A NNALES DE L ’I. H. P., SECTION A
R ICHARD K ERNER
Approximate mass formula for mesons : a model with quarks interacting by means of the Yang-Mills field
Annales de l’I. H. P., section A, tome 23, n
o4 (1975), p. 379-388
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379
Approximate
massformula for
mesons:a
model with quarks interacting by
meansof the Yang-Mills field
Richard KERNER
Departement de Mecanique, Laboratoire de Mecanique relativiste, Université de Paris VI, Tour 56-66, 4, place Jussieu, Paris-5e, France
Ann. Inst. Henri Poincaré, Vol. XXIII, n° 4, 1975,
Section A : Physique théorique.
1. INTRODUCTION.
NOTATIONS AND PRELIMINARIES
Since the introduction of
quarks
intoelementary particle physics by Gell-Mann, Ne’eman, Zweig,
Okubo andothers,
a lot of models had been tried with more of less success. Most of these models do not dealexplicitly
with any
precise
form of interaction between thequarks constituting
anelementary particle :
the essence of thetheory
lies in thealgebraic symmetry properties
of theseinteractions,
which lead inelegant
andsimple
way to the massformulæ,
as well as to thealgebraic
relations between the cross-sections of the different
scattering
processes.In the model
proposed
below wetry
to describe asystem composed
of two
quarks interacting by
means of theYang-Mills
field. In order tobe honest we have to say
already
that we don’tyet
know how to handle in a similar way asystem composed
of threequarks,
so that theresulting
mass formulae will
apply
to the mesonsonly.
Theplausibility
ofusing
the
Yang-Mills
fields fordescribing
an intermediate boson has been dis- cussed in many papers, and it does not seem worthwhile tojustify
it hereonce more.
The
objection
one could make that theYang-Mills
fields are inprinciple
massless and therefore do describe a
long-range
force isserious,
but it hadbeen also shown that one can introduce a mass, term, and then reestablish thus broken
symmetry (Higgs-Kibble, Veltman, t’Hooft),
at least in someorder of
approximation.
Annales de l’lnstitut Henri Poincare - Section A - Vol. XXIII, n° 4 - 1975.
Our
example, though
on thequantum
mechanical levelonly,
followsa similar line of
thought.
In the Hamiltoniandescribing
oursystem
we will first add anarbitrary mass-splitting
term, thereforebreaking
the gaugesymmetry.
Then weperform
ageneralized Foldy-Wouthuysen
transfor-mation in order to
diagonalize
the Hamiltonian in the first few orders ofapproximation.
The masssplitting
is stillpresent
in the final result.Its
general
form is the same as in the Gell-Mann-Okubo mass formula forSU(3),
but the coefficients can be inprinciple
deducedby feeding
insome
particular
form of theYang-Mills
fieldpotential.
For the sake ofsimplicity,
ourYang-Mills
field will begenerated by
the groupsSU(2)
orSU(3).
Our notations will be the
following :
The Minkowskian
space-time: M4, x E M4 :
x = J1, V =0, 1, 2, 3,
or x =
(xo, x) = (xo, x’),
withi, j,
... =1, 2,
3The gauge group,
supposed
to becompact
andsemi-simple : G,
dim G =N;
a, b, ...=1,2,
... N.C~ = - C b
are the structure constants of the group G.The basis of the Lie
algebra
of G :Q~ verifying :
The
Yang-Mills
fieldpotential
will be denotedby :
The
Yang-Mills
field tensor has the formand the field
equations
are :and
where
and
J~
is the conserved external current, null in the vacuum.Dirac’s
equation
reads as follows :Annales de l’Institut Henri Poincaré - Section A
381
APPROXIMATE MASS FORMULA FOR MESONS
with :
and the matrices
~3,
oc,verify
E~ meaning
the matrixbeing
the usual 2 x 2Pauli matrices;
- -
’
,
in what
follows,
we shall use the notation -; instead of ~ where there is no risk ofconfusion;
Idstays
for the 4 x 4identity
matrix.The
equation (9)
isnaturally generalized
for the case of theYang-Mills
field interaction. It becomes :
The whole difference is that now the
generalized charges Qa
do not com-mute
(2) ;
we suppose,however,
thatthey
commutewith {3
and a I. In otherwords,
our wavefunction ~ belongs
now to aproduct
space,where every
component
is a4-spinor.
The matrices/~
(ihQa
are thereforein a
product representation
and arecomposed by
4 x 4blocks;
the dimensionis 4N :
Qa
are thematrices z i of
theSU(2)
group orthe Àa
of theSU(3),
with eachunity replaced by
a 4 x 4identity
matrix.Our basic
equations (8), ( 11 ) being
nowdefined,
we canproceed
to thenext
problem,
which is todiagonalize
the Hamiltonian.2. THE FOLDY-WOUTHUYSEN TRANSFORMATION
The
diagonalization
of the Hamiltonian(11)
can not beperformed exactly
at once, but we can
diagonalize
it in any order of11m by
means of theVol. XXIII, nO 4 - 1975.
