VOLUME 45, NUMBER 12 P H Y S I C A L R E V I E W L E T T E R S 22 SEPTEMBER 1980
Charmed-Baryon Production in High-Energy Neutrino-Deuterium Interactions T. Kitagaki, S. Tanaka, H. Yuta, K. Abe, K. Hasegawa, A. Yamaguchi, K. Tamai,
T. Hayashino, S. Kunori, Y. Ohtani, and H. Hayano Tohoku University, Sendai 980, Japan
and
R. A. Burns te in , J . Hanlon, and H. A. Rubin Illinois Institute of Technology, Chicago, Illinois 60616
and
C. Y. Chang, T. Dombeck, G. A. Snow, D. Son, and P. H. Steinberg University of Maryland, College Park, Maryland 20742
and
R. Engelmann, T. Kafka, and S. Sommars State University of New York at Stony Brook, Stony Brook, New York 11794
and
J. Callas, C. C. Chang, W. A. Mann, and J. Schneps Tufts University, Medford, Massachusetts 02155
(Received 9 June 1980)
In a sample of ~15 000 charged current v + d interactions from an exposure of the Fer-milab 15-ft bubble chamber to a high-energy, wide-band neutrino beam, the production of the Ac
+ charmed baryon decaying into Air+ and K°p is observed. The measured mass value is 2.275±0.010 GeV. The products of the production rate and the branching ratio for these channels are (1.8± 0.9) x io"3 and (3.5± 2.0) x 10"3 , respectively.
PACS numberst 13.15.+g, 14.20.-c
Since the first observation1 of the charmed baryon, Ad
+ , in an exclusive neutrino reaction, additional evidence for Ac
+ production has been reported in photon interactions,2/)-/? interactions,3
ande+e~ annihilation.4 In inclusive neutrino r e actions the Ac
+ has been observed5 as the decay product of the S c
+ + . However, most of the Ac +
properties have not been established. In this paper, we present results on Ac
+ production in high-energy inclusive neutrino-deuterium reactions, using a data sample of events with associated neutral strange particles (vees). In particular , we report the first observation of the Ac
+
peak in the inclusive channels of Avr+ and/f°/>, including their production rates times branching ratios and a new measurement of the Ac
+ mass . The data sample used for this analysis is based
on measurements of 90% of the vee events in a 328 000-frame exposure of the Fermilab 15-ft deuterium-filled bubble chamber, with a two-plane external muon identifier, to a wide-band single-horn focused neutrino beam produced by 350-GeV/c protons. This sample corresponds to a flux of 4.46xl01 8 protons on the target. The neutrino energies range from 10 to 250 GeV, with
an average energy (E)~ 50 GeV. The vee-associated events are collected from
a double scan for all neutral-induced events (^ 2 prongs) with one or more possible neutral strange decays. These events are measured and processed through the TVGP-SQUAW program chain. The vees are classified into KS°-~TT+TT~ and A *pir~ with use of the x2 probability of the fits together with information about the transverse momenta of the decay products. The A/K° ambiguous fits (~ 12% of the V° decays) are now classified: 10% into the A and 2% into the K° sample from this selection. Examination of the TT+TT" mass distribution for the A decay sample (assuming the proton as a TT + ) indicates - 3 % contamination from Ks° decays in the A sample.
To reduce background from low-energy neutral hadron events, we require that the sum of the longitudinal momenta for all visible secondaries including the V° be greater than 5 GeV/c. In addition, we restrict the fiducial volume to 14.2 m3
corresponding to 2.0 tons of deuterium, to improve the momentum resolution. For these selected events, we find the Ks° and A mass values of 497.7± 0.2 and 1115.6± 0.1 MeV/c2 with the
© 1980 The American Physical Society 955
VOLUME 45, NUMBER 12 P H Y S I C A L R E V I E W L E T T E R S 22 SEPTEMBER 1980
mass resolutions of a = 5.1 and 1.7 MeV/c2, r e spectively. This Ks° mass resolution is better than that obtained from the Ne-H2 mixture experiment6 by more than a factor of 2C
The charged-current events are selected by applying the following kinematic method7 to the sample described above: Fi rs t , we take the M" to be the negative track having no visible interactions and the maximum value of the quantity JP , defined in Ref. 7. Then, we select the charged-current events as those with the M~ transverse momentum relative to the other total visible particles, P T R , greater than 0.7 GeV/c. From this selection, we estimate a total of 15 000 charged-current events8 corresponding to the V° sample used for this analysis. This number includes the corrections for the scanning and measuring efficiencies.
