W. A. Teasdale
Los Alamos National Laboratory
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Featured researches published by W. A. Teasdale.
Physical Review C | 1999
J. N. Abdurashitov; V. N. Gavrin; S. V. Girin; V. V. Gorbachev; T. V. Ibragimova; A. V. Kalikhov; N. G. Khairnasov; T. V. Knodel; I. N. Mirmov; A. A. Shikhin; E. P. Veretenkin; V. M. Vermul; V. E. Yants; G. T. Zatsepin; T. J. Bowles; W. A. Teasdale; D. L. Wark; Michael L. Cherry; Jeffrey S. Nico; B. T. Cleveland; Raymond Davis; K. Lande; P. Wildenhain; S. R. Elliott; J. F. Wilkerson
The solar neutrino capture rate measured by the Russian-American Gallium Experiment (SAGE) on metallic gallium during the period January 1990 through December 1997 is 67.2 (+7.2-7.0) (+3.5-3.0) SNU, where the uncertainties are statistical and systematic, respectively. This represents only about half of the predicted Standard Solar Model rate of 129 SNU. All the experimental procedures, including extraction of germanium from gallium, counting of 71Ge, and data analysis are discussed in detail.
Physical Review C | 2009
J. N. Abdurashitov; V. N. Gavrin; V. V. Gorbachev; P. P. Gurkina; T. V. Ibragimova; A. V. Kalikhov; N. G. Khairnasov; T. V. Knodel; I. N. Mirmov; A. A. Shikhin; E. P. Veretenkin; V. E. Yants; G. T. Zatsepin; T. J. Bowles; S. R. Elliott; W. A. Teasdale; Jeffrey S. Nico; B. T. Cleveland; J. F. Wilkerson
The Russian-American experiment SAGE began to measure the solar neutrino capture rate with a target of gallium metal in December 1989. Measurements have continued with only a few brief interruptions since that time. In this article we present the experimental improvements in SAGE since its last published data summary in December 2001. Assuming the solar neutrino production rate was constant during the period of data collection, combined analysis of 168 extractions through December 2007 gives a capture rate of solar neutrinos with energy more than 233 keV of
Physics Letters B | 1994
J. N. Abdurashitov; E. L. Faizov; V. N. Gavrin; A.O. Gusev; A. V. Kalikhov; T. V. Knodel; I. I. Knyshenko; V. N. Kornoukhov; I. N. Mirmov; A.M. Pshukov; A.M. Shalagin; A. A. Shikhin; P. V. Timofeyev; E. P. Veretenkin; V. M. Vermul; G. T. Zatsepin; T. J. Bowles; J.S. Nico; W. A. Teasdale; D.L. Wark; J.F. Wilkerson; B.T. Cleveland; T. Daily; Raymond Davis; K. Lande; C.K. Lee; P.W. Wildenhain; S.R. Elliott; Michael L. Cherry; R.T. Kouzes
65.{4}_{\ensuremath{-}3.0}^{+3.1}
Physical Review C | 1998
J. N. Abdurashitov; V. V. Gorbachev; V. N. Gavrin; A. V. Zvonarev; I. N. Mirmov; John F. Wilkerson; B T. Cleveland; V. N. Kornoukhov; R. Davis; V. E. Yants; A. V. Kalikhov; Tatiana V. Ibragimova; W. A. Teasdale; Jeffrey S. Nico; V.N. Karaulov; A. A. Shikhin; E. P. Veretenkin; Yu. S. Khomyakov; D.L. Wark; K. Lande; S. R. Elliott; T.J. Bowels; V.I. Maev; V. S. Shkol'nik; C. K. Lee; N. V. Skorikov; T. Daily; V. M. Vermul; V.L. Levitin; P.I. Nazarenko
(stat)
Physical Review C | 1999