Foldy-Wouthuysen procedure.
Theunitary .
transformation needed is of the form :, ,, B
where S is the some unknown hermitian matrix.
First we
try
todiagonalize
H in thespin
space, i. e. toget
rid of theexpression containing
thenon-diagonal
matrices ex. Let us callso that
Supposing
that the matrix S if of order1/~,
theexpression ( 14)
can be deve-loped
as follows :The
only
0-order term in11m
will be :and we want it to be
equal
to the 0-order oddpart :
This is obtainedby putting
Now our Hamiltonian will take on the form :
where the new odd term is of order
1/~. Performing
the nextunitary
trans-formation of the same
type,
withwe shall obtain :
with the odd
part
9" of order1/m2,
and so on.The result calculated up to the order
11m3
is as follows :Annales de l’lnstitut Henri Poincaré - Section A
383
APPROXIMATE MASS FORMULA FOR MESONS
where
by
definition:However,
our Hamiltonian still contains theblock-non-diagonal
matricesQa,
and we have to
perform
a similar transformation in order todiagonalize
it
completely.
The case when G =SU(2)
andQa
are the three 1" is resolvedvery
easily.
We add to our Hamiltonian the termThen,
because of the relationswe can
perform
the same kind of thetransformation,
the matrix Sbeing
now
equal
towhere:; means now the sum of all terms of H
containing
thenon-diagonal matrices Tl
and z2. In order to make ourapproximation valid,
we haveto assume M of the same order of
magnitude
that m. Theresult,
up to the order1/M3 (or I/Mm2, 1/mM2, etc.)
is as follows:and after
developping 82 explicitly
becomesThe last formula becomes even more
interesting
when we feed in somesimple
static solution of theYang-Mills
fieldequations.
The Coulomb- likepotential gives:
with 0" =
BQ =
0.The solution
corresponding
to thegeneralized magnetic monopole
Vol. XXIII, no 4 - 1975.
gives :
and the
magnetic spin-monopole (see
e. g.[4], [5]),
withyields
the formula:Here the mass
splitting depends
on thedirection;
this proves that thespin- monopole potential
isunphysical.
Besides added at the
beginning
of thediagonalization procedure,
the mass
splitting persists
withrespect
to theeigenvalues
of theoperator z2,
i. e.
1(1
+1 )
and theeigenvalue
of theoperator
!3, i. e.I~. However,
we arestill far from the Gell-Mann-Okubo
formula, which,
as weknow,
isquite
well verified. In order to obtain a formula of this
type,
we have togeneralize
our
procedure
for theSU(3)
group.3. DIAGONALIZATION OF THE
SU(3)
HAMILTONIAN Let us start with the Hamiltonianin which the
Qa’s
are thegenerators
of theSU(3)
Liealgebra.
In thesimplest
3 x 3
representation
we have(a, b,
...1, 2,
...8)
The idea of the
approximate diagonalizing procedure
isessentially
thesame. We shall first illustrate it
taking
theroughest approximation,
inwhich
Annales de l’Institut Henri Poirzcare - Section A
385
APPROXIMATE MASS FORMULA FOR MESONS
i. e.
conserving
the terms of order11m only.
Afterexpanding
the term(p - QaAa)2
we obtain:and the Hamiltonian becomes:
Now,
here we have twodiagonal operators Q3
andQs,
and sixnon-diagonal
ones,
Q 1, Q2,
...,Q7.
Let us introduce the indicesA, B,
...,taking
on thevalues
1, 2, 4, 5, 6,
7. Then we can write our Hamiltoniansymbolically
asHere 3 =
:1AQA
is the sum of all the termscontaining
thenon-diagona
matrices
QA,
and 8 =E3Q3
+88Q8
is thediagonal
term. Now we add to ourHamiltonian the
symmetry-breaking
terms :As
above, M3
andMg
should begreat enough
to ensuregood
convergence of theapproximation
series.Next we have to find a matrix S which shall
verify :
in order
toget
rid of thenon-diagonal part
up to the order1/m.
It is obviousthat in
(40)
the lowest-order term will beother terms
being
at least of order1/m.
The matrix S is therefore defined up to anarbitrary
termS3Q3
+SsQs commuting
withM3Q3
+We
put
this termequal
to zero, of course, and therefore can write S =So we
haveDeveloping
this commutator weget explicitly Defining
Vol. XXIII, no 4 - 1975.
we obtain
and therefore
if det B # 0.
The 6 x 6 matrix
BAC
has thefollowing
form:and its determinant is
equal
toThis determinant is different from zero if and
only
ifM3 #
0 andM 3
#3M~.
The last condition could be
postponed
if we assume that the fieldA~, Ba
has no
components
6 and7,
but this isequivalent
to thereducing
our sym-metry
group toSU(2)
xV(I)
which is notinteresting. Moreover,
one shouldkeep
in mind that the differenceM3 - B/3Mg cannot
be toosmall,
because if it was, the
development
in orders of(M3 - y3Ms) -1
whichoccurs afterwards is not valid.
