell Green functions do depend on a choice
but the measurable quantities do not• choose the most convenient realization of the symmetry
start to build up the most general invariant Lagrangian• this is going to be the topic of the 3rd lecture