J. N. Abdurashitov; V. N. Gavrin; S. V. Girin; V. V. Gorbachev; T. V. Ibragimova; A. V. Kalikhov; N. G. Khairnasov; T. V. Knodel; V. N. Kornoukhov; I. N. Mirmov; A. A. Shikhin; E. P. Veretenkin; V. M. Vermul; V. E. Yants; G. T. Zatsepin; Yu. S. Khomyakov; A. V. Zvonarev; T. J. Bowles; J.S. Nico; W. A. Teasdale; D.L. Wark; Michael L. Cherry; V.N. Karaulov; V.L. Levitin; V.I. Maev; P.I. Nazarenko; V. S. Shkol’nik; N. V. Skorikov; B. T. Cleveland; T. Daily
{}_{\ensuremath{-}2.8}^{+2.6}
Physical Review C | 2000
L. J. Lising; Soo Ryong Hwang; Jonathan M. Adams; T. J. Bowles; Michael C. Browne; T. E. Chupp; Kevin Patrick Coulter; Maynard S. Dewey; Stuart J. Freedman; B. K. Fujikawa; Antonio Garcia; Geoffrey L. Greene; Gordon L. Jones; Hans Pieter Mumm; Jeffrey S. Nico; J. M. Richardson; R. G. H. Robertson; T.D. Steiger; W. A. Teasdale; Alan K. Thompson; E. G. Wasserman; F. E. Wietfeldt; Robert C. Welsh; J. F. Wilkerson
(syst) SNU. The weighted average of the results of all three Ga solar neutrino experiments, SAGE, Gallex, and GNO, is now
Physical Review C | 2006
J. N. Abdurashitov; V. I. Barsanov; T. J. Bowles; B. T. Cleveland; S. R. Elliott; V. N. Gavrin; S. V. Girin; V. V. Gorbachev; P. P. Gurkina; W. C. Haxton; T. V. Ibragimova; A. A. Janelidze; A. V. Kalikhov; A.I. Karpenko; N. G. Khairnasov; Yu. S. Khomyakov; T. V. Knodel; A. V. Korenkova; N. A. Kotelnikov; K. Lande; V.V. Maltsev; S. Yu. Markov; V. A. Matveev; I. N. Mirmov; O.V. Mishin; Jeffrey S. Nico; N.N. Oshkanov; V.M. Poplavsky; A. N. Petrov; V. V. Popov
66.1\ifmmode\pm\else\textpm\fi{}3.1
Physical Review Letters | 2002
C. L. Morris; Juan-Manuel Anaya; T. J. Bowles; B. W. Filippone; P. Geltenbort; R. Hill; Masahiro Hino; Seth Hoedl; Gary E. Hogan; Takeo Ito; T. Kawai; K. Kirch; S. K. Lamoreaux; C.-Y. Liu; M. Makela; L.J. Marek; Jonathan W. Martin; R.N. Mortensen; A. Pichlmaier; A. Saunders; S. J. Seestrom; D. Smith; W. A. Teasdale; Brian Tipton; Masahiko Utsuro; A. R. Young; Junhua Yuan
SNU, where statistical and systematic uncertainties have been combined in quadrature. During the recent period of data collection a new test of SAGE was made with a reactor-produced
Review of Scientific Instruments | 2013
A. Saunders; M. Makela; Y. Bagdasarova; H. O. Back; J. G. Boissevain; L. J. Broussard; T. J. Bowles; R. Carr; S. Currie; B. W. Filippone; Antonio Garcia; P. Geltenbort; K. P. Hickerson; Roger E. Hill; J. Hoagland; Seth Hoedl; A. T. Holley; Gary E. Hogan; Takeyasu M. Ito; S. K. Lamoreaux; Chen-Yu Liu; J. Liu; R. R. Mammei; Jeffrey William Martin; D. Melconian; M. P. Mendenhall; C. L. Morris; R. Mortensen; R. W. Pattie; M. L. Pitt
^{37}\mathrm{Ar}
Physical Review Letters | 2009
R. W. Pattie; J. Anaya; H. O. Back; J. G. Boissevain; T. J. Bowles; L. J. Broussard; R. Carr; D. J. Clark; S. Currie; S. Du; B. W. Filippone; P. Geltenbort; A. García; Ayman I. Hawari; K. P. Hickerson; R. Hill; M. Hino; S. A. Hoedl; G. E. Hogan; A. T. Holley; T. M. Ito; T. Kawai; K. Kirch; S. Kitagaki; S. K. Lamoreaux; C.-Y. Liu; J. Liu; M. Makela; R. R. Mammei; J. W. Martin
neutrino source. The ratio of observed to calculated rates in this experiment, combined with the measured rates in the three prior