排序方式: 共有26条查询结果,搜索用时 109 毫秒
11.
S. R. Mishra P. S. Auchincloss R. Blair C. Haber M. Ruiz E. Oltman F. J. Sciulli M. H. Shaevitz W. H. Smith F. S. Merritt M. Oreglia P. Reutens R. Coleman H. E. Fisk M. J. Lamm D. Levinthal D. D. Yovanovitch W. Marsh P. A. Rapidis H. B. White A. Bodek F. Borcherding N. Giokaris K. Lang I. E. Stockdale 《Zeitschrift fur Physik C Particles and Fields》1989,44(2):187-198
We report on a search forv μ-induced events where the single emerging muon carries lepton number opposite that of the incident neutrino. The rate and kinematic quantities of the candidate events are compared with known backgrounds from \(\bar v_\mu \) -induced charged current interactions and ν-induced interactions that produce dileptons. We derive an upper limit on the rate of wrong-sign single muon production relative to the rate ofv μ charged current interactions to be 1.6×10?4 fory<0.5 and 3.1×10?4 fory>0.5 (90% CL). These upper limits enable us to constrain exotic sources of wrong-sign muons such as the charm component of the nucleon sea, flavor changing neutral currents and lepton number violating processes. Finally, the rate and kinematic properties of these events are compared with those of the neutrino-induced opposite-sign dimuon events. 相似文献
12.
A. Bodek W. Marsh M. V. Purohit P. S. Auchincloss R. Blair M. A. Ruiz F. J. Sciulli M. H. Shaevitz H. E. Fisk T. Kondo S. Pordes P. A. Rapidis D. D. Yovanovitch M. Abolins R. Brock D. Owen K. A. Jenkins O. Fackler 《Zeitschrift fur Physik C Particles and Fields》1983,18(4):289-299
We have observed Cerenkov light, well below threshold, in an integrating Cerenkov counter used to determine particle composition of the secondary hadron beam, which is the source of Fermilab narrow-band neutrinos. The phenomenon can be understood in terms of diffraction effects in a finite length counter caused by radiation emitted by particles traversing the counter even when it is evacuated. At zero pressure, the light can be considered as transition radiation produced when particles enter and leave the counter. A standard Cerenkov diffraction formula describes both the normal Cerenkov radiation and the light emitted below Cerenkov threshold. 相似文献
13.
K. Lang A. Bodek F. Borcherding N. Giokaris I. E. Stockdale P. Auchincloss R. Blair C. Haber S. Mishra E. Oltman M. Ruiz F. J. Sciulli M. Shaevitz W. H. Smith R. Zhu Y. K. Chu D. B. MacFarlane R. L. Messner D. B. Novikoff M. V. Purohit D. Garfinkle F. S. Merritt M. Oreglia P. Reutens R. Coleman H. E. Fisk Y. Fukushima O. Kerns B. Jin D. Levinthal T. Kondo W. Marsh P. A. Rapidis S. Segler R. Stefanski D. Theriot H. B. White D. Yovanovitch O. Fackler K. Jenkins 《Zeitschrift fur Physik C Particles and Fields》1987,33(4):483-503
Neutrino interactions with two muons in the final state have been studied using the Fermilab narrow band beam. A sample of 18v μ like sign dimuon events withP μ>9 GeV/c yields 6.6±4.8 events after backgroud subtraction and a prompt rate of (1.0±0.7)×10?4 per single muon event. The kinematics of these events are compared with those of the non-prompt sources. A total of 437v μ and 31 \(\bar v_\mu \) opposite sign dimuon events withP μ>4.3 GeV/c are used to measure the strange quark content of the nucleon: \(\kappa = {{2s} \mathord{\left/ {\vphantom {{2s} {\left( {\bar u + \bar d} \right) = 0.52_{ - 0.15}^{ + 0.17} \left( {or\eta _s \frac{{2s}}{{u + d}} = 0.075 \pm 0.019} \right) for 100< E_v< 230 GeV\left( {\left\langle {Q^2 } \right\rangle = {{23 GeV^2 } \mathord{\left/ {\vphantom {{23 GeV^2 } {c^2 }}} \right. \kern-0em} {c^2 }}} \right)}}} \right. \kern-0em} {\left( {\bar u + \bar d} \right) = 0.52_{ - 0.15}^{ + 0.17} \left( {or\eta _s \frac{{2s}}{{u + d}} = 0.075 \pm 0.019} \right) for 100< E_v< 230 GeV\left( {\left\langle {Q^2 } \right\rangle = {{23 GeV^2 } \mathord{\left/ {\vphantom {{23 GeV^2 } {c^2 }}} \right. \kern-0em} {c^2 }}} \right)}}\) using a charm semileptonic branching ratio of (10.9±1.4)% extracted from measurements ine + e ? collisions and neutrino emulsion data. 相似文献
14.
