K. Ruddick
University of Minnesota
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Featured researches published by K. Ruddick.
Physics Letters B | 1999
W. W. M. Allison; G. J. Alner; D. S. Ayres; G. Barr; W. L. Barrett; C. Bode; P. M. Border; C.B. Brooks; J. H. Cobb; R. Cotton; H. Courant; D. M. Demuth; T. Fields; Hugh R. Gallagher; C. Garcia-Garcia; M. C. Goodman; R. Gran; T. Joffe–Minor; T. Kafka; S. M S Kasahara; W. Leeson; P. J. Litchfield; N. P. Longley; W. A. Mann; M. L. Marshak; R. H. Milburn; W. H. Miller; L. Mualem; A. Napier; W. P. Oliver
Abstract We report a measurement of the atmospheric neutrino flavor ratio, R, using a sample of quasi-elastic neutrino interactions occurring in an iron medium. The flavor ratio (tracks/showers) of atmospheric neutrinos in a 3.9 fiducial kiloton-year exposure of Soudan 2 is 0.64±0.11(stat.)±0.06(syst.) of that expected. Important aspects of our main analysis have been checked by carrying out two independent, alternative analyses; one is based upon automated scanning, the other uses a multivariate approach for background subtraction. Similar results are found by all three approaches.
Physics Letters B | 1997
W. W. M. Allison; G. J. Alner; D. S. Ayres; W. L. Barrett; C. Bode; P. M. Border; C.B. Brooks; J. H. Cobb; D. J. A. Cockerill; R. Cotton; H. Courant; D. M. Demuth; T. Fields; Hugh R. Gallagher; C. Garcia-Garcia; M. C. Goodman; R.N. Gray; K. Johns; T. Kafka; S. M S Kasahara; W. Leeson; P. J. Litchfield; N. P. Longley; M. Lowe; W. A. Mann; M. L. Marshak; Edward May; R. H. Milburn; W. H. Miller; L. Mualem
Abstract The atmospheric neutrino flavour ratio measured using a 1.52 kton-year exposure of Soudan 2 is found to be 0.72 ± 0.19−0.07+0.05 relative to the expected value from a Monte Carlo calculation. The possible background of interactions of neutrons and photons produced in muon interactions in the rock surrounding the detector has been investigated and is shown not to produce low values of the ratio.
Physical Review D | 2003
Manuel Calderon De La Barca Sanchez; W. W. M. Allison; G. J. Alner; D. S. Ayres; W. L. Barrett; P. M. Border; J. H. Cobb; D. J. A. Cockerill; H. Courant; D. M. Demuth; T. Fields; H. R. Gallagher; M. C. Goodman; T. Joffe-Minor; T. Kafka; S. M. S. Kasahara; P. J. Litchfield; W. A. Mann; M. L. Marshak; R. H. Milburn; W. H. Miller; L. Mualem; J. K. Nelson; A. Napier; W. P. Oliver; G. F. Pearce; E. A. Peterson; D. Petyt; K. Ruddick; J. Schneps
The effects of oscillations of atmospheric muon neutrinos are observed in the 5.90 fiducial kiloton-year exposure of the Soudan 2 detector. An unbinned maximum likelihood analysis of the neutrino L/E distribution has been carried out using the Feldman-Cousins prescription. The probability of the no oscillation hypothesis is 5.8x10-4. The 90% confidence allowed region in the sin**(2theta), Delta m**2 plane is presented.
Physics Letters B | 1995
A.S. Barabash; F. T. Avignone; J. I. Collar; C.K. Guerard; R.J. Arthur; R.L. Brodzinski; H.S. Miley; J.H. Reeves; J.R. Meier; K. Ruddick; V.I. Umatov
Abstract Double-beta decay of 100Mo to the 0+ excited sate at 1130.29 keV in 100ru has been observed. A 956g sample of molybdenum powder enriched to 98.468% 100Mo was counted in a “Marinelli” geometry with a well-shielded, ultralow-background germnium detector. The cascade gamma rays at 539.53 and 590.76 keV in 100Ru were observed. The resulting half-life is (6.1−1.1+1.8)×1020 yr at the 68% confidence limit in disagreement with a recently published limit.
Physical Review D | 2005
W. W. M. Allison; G. J. Alner; D. S. Ayres; G. Barr; W. L. Barrett; P. M. Border; J. H. Cobb; D. J. A. Cockerill; H. Courant; D. M. Demuth; T. Fields; H. R. Gallagher; M. C. Goodman; T. Kafka; S. M S Kasahara; P. J. Litchfield; W. A. Mann; M. L. Marshak; W. H. Miller; L. Mualem; J. K. Nelson; A. Napier; W. P. Oliver; G. F. Pearce; E. A. Peterson; D. Petyt; K. Ruddick; Manuel Calderon De La Barca Sanchez; J. Schneps; A. Sousa
Upward-going stopping muons initiated by atmospheric {nu}{sub {mu}} and {nu}{sub {mu}} interactions in the rock below the Soudan 2 detector have been isolated, together with a companion sample of neutrino-induced single muons, created within the detector, which travel downwards and exit. The downward-going sample is consistent with the atmospheric-neutrino flux prediction, but the upward-going sample exhibits a sizable depletion. Both are consistent with previously reported Soudan 2 neutrino-oscillation results. Inclusion of the two samples in an all-event likelihood analysis, using recent 3D-atmospheric-neutrino-flux calculations, reduces both the allowed oscillation parameter region and the probability of the no-oscillation hypothesis.
