This article is meant as an introduction to the field of meson spectroscopy, it is not intended to be a comprehensive review of the subject. I have divided this article into four parts. Initially, I will identify what mesons are, and how we classify them. In particular, their nonet structure and how we can use mass, width and decay patterns to assign them. Next, I will review partial wave analyses, and how we use this information to extract the quantum numbers of the mesons. I will then discuss what the current issues in meson spectroscopy are, and how these issues can help us understand non-perturbative QCD. Finally, I will discuss the issues which we can address using an upgraded CEBAF with 10 to 12 GeV photons.
A
system can have the two spin
quarks in
either a spin singlet, S=0, or a spin triplet, S=1 state. In
addition, there is a relative orbital angular momentum L between
the
pair and a total spin J of the system. Finally,
there are radial excitations, n, of the
system.
A particular nonet is then described in spectroscopic notation as
n2s+1LJ. In this notation, the pseudo-scalar mesons, (
,
K,
and
), are 11S0 mesons, and the
vectors, (
,
K*,
and
), 13S1 mesons.
Because most of the processes of interest are purely strong
interactions, we denote the mesons in terms of the conserved quantum
numbers, (IG)JPC: isospin ,I; G-parity, G;
total spin, J; parity, P; and C-parity, C, . For a
system, P=-(-1)(L),
C=(-1)(L+S) and
G=(-1)(L+S+I). A nice description is given in
reference [1].
This leads to the expected spectrum of nonets shown schematically in Figure 1. The states labeled in black are reasonably well established, while those labeled in gray either need confirmation, or the assignment is not certain. The empty boxes indicate states which are not known. The mass listed below each box are taken from reference [2]. They are the estimated mass of the states containing mostly u and d quarks.
In order to uniquely identify that a state belongs to a
particular nonet, it is necessary to look at several properties
of the state. Table 1 lists the tensor mesons, JPC=2++
along with their masses, widths, and known two pseudo-scalar
decay modes. Given a series of mesons which we believe belong to
the same nonet, we can use the mass relation in equation 1
to arrive at a mixing angle for the nonet.
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Depending on the beam and mechanism, different types of mesons
are more likely to be produced. Kaon beams are a good way to produce
both the excited Kaons, as well as the mostly
mesons. Certain
reactions such as
decays,
annihilations and
double pomeron exchange are considered to be glue-rich. Other
reactions such as
and e+e- are felt to
be glue-poor environments.
annihilations at rest
favor production of scalar mesons, and
states tend to
be weakly produced. The bottom line is that looking at the different
production mechanisms of a meson can also yield information on
its constituents.
In the case of either
decay or
annihilation at
rest the analyses are quite similar. The system starts in a well
defined state, ( (IG)JPC are known). If we then consider
a process such as
,
we assume that this
can be described in terms of the isobar model [4],
which leads to the chain shown in eqn. 2.
In the case of a three-body final state, the analysis is normally
carried out in the framework of a Dalitz plot. Figure 3
shows the Dalitz plot for the process
at rest, (these data are
taken from reference [7]). The prominent diagonal band is
the
recoiling against a spectator
.
There is
also a horizontal band corresponding to the
against a spectator
and a vertical band corresponding to
the
a2-(1320) recoiling against a spectator
.
The data are fit identifying a complex amplitude,
,
for each possible resonance. Those
from the same initial state are added coherently, and then squared
to yield an estimated weight for each bin in the Dalitz plot. The
parameters of the complex amplitudes, as well as their relative strengths
and phases are varied to minimize a
difference between
the data and the fit.
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Only fitting with the amplitudes listed above yields a
per
degree of freedom of 2.69. The difference between the fit and the data
are shown in . The structure in this plot
indicates that there is something missing in the fit. Adding a resonance
in the
P-wave to the mix reduces the
per degree of
freedom down to 1.29 and produces the difference plots shown in
. The differences are now essentially
statistical in nature.