Figures 1(a), 1(b), and 1(c) show, respectively, the invariant mass distributions for the An* ,K°p and the sum of these two channels, which are among the expected Cabibbo-favored weak decays of the Ac
+ . The charged multiplicity in these distributions is restricted to be less than 8 prongs to reduce combinatorial background. With this r e -
2.2 2.6 3.0 MA55,GeV
FIG. 1. Invariant-mass distributions for (a) ATT+ , (b) Kfy f and (c) sum of the two channels. The shaded areas correspond to the events with the helicity decay angular cuts; (a) cosfl>-0.75, (b) cos0>-O.9, and (c) sum of these from (a) and (b).
striction, we obtain 402 K° and 339 A events. The corresponding number of charged-current events is estimated to be 13 000,9 of which 11 000 events have hadronic energy W> 2.2 GeV. For calculating the effective masses , we take all hadron tracks except identified protons to be pions for events with an identified nonspectator proton or A. For events without an identified nonspectator proton or A, each positive track is taken to be both rr or proton.
As seen in Fig. 1, we observe peaks at the Ac +
mass region in the ATT+ ,K°p channels as well as in their sum0 We examine the effect of the A/K° ambiguous events on the Ac
+ mass region and find that these events contribute a smooth background [5 events in the mass range of 2.24 to 2.32 GeV/c2 in Fig. 1(c)]. The best fits to a polynomi-nal background plus a Gaussian, shown by the curves in Fig. 1, give the excesses of events 9.5 ±4.7, 9.8± 5.7, and 19.3± 7.3 above the background curves for ATT + , K°p, and their sum in the mass interval of 2.24 to 2.32 GeV/c2, where the mass value and the resolution are fixed as m = 2.275 GeV/c2 and a =0.02 GeV/c2.
In order to examine further this mass peak, we show in Figs. 2(a) and 2(b) the cos# distributions for the ATT+ andK°p channels, where 9 is the
FIG. 2. The decay angular distributions for (a) A7r+
and (b) K°p system.
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VOLUME 45, NUMBER 12 P H Y S I C A L R E V I E W L E T T E R S 22 SEPTEMBER 1980
helicity decay angle of the baryon relative to the momentum direction of ATT + (K°p) system in its rest frame. Apparent peaks are observed at cos# = - 1 for both systems. The peak for the Air* is broader than that for the K°p. To examine whether the effect at the Ac
+ mass is related to the peaks observed in Figs. 2, we remove events with cosO < - 0.75 for the ATT+ channel and cos0 < - 0.90 for the K°p channel and display the r e -remainder in Fig. 1 as the shaded events. These angular cuts should remove only 12.5% and 5% of the An + and K°p events, respectively, at the Ac
+
mass if the Ac + decay angular distribution is uni
form. As seen from the shaded events in Fig. 1, no apparent loss of events is observed from these angular cuts, indicating that the effect observed at the Ac
+ mass is not related to the peaks observed in Fig. 2. The best fits to a polynomial background plus a Gaussian for the shaded events in Fig. 1 give the signals 8±3.5, 11±4.5, and 19 ± 5.7 events for the Atr+, K°p, and their sum, r e spectively. The small peaks (< 3a) observed at 2.02 and 2.74 GeV/c2 in Fig. 1 are much reduced by these angular cuts indicating that these come primarily from the peak region observed in Fig. 2« There has been a F*(2030) reported,10 however.
Since the sum of the two channels gives a peak of 3.3a and 2.6a for the shaded and unshaded events above the background at the previously measured values of the Ac
+ mass , we interpret this peak as the production of the charmed baryon, Ac
+ , in inclusive neutrino reactions. In order to obtain the mass value of the Ac
+ , we show in Fig. 3(a) the ideogram11 for the sum of the An* and#°/> channels fit to a distribution with a polynominal background plus a Gaussian. The mass value obtained from the fit is
m = 2.275± 0.010 GeV/c2,
with a mass resolution of 20 MeV/c2 which is consistent, within the er ror , with the Ac
+ mass values1"5 reported previously. We have examined the systematic shift of the ATT + and K°p masses. Examination of the KS°-~IT+TT" peak position throughout the exposure indicates the variation of the magnetic field to be less than 0.7%; hence any shift of the ATT+ andif°£ masses resulting from drifting of the field strength is less than 10 MeV/c2. Also, we have studied the masses of Ks° for possible dependence upon position in the chamber and for possible variation with different sets of optical constants. We find that any variation amounts to less than 1 MeV/c2.