Physical Review D | 2002
J. Chung; J. L. Thron; A. Sousa; B. Speakman; W. P. Oliver; W. W. M. Allison; A. Napier; R. H. Milburn; P. M. Border; W. H. Miller; T. Joffe-Minor; G. J. Alner; H. R. Gallagher; J. Schneps; R. Gran; P. J. Litchfield; D. Petyt; M. L. Marshak; D. S. Ayres; W. L. Barrett; D. M. Demuth; N. West; W. A. Mann; M. C. Goodman; Manuel Calderon De La Barca Sanchez; L. Mualem; K. Ruddick; E. A. Peterson; S. M. S. Kasahara; J. H. Cobb
We have searched for neutron-antineutron oscillations using the 5.56 fiducial kiloton-year exposure of the Soudan 2 iron tracking calorimeter. We require candidate n-nbar occurrences to have .GE. 4 prongs (tracks and showers) and to have kinematics compatible with nbar-N annihilation within a nucleus. We observe five candidate events, with an estimated background from atmospheric neutrino and cosmic ray induced events of 4.5 \pm 1.2 events. Previous experiments with smaller exposures observed no candidates, with estimated background rates similar to this experiment. We set a lifetime lower limit for oscillation time in iron: T_A(Fe) > 7.2x10^{31} years. The corresponding lower limit for oscillation of free neutrons is \tau_{n-nbar} > 1.3x10^8 seconds.
Physical Review D | 1997
D. S. Ayres; T.H. Fields; M. C. Goodman; Edward May; L. E. Price; R.V. Seidlein; J. L. Thron; H.J. Trost; Jack L. Uretsky; S. M S Kasahara; C. Bode; P.M. Border; H. Courant; D. M. Demuth; R. Gran; R.N. Gray; K. Johns; N. P. Longley; M. Lowe; M. L. Marshak; W. H. Miller; L. Mualem; E.A. Peterson; D.M. Roback; K. Ruddick; D. J. Schmid; M.H. Schub; Shupe; V. Vassiliev; G. Villaume
Deep underground muon events recorded by the Soudan 2 detector, located at a depth of 2100 m of water equivalent, have been used to infer the nuclear composition of cosmic rays in the ``knee`` region of the cosmic ray energy spectrum. The observed muon multiplicity distribution favors a composition model with a substantial proton content in the energy region 8{times}10{sup 5}{endash}1.3{times}10{sup 7} GeV/nucleus. {copyright} {ital 1997} {ital The American Physical Society}
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1996
W. W. M. Allison; G. J. Alner; I. Ambats; D. S. Ayres; L. J. Balka; G. Barr; W. L. Barrett; Douglas Benjamin; C. Bode; P. M. Border; C.B. Brooks; J. H. Cobb; D. J. A. Cockerill; K. Coover; R. Cotton; H. Courant; B. Dahlin; U. DasGupta; J. Dawson; D. M. Demuth; V.W. Edwards; B. Ewen; T. Fields; C. Garcia-Garcia; H.M. Gallagher; R.H. Giles; G.L. Giller; M. C. Goodman; R.N. Gray; S. Heppelmann
SOUDAN 2 is a 960-ton tracking calorimeter which has been constructed to search for nucleon decay and other phenomena. The full detector consists of 224 calorimeter modules each weighing 4.3 tons. The design and construction of the modules are described. The modules consist of finely segmented iron instrumented with 1 m long drift tubes of 15 mm internal diameter. The tubes enable three spatial coordinates and dE/dx to be recorded for charged particles traversing the tubes.
Physics Letters B | 1977
R. Klem; G. Igo; R. Talaga; A. Wriekat; H. Courant; K. Einsweiler; T. Joyce; H. Kagan; Y. Makdisi; M. L. Marshak; B. Mossberg; E. A. Peterson; K. Ruddick; T.F. Walsh
Abstract We have measured the differential cross section for p- 4 He elastic scattering at proton kinetic energies of 0.56, 0.80, 1.03, 1.27 and 1.73 GeV in a range of four-momentum transfer squared between 0.006 and 1.2 (GeV/ c ) 2 . The cross section has the usual diffraction minimum which decreases in depth with increasing energy. This data is consistent with contemporaneous data from Berkeley, but disagrees, particularly in the normalization, with earlier data from Brookhaven and Saclay.
Physical Review Letters | 1991
G. Alverson; P. F. Shepard; M. Glaubman; K. Ruddick; L. Sorrell; W. Toothacker; David A. Brown; E. Prebys; D. Skow; T. Chand; G. Fanourakis; J. Dunlea; C. Yosef; J. Huston; W. DeSoi; W. H. Chung; M. Zielinski; C. Bromberg; B. Y. Oh; D. Weerasundara; I. Kourbanis; G. Ginther; D. Berg; B. M. Rajaram; B.C. Choudhardy; T. Yasuda; W. Dlugosz; David C. Carey; R. K. Shivpuri; F. Lobkowicz
We report new measurements of inclusive direct photon production at high transverse momenta (pT) for π - and p interactions on Be at 500 Gev/r. The yields as a function of pT and rapidity (y) are in good agreement with expectations from next-to-leading-log QCD calculations employing recently extracted quark and gluon structure functions