W. Smart
University of California, Berkeley
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Physical Review D | 1989
H.C. Ballagh; G.R. Lynch; F.A. Harris; E. Wolin; K. Moriyasu; W. Smart; V. Z. Peterson; D.D. Reeder; Jones; R.J. Cence; E. E. Schmidt; T.J. Lawry; H.H. Bingham; U. Camerini; E. Treadwell; W. Fry; M. L. Stevenson; H.J. Lubatti; A. Koide; J. Lys; R.J. Loveless; M. Gee; Sokoloff; D. Gee; M.W. Peters; F.R. Huson
In an experiment (E546) to study interactions of {l angle}{ital E}{r angle}=100 GeV and {l angle}{ital Q}{sup 2}{r angle}=17 GeV{sup 2} neutrinos in the Fermilab 15-foot bubble chamber, we have looked for a left-right asymmetry in the azimuthal angle {phi} of individual hadrons about the direction of the lepton momentum transfer ({ital q} vector). Significant asymmetry is found for forward positive hadrons; for {ital x}{sub {ital F}}{gt}0.10, we find {l angle}cos{phi}{r angle}={minus}0.029{plus minus}0.008, where {ital x}{sub {ital F}} is the Feynman {ital x} variable. Negative hadrons with {ital x}{sub {ital F}}{gt}0.10 show no asymmetry, {l angle}cos{phi}{r angle}=0.004{plus minus}0.011. A model which includes parton intrinsic transverse momentum {ital k}{sub {ital t}} reproduces the asymmetry of combined positive and negative hadrons with {ital x}{sub {ital F}}{gt}0.10, {l angle}cos{phi}{r angle}={minus}0.018{plus minus}0.0065, if {l angle}{ital k}{sub {ital t}}{sup 2}{r angle}=0.065{plus minus}0.024 GeV{sup 2}/c{sup 2}. But the model predicts almost equal asymmetries for positive and negative hadrons. The model also agrees poorly with the observed dependence on the kinematic variables {ital x} and {ital Q}{sup 2} if the {ital k}{sub {ital t}} distribution is assumed to be independent of kinematic variables.
Physical Review D | 1982
G.N. Taylor; H.H. Bingham; S.I. Parker; D. Gee; Jones; V.J. Stenger; T.J. Lawry; F.R. Huson; E. E. Schmidt; F.A. Harris; R.J. Cence; M.W. Peters; E. Treadwell; G.P. Yost; M. L. Stevenson; J. Lys; W. Smart; V. Z. Peterson; H.C. Ballagh
In an exposure of the Fermilab 15-ft bubble chamber to the dichromatic antineutrino beam, 427 nu-bar/sub ..mu../ charged-current interactions were obtained. Taking advantage of the small and well understood background flux of nu-bar/sub e/s in the dichromatic nu-bar/sub ..mu../ beam, upper limits on the rates of antineutrino oscillations are obtained, with the precision limited by statistical rather than systematic errors, in contrast to previous experiments. The 90%-C.L. upper limits obtained for the average oscillation probabilities indicated are P(nu-bar/sub ..mu../..-->..nu-bar/sub e/) ..nu-bar/sub tau/)<4.4 x 10/sup -2/. The mean value of the distance from the neutrino-production point to the bubble chamber divided by the neutrino energy, , is 0.03 m/MeV.
Physical Review Letters | 1978
J. Bell; J. P. Berge; D. Bogert; R. J. Cence; C. T. Coffin; R. N. Diamond; F.A. DiBianca; R. Endorf; R. Hanft; F. A. Harris; M. Jones; C. Kochowski; W.C. Louis; G. Lynch; J. A. Malko; John P. Marriner; G.I. Moffatt; F.A. Nezrick; M. Peters; V.Z. Peterson; B.P. Roe; R.T. Ross; W. G. Scott; A.A. Seidl; W. Smart; V. J. Stenger; M. L. Stevenson; J.C.V. Velde; E. Wang
Physical Review Letters | 1971
A. D. Brody; W. B. Johnson; Brandt Kehoe; D. W. G. S. Leith; J. S. Loos; George Luste; K. Moriyasu; B. S. Shen; W. Smart; F. C. Winkelmann; R. J. Yamartino
Physical Review D | 1980
V. I. Efremenko; A. V. Fedotov; P. A. Gorichev; V. S. Kaftanov; G. K. Kliger; V. Z. Kolganov; S. P. Krutchinin; M. A. Kubantsev; I. V. Makhlyueva; M. M. Savitsky; V. I. Shekeljan; V. G. Shevchenko; J. P. Berge; D. Bogert; R. Endorf; R. Hanft; J.A. Malko; G. I. Moffatt; F.A. Nezrick; R. Orava; W. Smart; J. Wolfson; V. V. Ammosov; A. G. Denisov; G. S. Gapienko; V. A. Gapienko; V.I. Klyukhin; V. I. Koreshev; P. V. Pitukhin; E. A. Slobodyuk
Physical Review Letters | 1966
W. Smart; Anne Kernan; George E. Kalmus; Robert P. Ely
Physical Review D | 1980
H. C. Ballagh; H.H. Bingham; W.B. Fretter; T. Lawry; G. Lynch; J. Lys; John P. Marriner; J. Orthel; Sokoloff; M. L. Stevenson; G.P. Yost; B. Chrisman; D. Gee; A. Greene; G. Harigel; F. R. Huson; T. Murphy; E. E. Schmidt; W. Smart; E. Treadwell; J. Wolfson; R. J. Cence; F. A. Harris; Jones; Sherwood Parker; M. Peters; V. Z. Peterson; T. H. Burnett; L. Fluri; D. Holmgren
Physical Review Letters | 1978
J. Bell; J. P. Berge; D. Bogert; R. J. Cence; C. T. Coffin; R. N. Diamond; Frank A. DiBianca; R. Endorf; R. Hanft; F. A. Harris; M. Jones; C. Kochowski; W.C. Louis; G. Lynch; J. A. Malko; John P. Marriner; G. I. Moffatt; F.A. Nezrick; M. Peters; V. Z. Peterson; B.P. Roe; R.T. Ross; W. G. Scott; A.A. Seidl; W. Smart; V. J. Stenger; M. L. Stevenson; J.C.V. Velde; E. Wang
Physical Review Letters | 1966
Anne Kernan; W. Smart
Physical Review D | 1993
S. Willocq; M. Aderholz; H. Akbari; Phillip Allport; S.K. Badyal; H.C. Ballagh; M. Barth; H.H. Bingham; E.B. Brucker; R.A. Burnstein; R.J. Cence; T.K. Chatterjee; E.F. Clayton; G. Corrigan; D. De Prospo; Devanand; E. A. De Wolf; P.J.W. Faulkner; H. Foeth; W.B. Fretter; V.K. Gupta; J. Hanlon; G. Harigel; Frederick A. Harris; P.F. Jacques; V. Jain; G. Jones; Jones; T. Kafka; M. Kalelkar