To estimate the production rates of the Ac+ fol-
2.2 2.4 MASS, GeV
2.6
FIG. 3. Ideograms for (a) sum of the A7r+ and K°p mass distribution [unshaded area in Fig. 1(c)] and (b) for the ATT+ mass distribution for events fitting to the AS = — AQ exclusive hypotheses. The inset is the A7r+ mass distribution with 40~MeV/c2 bins for these exclusive events.
lowed by decays into Air + and K°p, we correct the observed events above the background for the A *pTT~ andK^-^TT^TT' branching rat ios, the vee detection efficiencies (0.94 for A and 0.92 for Ks°) and the scan-measuring efficiency (0.80) and obtain 19.9± 9.8 and 38.4± 22.3 events for the Air +
and/f°/> channels, respectively. Comparing these to 11000 charged-current (CC) events (less than 8 prongs, W>2.2 GeV) expected in this vee sample, we obtain the products between the production rate and the branching ratio,
o^(Ac+)i?(Ac + ~A7r + )
i(CC) = (1.8±0.9)xl0"3
and
a„ (A/ ) f l (A , + -*<») = ( 3 < 5 ± 2 > 0 ) x l 0 - 3 a^(CC)
for the A7r+ a,ndK°p channels, respectively. The ratio for the two Ac
+ decay branching rat ios, R(AC
+ -*ATT + )/R(AC + -~K°P), is 0 . 5 1 ± ^ 2 , which is consistent with the value of 0.67±£;™ obtained by Baltay et al.5
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VOLUME 45, NUMBER 12 P H Y S I C A L R E V I E W L E T T E R S 22 SEPTEMBER 1980
We have also searched for the Ac + decaying in
to A7r+7r+77" and K°pir*iT~ by examining these invariant-mass distributions. No significant signal is observed in the Ac
+ mass region in either of these mass distributions. We obtain upper limits on the products between production rate and the branching ratio, with 95% confidence level,
(rvd(Ae+)R(Ae
+ ^Ait+v+ir') 6 x 3
or^(CC)
and
q ^ A / M A / ^ V V ) ^ 8 x l 0 _ 3
crvd(CC)
for the A7r+7T+7r" andif°/>TT+7T" channels, respective
ly. We have also searched for charmed-baryon pro
duction in exclusive reactions from the vee event samplec Requiring the x2 probability to be greater than 5%, we find 48 events with A which fit three-constraint hypotheses with the AS = - AQ signature of charm production. Of course, the three-constraint fit does not always give a correct hypothesis, but certainly enhances the signal of charmed events above background.
Figure 3(b) shows the ideogram of the An+ mass distribution for these 48 events. The inset displays the histogram of this mass distribution. We observe 5 events in the ATT+ mass range between 2.24 and 2.32 GeV/c2. Of these, 2 events have the x2 probability of the AS = - AQ hypotheses strongly favored over background hypotheses with AS =0. It is interesting to note that, in spite of the low-statistics data, the ideogram shows the peak at the Ac
+ mass. The fitted mass value obtained from the ideogram in Fig. 3(b) gives m = 2.272± 0.010 GeV/c2 which is consistent with our measured mass value of the A c
+ . In summary, we have observed the Ac
+ signal in the An* andK°p channels with a statistical significance of about 3 standard deviations in inclusive neutrino reactions. The Ac
+ mass value is
measured to be 2.275± 0.010 GeV/c2. The products between the production rate and the branching ratio are (1.8±0.9)xl0~3 and (305± 2.0)xl0"3
for ATT+ 2LndK°p channels, respectively. No significant signal of the Ac
+ i s found in the ATT+TT+7I~ andK°pTT+iT~ channels .
We thank the members of the Accelerator Division and Neutrino Department at Fermilab for their assistance in conducting this experiment, with special appreciation to the 15-ft-bubble-chamber staff. We express our appreciation to the scanners and measurers who helped extract these data from the film. This research is supported in part by the U. S. Department of Energy and the National Science Foundation.
1E. G. Cazzoli etal., Phys. Rev. Lett. 34, 1125 (1975); A. M. Cnops etal., Phys. Rev. Lett. 42, 197 (1979).
2B. Knapp etal., Phys. Rev. Lett. 37, 882 (1976). 3D. Dr i ja rd^aZ. , Phys. Lett. 85B, 452 (1979); K. L.
Giboni etal., Phys. Lett. 85B, 437 (1979); W. Lockman etal., Phys. Lett. 85B, 443 (1979).
4G. S. Abrams etal., Phys. Rev. Lett. 44, 10 (1980). 5C. Baltay^aZ. , Phys. Rev. Lett. 42, 1721 (1979). 6C. Baltay, private communication. 7J. Bell etal., Phys. Rev. D19 , 1 (1979). 8According to our Monte Carlo simulation, the charged-
current events selected in this way contain about 6% background from the v neutral current, V charged current, and V neutral current. These background events give a negligible effect for the Ac + mass region in the ATT+ and pKs ° mass distributions.
9The scan-measuring efficiency is 0.78 for all-prong events and 0.80 for events with less than 8 prongs.
10R. L. Kelly etal. (Particle Data Group), Rev. Mod. Phys. 52, No. 2, Pt. 2, SI (1980).
nThe ideogram is generated by smearing each observed mass according to Gaussian distribution with the mass resolution calculated from the TVGP error matrices., We have checked that the ideograms reproduce the observed K° and A mass distributions. The areas in Fig. 3 are normalized to the corresponding combination numbers.
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