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Dive into the research topics where E. Hungerford is active.

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Featured researches published by E. Hungerford.


Physical Review Letters | 1999

New limit for the family number nonconserving decay mu+ ---> e+ gamma

M.L. Brooks; A. Empl; W. von Witsch; X.L. Tu; S.C. Wright; L. A. Van Ausdeln; K. Lan; R. Manweiler; Y. Chen; Kroupa; Cooper; J. J. Szymanski; L. E. Piilonen; C. A. Gagliardi; B. Mayes; K. O. H. Ziock; D. D. Koetke; E.B. Hughes; T. D. S. Stanislaus; G. E. Hogan; R. E. Mischke; J. E. Knott; E. Hungerford; K. M. Stantz; Peter S. Cooper; M. Dzemidzic; C. C. H. Jui; R. E. Tribble

The transport properties of a quasi-three-dimensional, 200 layer quantum well structure are investigated at integer filling in the quantum Hall state. We find that the transverse magnetoresistance R xx , the Hall resistance R xy , and the vertical resistance R zz all follow a similar behavior with both temperature and in-plane magnetic field. A general feature of the influence of increasing in-plane field B in is that the Hall conductance quantization first improves, but above a characteristic value B C in , the quantization is systematically removed. We consider the interplay of the chid edge state transport and the bulk (quantum Hall) transport properties. This mechanism may arise from the competition of the cyclotron energy with the superlattice band structure energies. A comparison of the resuIts with existing theories of the chiral edge state transport with in-plane field is also discussed.An experiment has been performed to search for the muon- and electron-number non-conserving decay mu+ to e+_gamma. The upper limit for the branching ratio to be GAMMA(mu+ to e+_gamma)/GAMMA(mu+ to e+_nu_nubar) < 1.2e-11 with 90% confidence.


Physics Letters B | 2013

Measurement of geo-neutrinos from 1353 days of Borexino

G. Bellini; J. Benziger; D. Bick; G. Bonfini; D. Bravo; M. Buizza Avanzini; B. Caccianiga; L. Cadonati; F. Calaprice; P. Cavalcante; A. Chavarria; A. Chepurnov; D. D'Angelo; S. Davini; A. Derbin; A. Empl; A. Etenko; G. Fiorentini; K. Fomenko; D. Franco; C. Galbiati; S. Gazzana; C. Ghiano; M. Giammarchi; M. Goeger-Neff; A. Goretti; L. Grandi; C. Hagner; E. Hungerford; Aldo Ianni

Abstract We present a measurement of the geo-neutrino signal obtained from 1353 days of data with the Borexino detector at Laboratori Nazionali del Gran Sasso in Italy. With a fiducial exposure of ( 3.69 ± 0.16 ) × 10 31 proton × year after all selection cuts and background subtraction, we detected ( 14.3 ± 4.4 ) geo-neutrino events assuming a fixed chondritic mass Th/U ratio of 3.9. This corresponds to a geo-neutrino signal S geo = ( 38.8 ± 12.0 ) TNU with just a 6 × 10 − 6 probability for a null geo-neutrino measurement. With U and Th left as free parameters in the fit, the relative signals are S Th = ( 10.6 ± 12.7 ) TNU and S U = ( 26.5 ± 19.5 ) TNU . Borexino data alone are compatible with a mantle geo-neutrino signal of ( 15.4 ± 12.3 ) TNU , while a combined analysis with the KamLAND data allows to extract a mantle signal of ( 14.1 ± 8.1 ) TNU . Our measurement of 31.2 − 6.1 + 7.0 reactor anti-neutrino events is in agreement with expectations in the presence of neutrino oscillations.


Journal of High Energy Physics | 2013

SOX: Short distance neutrino Oscillations with BoreXino

G. Bellini; D. Bick; G. Bonfini; D. Bravo; B. Caccianiga; F. Calaprice; A. Caminata; P. Cavalcante; A. Chavarria; A. Chepurnov; D. D’Angelo; S. Davini; A. Derbin; A. Etenko; G. Fernandes; K. Fomenko; D. Franco; C. Galbiati; C. Ghiano; M. Göger-Neff; A. Goretti; C. Hagner; E. Hungerford; Aldo Ianni; Andrea Ianni; V. Kobychev; D. Korablev; G. Korga; D. Krasnicky; D. Kryn

A bstractThe very low radioactive background of the Borexino detector, its large size, and the well proved capability to detect both low energy electron neutrinos and antineutrinos make an ideal case for the study of short distance neutrino oscillations with artificial sources at Gran Sasso.This paper describes the possible layouts of 51Cr (νe) and 144Ce-144Pr


