J. BELZ[(a)],
R.D. COUSINS
,
M.V. DIWAN
[(b)],
M. ECKHAUSE
,
K.M. ECKLUND
[(c)],
A.D. HANCOCK
,
V.L. HIGHLAND
[(d)],
C. HOFF
,
G.W. HOFFMANN
,
G.M. IRWIN
,
J.R. KANE
,
S.H. KETTELL
[(b)],
J.R. KLEIN
[(e)],
Y. KUANG
,
K. LANG
,
R. MARTIN
,
M. MAY
,
J. McDONOUGH
[(e)],
W.R. MOLZON
,
P.J. RILEY
,
J.L. RITCHIE
,
A.J. SCHWARTZ
,
A. TRANDAFIR
,
B. WARE
[(f)],
R.E. WELSH
,
S.N. WHITE
,
M.T. WITKOWSKI
[(g)],
S.G. WOJCICKI
,
and S. WORM
[(h)]
(BNL E888 Collaboration)
(1) Brookhaven National Laboratory, Upton, NY 11973
(2) University of California, Irvine, California 92717
(3) University of California, Los Angeles, California 90024
(4) Princeton University, Princeton, NJ 08544
(5) Stanford University, Stanford, California 94309
(6) Temple University, Philadelphia, Pennsylvania 19122
(7) University of Texas at Austin, Austin, Texas 78712
(8) College of William and Mary, Williamsburg, Virginia 23187
We have searched for a neutral H dibaryon decaying
via and
.
Our search has yielded two candidate events from which we set
an upper limit on the H production cross section. Normalizing
to the inclusive
production cross section, we find
at 90% C.L., for an H of mass
2.15 GeV/
.
The theory of quantum chromodynamics imposes no specific limitation
on the number of quarks composing hadrons other than that they form
color singlet states. Although only qqq and states
have been observed, other combinations can form color singlets.
Jaffe[1] has proposed that a six-quark state
uuddss may have sufficient color-magnetic binding
to be stable against strong decay. Such a state, which Jaffe
named H, would decay weakly, and the resultant long lifetime
would allow the possibility of observing such particles in
neutral beams. Theoretical estimates[2] of
have varied widely, ranging from a deeply bound state
with
<2.10 GeV/
to a slightly unbound state with
near the
threshold, 2.23 GeV/
.
In this mass range the H would decay almost exclusively to
,
, and
[3].
Several previous experiments have searched for H's but with no
compelling success[4]. The search described here
is sensitive to H's having mass and lifetime in a previously
unexplored range.
We have searched for and
decays
by looking in a neutral beam for
decays in which the
momentum vector does
not point back to the production target.
The experiment, E888, was performed in the B5 beamline
of the Alternating Gradient Synchotron (AGS) of Brookhaven
National Laboratory. A second phase of the experiment searched
for long-lived H's by using a diffractive dissociation
technique[5].
The detector used for the decay search (Fig. 1)
was essentially that used for the E791 rare kaon decay experiment
and has been described in detail elsewhere[6].
Figure 1: The E888 detector and beamline.
In brief,
a neutral beam was produced using the 24 GeV/c proton beam
from the AGS incident on a 1.4 interaction length Cu target.
The targeting angle was 48 mr. After passing through a series of
collimators and two successive sweeping magnets, the neutral
beam entered a 10 m long vacuum decay tank within which
candidate 's decayed. Downstream of the tank was a
two arm spectrometer consisting of two magnets with
approximately equal and opposite
impulses
and 5 drift chamber (DC) stations located before,
after, and in between the magnets.
Downstream of the spectrometer on each side of the beam were a pair
of trigger scintillator hodoscopes (TSCs), a threshold Cherenkov
counter (CER), a lead-glass array (PbG), 0.91 m of iron to filter
out hadrons, a muon-detecting hodoscope (MHO), and a muon
rangefinder (MRG) consisting of marble and aluminum slabs
interspersed with streamer tubes.
For the first half of the run the Cherenkov counters were
filled with a He-N mixture (n = 1.000114) to identify electrons;
for the second half the left-side counter was filled with
freon (n = 1.0011) to identify protons from
(due to lack of light).
Only the left counter was used for this purpose as the soft pion
from
decay is accepted only when on
the right; when it is on the left, the first magnet bends it
back across the beamline and it is not reconstructed. The lead-glass
array (PbG) consisted of two layers: a layer of front blocks 3.3
radiation lengths (r.l.) deep and a layer of back blocks 10.5 r.l.\
deep. The PbG was used to identify electrons by comparing the total
energy deposited (
) with the track's momentum.
