A. K. Cochran
Southern University and A&M College
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Featured researches published by A. K. Cochran.
Physical Review D | 2001
A. Aguilar-Arevalo; W. Metcalf; S. Yellin; R. Imlay; E. D. Church; R. Tayloe; G. J. VanDalen; R. L. Burman; A. Malik; L. Auerbach; W. Vernon; G. B. Mills; J. B. Donahue; I. Stancu; David O. Caldwell; N. Wadia; David Smith; W.C. Louis; D. H. White; M. Sung; A. K. Cochran; R. M. Gunasingha; R. Majkic; G. T. Garvey; A. R. Fazely; V. Sandberg
A search for muon anti-neutrino to electron anti-neutrino oscillations was conducted by the Liquid Scintillator Neutrino Detector at the Los Alamos Neutron Science Center using muon anti-neutrinos from positive muon decay at rest. A total excess of 87.9 +/- 22.4 +/- 6.0 events consistent with electron anti-neutrino plus proton scattering to positron plus neutron was observed above the expected background. This excess corresponds to an oscillation probability of (0.264 +/- 0.067 +/- 0.045), which is consistent with an earlier analysis. In conjunction with other known limits on neutrino oscillations, the LSND data suggest that neutrino oscillations occur in the 0.2-10 eV^2/c^4 Delta-m^2 range, indicating a neutrino mass greater than 0.4 eV/c^2.
Physical Review D | 2001
A. Aguilar; L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; W. C. Louis; R. Majkic; A. Malik; W. Metcalf; G. B. Mills; V. Sandberg; David Smith; I. Stancu; M. Sung; R. Tayloe; G. J. VanDalen; W. Vernon; N. Wadia; D. H. White; S. Yellin
A search for muon anti-neutrino to electron anti-neutrino oscillations was conducted by the Liquid Scintillator Neutrino Detector at the Los Alamos Neutron Science Center using muon anti-neutrinos from positive muon decay at rest. A total excess of 87.9 +/- 22.4 +/- 6.0 events consistent with electron anti-neutrino plus proton scattering to positron plus neutron was observed above the expected background. This excess corresponds to an oscillation probability of (0.264 +/- 0.067 +/- 0.045), which is consistent with an earlier analysis. In conjunction with other known limits on neutrino oscillations, the LSND data suggest that neutrino oscillations occur in the 0.2-10 eV^2/c^4 Delta-m^2 range, indicating a neutrino mass greater than 0.4 eV/c^2.
Physical Review D | 2005
L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; T. Katori; W. C. Louis; K. McIlhany; W. Metcalf; G. B. Mills; V. Sandberg; D. Smith; I. Stancu; W. Strossman; R. Tayloe; M. Sung; W. Vernon; D. H. White; S. Yellin
A recently developed Standard-Model Extension (SME) formalism for neutrino oscillations that includes Lorentz and CPT violation is used to analyze the sidereal time variation of the neutrino event excess measured by the Liquid Scintillator Neutrino Detector (LSND) experiment. The LSND experiment, performed at Los Alamos National Laboratory, observed an excess, consistent with neutrino oscillations, of
Physical Review Letters | 2004
L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; G. Kahrimanis; W. C. Louis; R. Majkic; A. Malik; K. McIlhany; W. Metcalf; G. B. Mills; D. Rupnik; V. Sandberg; David Smith; R. F. Somodi; I. Stancu; W. D. Strossman; M. Sung; R. Tayloe; G. J. VanDalen; W. Vernon; N. Wadia; D. H. White; S. Yellin
{\bar\nu}_e
Physical Review D | 2005
L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; T. Katori; W. C. Louis; K. McIlhany; W. Metcalf; G. B. Mills; V. Sandberg; D. Smith; I. Stancu; W. Strossman; R. Tayloe; M. Sung; W. Vernon; D. H. White; S. Yellin
in a beam of
Physical Review D | 2005
L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; T. Katori; W. C. Louis; K. McIlhany; W. Metcalf; G. B. Mills; V. Sandberg; David Smith; I. Stancu; W. Strossman; R. Tayloe; M. Sung; W. Vernon; D. H. White; S. Yellin
{\bar\nu}_\mu
Physical Review Letters | 2004
L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; G. Kahrimanis; W. C. Louis; R. Majkic; A. Malik; K. McIlhany; W. Metcalf; G. B. Mills; D. Rupnik; V. Sandberg; David Smith; R. F. Somodi; I. Stancu; W. D. Strossman; M. Sung; R. Tayloe; G. J. VanDalen; W. Vernon; N. Wadia; D. H. White; S. Yellin
. It is determined that the LSND oscillation signal is consistent with no sidereal variation. However, there are several combinations of SME coefficients that describe the LSND data; both with and without sidereal variations. The scale of Lorentz and CPT violation extracted from the LSND data is of order
Physical Review Letters | 2003
L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; G. Kahrimanis; W. C. Louis; R. Majkic; A. Malik; K. McIlhany; W. Metcalf; G. B. Mills; D. Rupnik; V. Sandberg; David Smith; R. F. Somodi; I. Stancu; W. D. Strossman; M. Sung; R. Tayloe; G. J. VanDalen; W. Vernon; N. Wadia; D. H. White; S. Yellin
10^{-19}
Physical Review D | 2001
A. Aguilar; L. Auerbach; R. L. Burman; David O. Caldwell; E. D. Church; A. K. Cochran; J. B. Donahue; A. R. Fazely; G. T. Garvey; R. M. Gunasingha; R. Imlay; W. C. Louis; R. Majkic; A. Malik; W. Metcalf; G. B. Mills; V. Sandberg; David Smith; I. Stancu; M. Sung; R. Tayloe; G. J. VanDalen; W. Vernon; N. Wadia; D. H. White; S. Yellin
GeV for the SME coefficients
Physical Review D | 2005
L. Auerbach; R. L. Burman; J. B. Donahue; G. T. Garvey; W.C. Louis; G. B. Mills; Vernon D. Sandberg; D. H. White; David O. Caldwell; S. Yellin; E. D. Church; K. McIlhany; W. Strossman; A. K. Cochran; A. R. Fazely; R. M. Gunasingha; Richard Imlay; W. Metcalf; M. Sung; T. Katori
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