We present a measurement of the production polarization of
mesons
produced in
collisions at
with the CDF detector at Fermilab.
This measurement is a sensitive test of
the Color Octet Model (COM) suggested as the
explanation for the unexpectedly large cross section for charmonium
production in
collisions
(roughly a factor 50 above the Color Singlet Model).
A prediction of the COM is that directly produced charmonia should
approach 100
transverse polarization
for high transverse momentum of the onium state.
We consider
mesons, reconstructed using the decay mode
in a
110 pb
data sample of
collisions.
The polarization of
prompt
is extracted to be
for
GeV/
.
Measurements of both direct
and
cross sections
by CDF [1] are
times higher than Color Singlet Model predictions
[2].
By ``direct'', we mean the charmonia produced directly from the
collisions, and not those from particle decays
such as
,
, etc.
One of the theoretical models which tries to explain this anomalous
production is the Color Octet Model (COM) [3].
The model raises the direct production cross section by including
color-octet
states in the fragmentation process. At
leading order in
and at high
(
,
where
is the charm quark mass), the
contribution to the cross section is dominated by gluon fragmentation
into the color octet
states. The fragmenting
gluon, being effectively on-shell at high
, is transversely
polarized. The
pair and subsequently
the
and
mesons
inherit the gluon's transverse polarization. Therefore, COM
predicts the direct
and the
to approach 100
transverse polarization at high
[4].
Observation of such a polarization
would support the color-octet fragmentation mechanism.
![]()
Experimentally, the
is a clean channel to test the COM.
The displacement of the
vertex from the primary
can be used to distinguish prompt (direct) production from B decays.
In the case of the
, the prompt production is contaminated with
feed-down like
.
![]()
Using spin formalism [5], the angular distribution
in
decay
is derived to be:
![]()
where
is the polarization and
denotes the angle
between the
momentum in the
rest frame
and the
momentum in the Lab frame.
Unpolarized
mesons would have
whereas
and -1
correspond to fully transverse and longitudinal polarizations
respectively.
The value of
is extracted from the data by fitting the
reconstructed angular distribution after acceptance corrections.
This analysis is based on a 110 pb
sample of low
dimuon
triggers collected by CDF during 1992-95. Both muons are required to
pass standard quality cuts and to be reconstructed in the silicon
vertex detector (SVX). In addition, they are required to have
larger than 2.0 GeV/
(in the Run 1A sample, the high
muon is
required to have
larger than 2.8 GeV/
). The selected
dimuons are vertex constrained to form the
candidates.
A
cut larger than 5.5 GeV/
is imposed on the
candidates. The
reconstructed dimuon mass distribution after the selection cuts is
shown in
Figure 1.
It is fitted
with a gaussian plus linear background. We find
signal
candidates. In a
mass window
around the
mass, the signal to background ratio (S/B) is
.
To study the
dependence of the polarization, we divide the
data sample into three
ranges (5.5-7, 7-9 and 9-20
GeV/
).
Each sample is further divided
into two sub-samples based on the
distribution.
ct is related to the transverse decay length
as follows:
![]()
where m is the reconstructed
mass.
The factor
is an average correction factor
obtained from Monte Carlo
studies to account for the fact that we use
instead of
.
The low ct region (-0.1<ct<0.01 cm) is prompt enriched
whereas the high ct region (ct>0.01 cm) is dominated by B decays.
![]()
The value of
for each candidate is calculated from the
momentum vectors of the
muons, and the mass and momentum of the reconstructed
.
Since the angular distribution is symmetric, the absolute value of
is used, and subdivided into 10 bins.
The mass distribution in each
bin is fit with a gaussian
and linear background to determine the number of observed signal
events. The values of the mean and width of the gaussian signal
function are constrained as the event yield at large
is
low. It is well known that the mass resolution depends on
. Due
to the kinematic correlation between
and
, the
mass width is also expected to have
dependence.
Figure 2
shows the mass width of the
Monte Carlo versus
in the three different
ranges.
In the
range
where the bin size is large, the mass
width is seen to rise
towards higher
bins. This distribution is then used
to parameterize the kinematic width variation in the mass fits.
The resultant fits to the mass distributions for
in the
low ct region are shown in
Figure 3,
Figure 4 and
Figure 5
for the three
ranges of
.
The
mass fits in the high ct region for the three
ranges are shown in
Figure 6,
Figure 7 and
Figure 8
respectively. The signal event yield from the mass fits then form the
distributions.
![]()
Monte Carlo events are used to obtain a parameterization of the acceptance.
events are generated with flat angular
distributions, and a
distribution given by
, where C, M and N are
obtained by fitting the parameterization to the Run 1A
differential cross
sections [1].
Figure 9
shows the fits to the
differential cross sections of the promptly produced
, and of
those arising from B meson decays.
mesons are decayed to dimuons
and simulated through the detector. The resulting prompt and
B decay acceptances as a function of
are shown in
Figure 10 and
Figure 11 respectively.
In Figure 12,
the prompt acceptance is separated into
three
subranges. One sees that the acceptance extends to higher
values of
as the
of the
increases.
Comparisons of the
distributions between the data and
the Monte Carlo are shown in
Figure 13 and
Figure 14
for prompt and B decay. We see they have good agreement.
![]()
We fit the ct distribution of the
mesons
to get the relative fractions of prompt and B decay in
different ct bins. This is based on an unbinned likelihood fit
[6]. The
distributions overlaid with fit
results for the three
ranges are shown in
Figure 15,
Figure 16 and
Figure 17
for events in the mass signal region, and in
Figure 18,
Figure 19 and
Figure 20
for events in the sidebands. In the figures,
is the fitted B
fraction;
is the
purity (including both prompt and
B) in the mass signal region.
Figure 21
shows the relative purity for the prompt and B decay components as a
function of ct. The two curves cross each other near ct =
0.01 cm. This motivates us to divide the ct distribution into two
regions with a
low ct region dominated by the prompt component and a
high ct region dominated by the B component.
![]()
The prompt and B decay production polarizations are extracted from the
distributions of the data by simultaneously fitting the
two ct regions using a binned
fitter.
The prompt fractions,
and
for the low and high ct
regions, and the
polarizations for prompt and B decay production are summarized in the
following table:

Figure 22
shows the
distributions in
the low ct region with their polarization fits overlaid. The same fits
for the high ct region are shown in
Figure 23.
We study two categories of systematic uncertainties. One is the
event yield uncertainty resulted from the mass fits in the
bins. The other is the uncertainty on the
acceptance due to
the modeling of the
distribution. They are summarized in
the table below:

Using a sample of
events
reconstructed with the CDF detector, we present a preliminary
measurement of the
polarization from prompt production,
as well as from B decays.
The results of the three
subranges and the integrated
range are as follows:

In Figure 24,
the prompt
polarization is plotted
versus
. Also shown is a theoretical calculation based on the
Color Octet Model [4].
The measurement has large statistical uncertainties, but it appears to
not support the Color Octet Model predication
that the
is transversely polarized at high
.
Figure 25 shows
the
polarization from B decay versus
.