A minimum bias trigger was defined as a coincidence between all
4 TSC counters and signals from the 3 most upstream DC stations.
A Level 1 trigger (L1) was formed by putting minimum bias triggers
in coincidence with veto signals from the Cherenkov counters and
muon hodoscope. All events passing L1 were passed to a Level 3
software trigger which used hit information from the first
3 DC stations to calculate an approximate two-body mass. Events with
<1.131 GeV/
were written to tape.
Offline, all events containing two opposite-sign tracks
forming a loose vertex were kinematically fit[6]
and subjected to the following cuts:
there could be at most one extra track-associated hit or one
missing hit in the ten DC planes which measure the x (bending)
view of each track; the 's per degree of freedom resulting
from the track and vertex fits had to be of good quality;
the
vertex had to be within the decay tank and
downstream of the fringe field of the last sweeper magnet;
both tracks had to be accepted by CER, PbG, MHO,
and MRG detectors and have p>1 GeV/c;
neither track could intersect significant material
such as the flange of the vacuum window;
to reject background from
,
had to be
;
and to reject background from
resulting
from secondary interactions,
had
to be >4 times the mass resolution of
decays (1.55 MeV/
).
Events passing these cuts were subjected to particle
identification criteria in order to reject background from
(
) and
(
) decays.
To reject electrons, we require that there be no
track-associated Cherenkov hit and
that tracks with p>2 GeV/c
(<2 GeV/c) have
(<0.52).
The low momentum track on the right side of the detector
was required to deposit <0.66
in the front PbG blocks.
To reject muons which passed the MHO veto in the trigger,
we cut events with a hit in the MRG which was consistent with the
projection of a track and which corresponded to at least 65% of
the expected range of a muon with that track's momentum.
Lambda candidates were selected by requiring that
be less than 4 times
the mass resolution of
decays
(0.55 MeV/
). The data was then divided into two streams:
a normalization stream consisting of
's which
project back to the production target, and a signal stream
consisting of
's which do not. The former were selected
by requiring that the square of the collinearity angle
be less than 1.5 mrad
, where
is the angle between the reconstructed
momentum vector and a line connecting the production target
with the decay vertex. This sample contains
negligible background. The signal sample was selected by requiring
that
>145 MeV/c, where
is the
momentum transverse to the line connecting the production target
with the decay vertex. This cut value was chosen to eliminate
decays, which have a kinematic
endpoint of 135 MeV/c. The
distribution of
's
from two-body
decays exhibit an
approximate Jacobian peak (not exact because the vertex is
the
's) with an endpoint which depends upon
. A large fraction of high-
's were
found to project back to a collimator located just upstream of
the decay tank. We thus required that the point in our beamline
to which a
projects back be located downstream of
this collimator:
m.
A signal region for H candidates was defined by the criteria
MeV/c and
, where
is
the distance in proper lifetimes between the decay vertex and
the nearest material (beamline element) to which the momentum
vector projects back. The
cut rejects
decays which survive the CER, PbG, MHO, and MRG vetoes due to
detector inefficiency, while the
cut rejects
's which originate from collimators, flanges, and
other beamline elements. All cuts were determined
without looking at events in the signal region, in order
that our final limit on H's be unbiased. After fixing cuts
we looked in the signal region and observed two events.
The estimated background is 0.15 events from
's
originating from beamline elements, and <0.21 events
from
decays (all
as the
is too high for
). The former is estimated
by studying the
distribution of
's originating
from a ``hot'' flange located immediately upstream of 9.65 m.
The latter is estimated by first counting the number of
final events cut because the low-momentum track had
(these are electrons); this is then
multiplied by the ratio of the number of electrons passing PbG
analysis cuts to the number having
,
as determined from a sample of
decays.
The
vs.
plot for the final high-
sample is shown in Fig. 2.
In this figure the Cherenkov veto for the freon counter is
not imposed. A band of
decays is visible at
MeV/c which results from the
MeV/c cut and the
cut;
this latter cut constrains
from above.
's which originate from beamline elements
are visible at low
. For the freon subset,
when we require that there be no signal in the left
Cherenkov counter, all but two
decays
are eliminated while all
's at low
remain.
Figure 2: vs.
for the high-
sample. The signal region is denoted by dashed lines. The band of
events from
=145 to
150 MeV/c are
decays; the leftmost edge is due to a
cut,
while the rightmost edge is due to a lower cut on
.
Figure 3: vs.
for the final high-
sample.
The two events in the signal region are circled.
The cluster of events at
GeV/c,
GeV/
are consistent with
Monte Carlo simulated
decays. There is a
third event which is well-separated from the
decays and which lies just outside the signal region; the
3 separated events are consistent with
decay if
GeV/
.