In the case of either the diffractive production or the t-channel exchange,
the partial wave analysis is done in a somewhat different way. The underlying
assumption here is that the amplitudes can be broken in to two or more
incoherent sets. These essentially correspond to spin-flip and spin-non-flip
amplitudes [8]. In these procedures, only the X system of
Figure 2 is treated. The data are binned according to the
mass of X, and with a series of functions which only describes the angular
distributions of the final state particles are fit two each bin. From these
fits, one extracts the intensity and phase of each partial wave as a function
of mass. Figure 4 shows the results from one of these fits
taken from reference [9]. Figure 4a shows mX,
in this case
.
Figures 4b and
c show the fit intensity in the 1++ and 2-+ partial waves.
These results are then fit two the assumption of resonances in the
partial waves. Here explaining the relative phase differences is key
to extracting the resonance parameters.
Finally, when fitting the resonance parameters, it is important to cite the T-matrix poles rather than the simple Breit-Wigner masses and widths. The latter can be severely distorted by the production method, decay thresholds, and other resonances, while the former have all these effects built in and are a better representation of the actual resonance.
Even in the few situations where we have identified a number of states, the identification of a particular state is often hindered by its observation in only one production mechanism, and only a very small number of decay modes. As an example, we will consider the 2++ and J- states.
Of all the higher mass mesons, there are more known 2++ states
than anything else. In Figure 5 are listed the known 2++
mesons from reference [13]. The bars indicate the expected location of
the first radial states, the 3F2 states and the glueball. Also indicated
are some of the 3F4 states which are expected to have similar masses
to the 3F2 states. The f2 states have the same quantum numbers
as the expected 2++ glueball. Finally, we give the known decay modes
from largest to smallest. Even with all these states, there are difficulties
in assigning them. In my opinion, the f2(1565) and f2(1640) are
probably the same state, just seen in different production mechanisms. One
would then like to assign the f2(1810) as the radial excitation of
the
.
Unfortunately the
mode is probably
too small. The f2(1950) is also a candidate for this state, but there
is also speculation that this broad state has a large glueball
content [14]. The fJ(2220) or
is also
a glueball candidate because of its very narrow width, and large rate in
radiative
decays [15]. Finally, there are several higher
mass states that have only been observed in one or two decay modes. In order
to untangle what is going on we need to know more about the decay patterns
of these states. In particular, unraveling the
modes such as:
Next we examine the J- mesons. Figure 6 shows the currently
known states, as well as expected missing states, (inside the box). In addition
to the meson states, a JPC=1- hybrid nonet is expected around a
mass of 1800 MeV/c2. Given the proximity of the 3D1
and both 23S1 and 33S1 states, strong mixing cannot be
excluded. Also, recent observations of the
and
indicate that they have large rates to the ground state vector plus
[17], [18]. This leads one to speculate
that a similar decay should be present for the
.
These decays
do not appear important for the
and the
.
It
is these latter states which people speculate are strongly mixed with the
hybrid nonet. Unfortunately, only detailed studies of the decay patters
will allow us to unravel this. Reference [16] calculates
the various rates for both the 3D1 and hybrid
.
Detailed
comparison with currently emerging results may yield new insights on this
problem. The bottom line is that we do not understand these states
particularly well.
Our understanding of non-perturbative QCD could be significantly advanced
by being able to experimentally identify the orbital and radial excitations
of mesons, and their likely mixings. More significantly, finding the expected
gluonic states, (hybrids and glueballs) and understanding their mixings with
the normal
states would expand our understanding of just how glue
behaves. Several talks at this workshop have addressed the role of
photo production that could be exploited at CEBAF. Reference [20]
discusses the
spectrum, which takes advantage of the fact that
there is a significant
content in the photon.
Reference [19] discusses why photo production is expected to
be a good place to find hybrid mesons, and which ones would be
most easily seen. Finally, reference [10] discusses the
Hall D project to build a state of the art detector whose
main goal would be to study meson spectroscopy.