Assuming
that these conditions areverified,
we canproceed
farther.We have to calculate the
expression
(supposing
forsimplicity
that0).
Theexpression (48)
will be of order11m2;
itsnon-diagonal part
can then be removedby
the next similarstep,
after which thenon-diagonal parts
will be of order2014 3 which we shall
drop
out.Therefore,
we can be interestedonly
in thediagonal components
of the(48).
It is easy to see that neither thefirst,
nor the second term do notyield
suchcomponents,
so we are leftonly
with two termsi[S, 8]
+i[S, G],
which
give explicitly :
(49) i[S, 8] = -
+.fABBQs)
+non-diagonal
termsand
(49 a) i[S, G]
=Q3]
+Qs]
= allnon-diagonal
Annales de l’Institut Henri Poincaré - Section A
387 APPROXIMATE MASS FORMULA FOR MESONS
The final calculus
depends
now on the kind of interaction we shall assume.In the case when
only
scalarpart
of thepotential
is different from zero, it is easy to see that the final formula will be of the formi. e. there will be
only
linearmass-splitting present.
In the case when there is
only
vectorpotential,
and theonly non-vanishing part
of scalarpotential
isQ3M3
+ theapproximated diagonalized
Hamiltonian will take on the form:
which can be written
symbolically
asThis is similar to the Gell-Mann-Okubo
formula,
with a,b,
cbeing
now somecomplicated
functions ofAa,
and J.DISCUSSION
In this very
simple-minded approach
we have chosen the external fieldapproximation
for the interaction betweenquarks.
Of course, this choice isquite arbitrary :
all thedynamics
is contained in thequarks themselves,
whereas the field of interaction has no
dynamics
of its own,being purely
kinematic in nature. But this kind of
arbitrary separation
ofdynamical
and kinematical features is all the way
present
in anytheory
ofinteractions,
and the actual difference between the
dynamical
and kinematicalquantities depends
on thephysical aspects
of thesystem
described andmostly
on theintuition.
Moreover,
thediagonalization technique
used here is basedessentially
on the non-relativistic
approximation,
which we are not at all sure is valid for thedescription
of the interaction between thequarks.
Butthen,
the fact that the meson massesobey
the sum rules deduced from the linear represen- tations ofSU(3)
group are no lessmysterious,
because should theelementary particles
becomposed
ofquarks,
theunderlying dynamics
would have to behighly
non-linear. It seemsinteresting
to obtain here notonly
theright
Vol. XXIII, no 4 - 1975.
qualitative
mass formula(52),
of the same kind that the Gell-Mann-Okubo one, but also thespin dependence
for the coefficients.This kind of formula would be
impossible
to obtain for thetotally SU(3)-symmetric
Hamiltonian : it is obvious that without thesymmetry- breaking
termM3Q3
+MsQs
anyunitary
transformationperformed
onHo
would
yield
nomass-splitting
at all.Therefore,
what we havedemonstrated,
is thefollowing:
if for any reason the Hamiltoniandescribing
twoquarks interacting by
means of theYang-Mills
field contains a linearsymmetry- breaking
term(this
initialassymetry being
due e. g. to the mass-difference betweennon-interacting quarks),
then in theapproximation given by
the
Foldy-Wuthoysen diagonalization procedure
we obtain the formula(52).
The
approximation
is thebetter,
the heavier are the assumed « naked »masses of the
quarks
and their differences. Anotherpossible interpretation
is to assume that the term
M3Q3
+MsQs
describes in the linearapproxi-
mation the mass of the intermediate boson.
We think that the same kind of
calculus,
however much morecomplicated,
can be
performed
for thebaryons
constitued of threequarks,
in which casewe should derive the
gauge-invariant
Hamiltonian from the Faddeevequations,
or theBethe-Salpeter equation.
ACKNOWLEDGMENT
The author expresses many thanks to Prof. M. Flato for
enlightening
discussions and remarks.
REFERENCES
[1] C. N. YANG and R. L. MILLS, Phys. Rev., t. 96, 1954, p. 191.
[2] BJORKEN and DRELL, Relativistic Quantum Mechanics, McGraw-Hill, New York, 1964.
[3] R. KERNER, Ann. Inst. H. Poincaré, vol. IX, n° 2, 1968.
[4] R. KERNER, Comptes Rendus Acad. Sci. Paris, t. 270, 1970, p. 1467.
[5] A. JOSEPH, Phys. Rev., t. 5, 1972, p. 313.
[6] P. A. M. DIRAC, Phys. Rev., t. 74, 1948, p. 817.
[7] B. FELD, Models of Elementary Particles, Blaisdell Publishing Company, 1969.
[8] M. GELL-MANN, Phys. Letters, t. 8, 1964, p. 214.
[9] G. MORPURGO, Physics, t. 2, 1965, p. 95.
[10] O. W. GREENBERG, Phys. Rev. Letters, t. 13, 1964, p. 598.
[11] Y. NE’EMAN, Algebraic Theory of Strong Interactions, Benjamin, New York, 1968.
Annales de l’Institut Henri Poincaré - Section A