Michael H. Shaevitz
Columbia University
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Featured researches published by Michael H. Shaevitz.
European Physical Journal A | 1995
Andrew O. Bazarko; C. G. Arroyo; K.T. Bachmann; T. Bolton; C. Foudas; B.J. King; W.C. Lefmann; W.C. Leung; S.R. Mishra; E. Oltman; P. Z. Quintas; S.A. Rabinowitz; F. Sciulli; W.G. Seligman; Michael H. Shaevitz; F. S. Merritt; M. J. Oreglia; B.A. Schumm; R. H. Bernstein; F. Borcherding; H. E. Fisk; M.J. Lamm; W. Marsh; K. W. Merritt; H. Schellman; D. Yovanovitch; Arie Bodek; Howard S. Budd; P. de Barbaro; Willis Sakumoto
AbstractWe present the first next-to-leading-order QCD analysis of neutrino charm production, using a sample of 6090νμ− and
Physical Review D | 2004
M. Sorel; J. M. Conrad; Michael H. Shaevitz
Reviews of Modern Physics | 1998
J. M. Conrad; Michael H. Shaevitz; Tim Bolton
\bar \nu _\mu
European Physical Journal A | 1984
D. B. MacFarlane; M. V. Purohit; R. L. Messner; D. B. Novikoff; R. E. Blair; F. Sciulli; Michael H. Shaevitz; H. E. Fisk; Y. Fukushima; B. Jin; Q. A. Kerns; T. Kondo; P. A. Rapidis; S. Segler; R. Stefanski; D. Theriot; D. Yovanovitch; Arie Bodek; R. N. Coleman; W. Marsh; O. Fackler; K. A. Jenkins
Annual Review of Nuclear and Particle Science | 2013
J. M. Conrad; W. C. Louis; Michael H. Shaevitz
-induced opposite-sign dimuon events observed in the CCFR detector at the Fermilab Tevatron. We find that the nucleon strange quark content is suppressed with respect to the non-strange sea quarks by a factor κ=0.477−0.053+0.063, where the error includes statistical, systematic and QCD scale uncertainties. In contrast to previous leading order analyses, we find that the strange seax-dependence is similar to that of the non-strange sea, and that the measured charm quark mass,mc=1.70±0.19 GeV/c2, is larger and consistent with that determined in other processes. Further analysis finds that the difference inx-distributions betweenxs(x) and
European Physical Journal C | 1992
E. Oltman; P. S. Auchincloss; R.E. Blair; C. Haber; S.R. Mishra; M. Ruiz; F. Sciulli; Michael H. Shaevitz; W. H. Smith; F. S. Merritt; M. J. Oreglia; P. G. Reutens; Richard Coleman; H. E. Fis; D. Levinthal; W. Marsh; P. A. Rapidis; H. B. White; D. Yovanovitch; Arie Bodek; F. Borcherding; N. Giokaris; K. Lang; I. E. Stockdale
International Journal of Modern Physics A | 2006
Kendall Brianna McConnel Mahn; Michael H. Shaevitz
x\bar s{\text{(}}x{\text{)}}
European Physical Journal A | 1987
K. Lang; Arie Bodek; F. Borcherding; N. Giokaris; I. E. Stockdale; P. S. Auchincloss; R.E. Blair; C. Haber; S. Mishra; E. Oltman; M. Ruiz; F. Sciulli; Michael H. Shaevitz; W. H. Smith; R. Zhu; Y. K. Chu; D. B. MacFarlane; R. L. Messner; D. B. Novikoff; M. V. Purohit; David Garfinkle; Frank Merritt; Mark Oreglia; P. G. Reutens; Richard Coleman; H. E. Fisk; Y. Fukushima; O. Kerns; B. Jin; D. Levinthal
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1991
B.J. King; C. G. Arroyo; K.T. Bachmann; R.E. Blair; C. Foudas; W.C. Lefmann; W.C. Leung; S.R. Mishra; E. Oltman; P. Z. Quintas; S.A. Rabinowitz; F. Sciulli; W.G. Seligman; Michael H. Shaevitz; Frank Merritt; Mark Oreglia; B.A. Schumm; R. H. Bernstein; F. Borcherding; H. E. Fisk; M.J. Lamm; W. Marsh; K. W. Merritt; H. Schellman; D. Yovanovitch; Arie Bodek; Howard S. Budd; P. de Barbaro; Willis Sakumoto; P.H. Sandler
is small. A measurement of the Cabibbo-Kobayashi-Maskawa matrix element |Vcd|=0.232−0.020+0.018 is also presented.
Nuclear Physics B - Proceedings Supplements | 1991
Michael H. Shaevitz
We investigate adding two sterile neutrinos to resolve the apparent tension existing between short-baseline neutrino oscillation results and CPT-conserving, four-neutrino oscillation models. For both (3+1) and (3+2) models, the level of statistical compatibility between the combined dataset from the null short-baseline experiments Bugey, CHOOZ, CCFR84, CDHS, KARMEN, and NOMAD, on the one hand; and the LSND dataset, on the other, is computed. A combined analysis of all seven short-baseline experiments, including LSND, is also performed, to obtain the favored regions in neutrino mass and mixing parameter space for both models. Finally, four statistical tests to compare the (3+1) and the (3+2) hypotheses are discussed. All tests show that (3+2) models fit the existing short-baseline data significantly better than (3+1) models.