Physics Letters B | 1982

Experimental observation of the Σ hypernuclei, Σ6H and Σ16C

H. Piekarz; S. Bart; R. Hackenburg; A.D. Hancock; E. Hungerford; B. Mayes; K. Sekharan; J. Piekarz; M. Deutsch; R.E. Chrien; S. Chen; M. J. Levine; D. Maurizio; M. May; H. Palevsky; Y. Xu; Peter D. Barnes; B. Basslleck; R. Eisenstein; R. Grace; C. J. Maher; P. Pile; R. Rieder; W. Wharton; R. L. Stearns


Physics Letters B | 1979

States of

R.E. Chrien; M. May; Daniel Marlow; F. Takeutchi; Moshe Deutsch; L. Pinsky; R. L. Stearns; T. M. Williams; E. Hungerford; R. Cester; Peter D. Barnes; R. Sutter; H. Palevsky; S. A. Dytman; S. Bart; B. Mayes

\left( {{{\overline{\nu}}_e}} \right)


Nuclear Physics | 1988

^{12}

Robert E. Chrien; P. Pile; R. E. Chrien; S. Bart; R. Sutter; N. Tsoupas; J. C. Peng; S. Mishra; T. Kishimoto; Liguang Tang; Z. Xu; W. von Witsch; E. Hungerford; K. Maeda; D. R. Gill; R. L. Stearns; B. Quinn; R. McCrady; J. Seydoux; H. Plendl; J. Reidy


Journal of Cosmology and Astroparticle Physics | 2013

C (

G. Bellini; J. Benziger; D. Bick; G. Bonfini; D. Bravo; M. Buizza Avanzini; B. Caccianiga; L. Cadonati; F. Calaprice; P. Cavalcante; A. Chavarria; A. Chepurnov; D. D'Angelo; S. Davini; A. Derbin; A. Empl; A. Etenko; K. Fomenko; D. Franco; C. Galbiati; S. Gazzana; C. Ghiano; M. Giammarchi; M. Göger-Neff; A. Goretti; L. Grandi; C. Hagner; E. Hungerford; Aldo Ianni; Andrea Ianni

source experiments in Borexino and shows the expected sensitivity to eV mass sterile neutrinos for three possible different phases of the experiment. Expected results on neutrino magnetic moment, electroweak mixing angle, and couplings to axial and vector currents are shown too.


Given at | 1998

\Lambda

S. Ajimura; E. Hungerford; M. Sekimoto; T.-A. Shibata; H. Tanida; T. Nagae; K. Omata; K. Aoki; Yasuhiro Ohta; H. Outa; Hyun Park; K. Koshino; Y. Saito; H. Bhang; M. Youn; L. Tang; Tadafumi Kishimoto; H. Tamura; T. Endo; K. Kubota; T. Tamagawa; Y. D. Kim; T. Saito; H. Hotchi; J.H. Kim; H. Noumi; O. Hashimoto; Y. Fujii; K. Maeda; T. Takahashi

Abstract The hypernuclei Σ 6 H and Σ 16 C were observed by the (K − , π + ) reaction on targets of 6 Li and liquid O, respectively, at 713 MeV/ c incident K − momentum. Structure is seen in Σ 6 H which may be interpreted in terms of particle-hole excitations similar to the previously observed states in Λ 6 Li. The inablitity to resolve individual Σ hypernuclear levels in Σ 16 C, due in part to the excitation of non-coherent states as a result of the large momentum transfer of about 130 MeV/ c , precludes the extraction of the Σ-nucleus spin-orbit potential strength. The Σ-nucleus well depth appears to be 7 to 10 MeV less than that for the Λ.


Nuclear Physics | 1997

) Formed in the Reaction

R. E. Chrien; R. Sawafta; R.J. Peterson; R.A. Michael; E. Hungerford

Abstract States of 12 Λ C formed in the (K − , π − ) reaction have been studied for momentum transfers up to 260 MeV/ c , using an incident K − beam of 800 MeV/ c momentum. The angular distributions for the g.s. and for a peak at 11 meV have been measured between 0° and 19° in the laboratory. Limits on the splitting of the 11 MeV peak and on the formation of low-lying excited states are given.


Physics Letters B | 1996

^{12}

R.A. Michael; M.B. Barakat; S. Bart; R.E. Chrien; B.C. Clark; D.J. Ernst; S. Hama; K. Hicks; Wendy L. Hinton; E. Hungerford; M.F. Jiang; T. Kishimoto; C.M. Kormanyos; L.J. Kurth; L. Lee; B. Mayes; R.J. Peterson; L. Pinsky; R. Sawafta; R. Sutter; L. Tang; J.E. Wise

Abstract The spectroscopy of hypernuclei across a wide range of mass number has been studies by the associated production (π+, K+) technique. The energies of Λ single particle states in the s, p, d, and f shells have been determinedas a function of A. It is demonstrated that the (π+, K+) reaction is the method of choice for studying Λ-bound levels of hypernuclei.

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L. Pinsky

University of Houston

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S. Bart

University of Houston

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S. Davini

University of Houston

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K. Fomenko

Joint Institute for Nuclear Research

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A. Empl

University of Houston

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