Also visible in Fig. 2 are our two candidates,
which have of 187 and 191 MeV/c and
of 6.7
and 9.4. The
values correspond to a Jacobian peak from
decay if
GeV/
.
The probability for a
decay to have such high
is extremely small, as it is
kinematically forbidden for a
decay to
have both
and
MeV/c (Fig. 3).
The probability for a
decay to look like
these events is also very small, as
the PbG response for the electron candidate tracks is very
uncharacteristic of electrons:
= 0.44 and 0.27, and for both events
= 0 (Fig. 4).
This response is typical of pions from
decay.
To investigate background from neutrons in the beam interacting
with residual gas molecules in the decay tank, we recorded and analyzed a
sample of data equivalent to 1% of the total sample with the decay tank
vacuum spoiled by a factor
. This sample yielded one event
in the signal region, implying a background level in the rest of
the data of 0.04 events. We also studied potential background from
decays where the
originates
from a beamline element; from Monte Carlo simulation and the number
of
's observed originating from beamline elements,
we estimate a background of less than 0.10 events.
The total background estimate from known sources is less than
0.50 events. The probability of 0.50 events
fluctuating up to two or more events is 0.090; if such a
fluctuation occurred, it is remarkable that the
of the events is so similar.
Figure 4: (PbG) vs.
for:
a) the low momentum track of
's from the final
high-
sample with only the PbG cuts relaxed, and
b) low momentum electrons from
decay. In (a), the tracks from the two events in
the signal region are circled. There are 4.7 times as many events
in (b) as in (a).
Figure 5: 90% C.L. upper limits on the H production cross section
as a function of or
(see Ref. [3]). The dashed
contour corresponds to an H lifetime half that given on the top
scale.
A 90% C.L. upper limit on the H production cross section can be
expressed in terms of the inclusive production cross section
as follows:
where
is the number of
's
originating from the target,
and
are geometric acceptances for
's
originating from the target and from H decays, respectively,
and
are branching ratios,
is the inclusive
production cross section,
and
is the factor which multiplies the single-event
sensitivity to give the value of
which has
a 10% chance of producing
2 detected events.
Here we conservatively assume no background and take
.
The acceptance
accounts
for the fact that
's from H's must project back to a
restricted region of the beamline.
Since
decays are common to both
signal and normalization channels, all trigger and detection
efficiencies divide out of Eq. (1).
The acceptances and
were determined from Monte Carlo
simulation using several different estimates of the production momentum
spectra. For the H simulation, a central production spectrum was
used with a broad peak at
. A spectrum corresponding
to a
coalescence model for
H production [7] resulted in a limit on
about 50% lower. We quote here the more
conservative limit resulting from the central production spectrum.
The inclusive
production spectrum
was taken from a measurement by Abe et al.[8];
comparison with our data shows very good agreement.
The acceptance also depends crucially on H lifetime.
Here we assume the relationship between
and
,
, and
calculated by Donoghue et al.[3], and
obtain 90% C.L. upper limits on
as a
function of
. Our acceptance is maximum
for
ns and becomes small for
ns due to
the
m cut. Our limits for
are
plotted in Fig. 5.
For
GeV/
, Jaffe's original prediction,
From Abe et al.[8],
mb/sr, so
b/sr.
For
GeV/
,
consistent with the observed
,
the acceptance is lower and the two candidate events correspond
to a differential cross section of
b/sr.
The authors of Ref. [3] note that
may be shorter than their predicted value by up
to a factor of two; this would increase our acceptance for
GeV/
and decrease our acceptance for
greater than this value.
The resultant 90% C.L. upper limits are plotted as the dashed
contour in Fig. 5. If we assume that the
invariant cross section
has the form
, then our limit (2)
corresponds to
nb for a wide range of
parameters B and C.
There are few theoretical predictions of the H production
cross section. Cousins and Klein[7] predict
a differential cross section of 100
b/sr
for p-Cu interactions at our targeting angle based on a
coalescence model. Cole et al.[9]
considers
and
coalescence
and predicts
for p-Cu collisions at AGS energies; taking the inelastic cross
section
to be
780 mb[10]
gives
b.
Rotondo[11] considers only
coalescence and
predicts a total cross section at Fermilab energies of 1.2
b.
We are indebted to the E791 and E871 collaborations, which built or supported most of the apparatus used here. We thank V.L.Fitch for much encouragement, and S. Black, K. Schenk, and N. Mar for their help in various stages of this work. We gratefully acknowledge the strong support of BNL, in particular R. Brown, A. Pendzick, the AGS staff, and the C.C.D. We also thank the SLAC computing division and the Princeton C.I.T., where all the data was reconstructed. This work was supported in part by the U.S. Department of Energy, the National Science Foundation, and the R.A. Welch Foundation.