Schumm BA Merritt FS Oreglia MJ Schellman H Bachmann KT Bernstein RH Blair RE Foudas C Lefmann WC Leung WC Mishra SR Oltman E Quintas PZ Sciulli FJ Shaevitz MH Smith WH Borcherding FO Fisk HE Lamm MJ Marsh W Merritt KW Yovanovitch D Bodek A Budd HS Sakumoto WK 《Physical review letters》1988,60(16):1618-1621
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I. E. Stockdale A. Bodek F. Borcherding N. Giokaris K. Lang D. Garfinkle F. S. Merritt M. Oreglia P. Reutens P. S. Auchincloss R. Blair C. Haber M. Ruiz F. Sciulli M. H. Shaevitz W. H. Smith R. Zhu R. Coleman H. E. Fisk B. Jin D. Levinthal W. Marsh P. A. Rapidis H. B. White D. Yovanovitch 《Zeitschrift fur Physik C Particles and Fields》1985,27(1):53-56
17.
W.R. Ditzler D.A. Finley O.E. Johnson F.J. Loeffler E.I. Shibata C.W. Akerlof P. Alley R. Fabrizio P. Kraushaar D. Koltick D.I. Meyer R. Thun D. Bintinger R.L. Loveless R.A. Lundy K.C. Stanfield D.D. Yovanovitch 《Physics letters. [Part B]》1977,71(2):451-454
We present final results of a sensitive search for new particles in π±K? effective mass spectra observed in proton-nucleus collisions at 400 GeV/c. We establish a limit for D0 (1.865) production Bπ+π? dσ/dy < 360 nb/nucleon at ycm≈ ?0.4. For D?0 → π?K+ the limit is 290 nb/nucleon. 相似文献
18.
C.E.W. Ward I. Ambats A. Lesnik W.T. Meyer D.R. Rust D.D. Yovanovitch 《Physics letters. [Part B]》1974,48(5):471-473
We have measured the Λ° polarization in π?p→ K°Λ° at 5 GeV/c, using a data sample of 3709 events. The polarization is positive for small t, passes through zero near t = ?0.3 (GeV/c)2, and becomes large and negative at larger t, consistent with a value of ?1.0 for t between ?0.7 and ?1.6(GeV/c)2. 相似文献
19.
P. S. Auchincloss R. Blair C. Haber E. Oltman W. C. Leung M. Ruiz S. R. Mishra P. Z. Quintas F. J. Sciulli M. H. Shaevitz W. H. Smith F. S. Merritt M. Oreglia P. Reutens R. Coleman H. E. Fisk D. Levinthal D. D. Yovanovitch W. Marsh P. A. Rapidis H. B. White A. Bodek F. Borcherding N. Giokaris K. Lang I. E. Stockdale 《Zeitschrift fur Physik C Particles and Fields》1990,48(3):411-431
This paper reports on measurements of the total cross section for the inclusive reaction vμ+N , as a function of incident energy. Neutrinos and antineutrinos with energy in the range 30–300 GeV were produced in the 1982 Fermilab narrow-band neutrino beamline. A total of 35 000 neutrino and 7000 antineutrino interactions were recorded in the CCFR detector located in LabE. The incident neutrino flux was determined by methods similar to those used in previous experiments. The rate of increase with energy of the total cross section (σ/E v) in the range 30 to 75 GeV was determined to be 0.659±0.005(stat)±0.039(syst)×10?38 cm2/GeV and 0.307±0.008(stat)±0.020(syst)×10?38 cm2/GeV for incident neutrinos and antineutrinos, respectively. The 5.9% systematic errors are due primarily to uncertainties in the flux intensity measurement. The energy dependence of the cross section in the regionE ν=100–300 GeV was found to be linear, as determined by relative normalization techniques. A weighted average of our previous and present measurement for the total ν-N cross section yields: $$\begin{gathered} \sigma (vN) = 0.666 \pm 0.020(statistical \hfill \\ + systematic)E_v 10^{ - 38} cm^2 ; \hfill \\ \sigma (\bar vN) = 0.324 \pm 0.014(statistical \hfill \\ + systematic)E_v 10^{ - 38} cm^2 ; \hfill \\ \end{gathered} $$ . 相似文献
20.
Foudas C Bachmann KT Bernstein RH Blair RE Lefmann WC Leung WC Mishra SR Oltman E Quintas PZ Sciulli FJ Shaevitz MH Smith WH Merritt FS Oreglia MJ Schellman H Schumm BA Borcherding F Fisk HE Lamm MJ Marsh W Merritt KW Yovanovitch DD Bodek A Budd HS Sakumoto WK 《Physical review letters》1990,64(11):1207-1210