R. L. Brodzinski
Pacific Northwest National Laboratory
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Featured researches published by R. L. Brodzinski.
Physical Review D | 2002
E. García; J. Puimedón; V.S. Pogosov; J. Morales; Walter K. Hensley; A.A. Vasenko; I.G. Irastorza; A.A. Smolnikov; J.H. Reeves; I.V. Kirpichnikov; S. Cebrián; S.B. Osetrov; Harry S. Miley; F. T. Avignone; J.A. Villar; A. Morales; A.S. Starostin; A.G. Tamanyan; R. L. Brodzinski; A.A. Klimenko; S.I. Vasilev; D. González; A. Ortiz de Solórzano; M.L. Sarsa
The International Germanium Experiment (IGEX) has analyzed 117 mole yr of 76Ge data from its isotopically enriched (86% 76Ge) germanium detectors. Applying pulse-shape discrimination (PSD) to the more recent data, the lower bound on the half-life for neutrinoless double-beta decay of 76Ge is:
Modern Physics Letters A | 2002
Frank T. Avignone; A. S. Barabash; F. Boehm; R. L. Brodzinski; J. I. Collar; P. J. Doe; H. Ejiri; Stephen R. Elliott; E. Fiorini; R.J. Gaitskell; G. Gratta; R. Hazama; K. Kazkaz; G. S. King; Richard T. Kouzes; Harry S. Miley; M. Moe; A. Morales; J. Morales; A. Piepke; R. G. H. Robertson; W. Tornow; P. G. Vogel; Ray A. Warner; J. F. Wilkerson
T_{1/2}(0\nu)> 1.57 \times 10^{25}
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1999
K. Zioutas; C.E. Aalseth; D. Abriola; Frank T. Avignone; R. L. Brodzinski; J. I. Collar; Richard J. Creswick; D. E. Di Gregorio; Horacio A. Farach; A. O. Gattone; C.K. Guerard; F. Hasenbalg; M. Hasinoff; H. Huck; A. Liolios; Harry S. Miley; A. Morales; J. Morales; D. Nikas; Shmuel Nussinov; A. Ortiz; E. Savvidis; S. Scopel; Peter Sievers; J.A. Villar; L. Walckiers
yr (90% C.L.). This corresponds to an upper bound in the Majorana neutrino mass parameter,
Astroparticle Physics | 2002
A. Morales; Frank T. Avignone; R. L. Brodzinski; S. Cebrián; E. García; D. González; I.G. Irastorza; Harry S. Miley; J. Morales; A. Ortiz de Solórzano; J. Puimedón; J.H. Reeves; M.L. Sarsa; S. Scopel; J.A. Villar
Physics Letters B | 1991
F. T. Avignone; R. L. Brodzinski; C.K. Guerard; I.V. Kirpichnikov; Harry S. Miley; V.S. Pogosov; J.H. Reeves; A.S. Starostin; A.G. Tamanyan
, between 0.33 eV and 1.35 eV, depending on the choice of theoretical nuclear matrix elements used in the analysis.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1990
R. L. Brodzinski; Harry S. Miley; J.H. Reeves; F. T. Avignone
We comment on the recent claim for the experimental observation of neutrinoless double-beta decay. We discuss several limitations in the analysis provided in that paper and conclude that there is no basis for the presented claim.
Physics Letters B | 2000
A. Morales; C.E. Aalseth; Frank T. Avignone; R. L. Brodzinski; S. Cebrián; E. García; D. González; W. K. Hensley; I.G. Irastorza; I.V. Kirpichnikov; A.A. Klimenko; Harry S. Miley; J. Morales; A. Ortiz de Solórzano; S.B. Osetrov; V.S. Pogosov; J. Puimedón; J.H. Reeves; M.L. Sarsa; S. Scopel; A.A. Smolnikov; A.G. Tamanyan; A.A. Vasenko; S.I. Vasiliev; J.A. Villar
The 8.4 T, 10 m long transverse magnetic field of a twin aperture LHC bending magnet can be utilized as a macroscopic coherent solar axion-to-photon converter. Numerical calculations show that the integrated time of alignment with the Sun would be 33 days/yr with the magnet on a tracking table capable of
Physics of Atomic Nuclei | 2000
C.E. Aalseth; F. T. AvignoneIII; R. L. Brodzinski; S. Cebrián; D. Gonzáles; E. García; W. K. Hensley; I.G. Irastorza; I.V. Kirpichnikov; A. A. Klimenko; Harry S. Miley; A. Morales; J. Morales; A. Ortiz de Solórzano; S.B. Osetrov; V.S. Pogosov; J. Puimedón; J.H. Reeves; M.L. Sarsa; S. Scopel; A.A. Smolnikov; A.S. Starostin; A.G. Tamanyan; A.A. Vasenko; S.I. Vasiliev; J.A. Villar
5i in the vertical direction and
Physics of Atomic Nuclei | 2004
Dale N. Anderson; R. Arthur; Frank T. Avignone; C. Baktash; T. Ball; A. S. Barabash; R. L. Brodzinski; V. Brudanin; W. Bugg; A.E. Champagne; Y.D. Chan; T.V. Cianciolo; J. I. Collar; R. W. Creswick; P. J. Doe; G. Dunham; S. Easterday; Yu. Efremenko; V. Egorov; H. Ejiri; S. R. Elliott; J. Ely; P. Fallon; Horacio A. Farach; R.J. Gaitskell; V. Gehman; R. Grzywacz; R. Hazma; H. Hime; T. Hossbach
40i in the horizontal direction. The existing lower bound on the axion-to-photon coupling constant can be improved by a factor between 30 and 100 in 3 yr, i.e., g !cc [9]10~11 GeV~1 for axion masses [ 1 eV. This value falls within the existing open axion mass window. The same set-up can simultaneously search for low- and high-energy celestial axions, or axion-like particles, scanning the sky as the Earth rotates and orbits the Sun. ( 1999 Elsevier Science B.V. All rights reserved.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2003
D. González; J. Morales; S. Cebrián; E. García; I.G. Irastorza; A. Morales; A. Ortiz de Solórzano; J. Puimedón; M.L. Sarsa; J.A. Villar; C.E. Aalseth; F. T. Avignone; R. L. Brodzinski; Walter K. Hensley; Harry S. Miley; J.H. Reeves; I.V. Kirpichnikov; A.A. Vasenko; A.A. Klimenko; S.B. Osetrov; A.A. Smolnikov; S.I. Vasiliev; V.S. Pogosov; A.G. Tamanyan
Abstract A small, natural abundance, germanium detector (COSME) has been operating recently at the Canfranc Underground Laboratory (Spanish Pyrenees) in improved conditions of shielding and overburden with respect to a previous operation of the same detector (Nucl. Instrum. Meth. A 321 (1992) 410; Phys. Rev. D 51 (1995) 1458). An exposure of 72.7 kg day in these conditions has at present a background improvement of about one order of magnitude compared to the former operation of the detector. These new data have been applied to a direct search for weakly interacting massive particles (WIMPs) and solar axions. New WIMP exclusion plots improving the current bounds for low masses are reported. The paper also presents a limit on the axion–photon coupling obtained from the analysis of the data looking for a Primakoff axion-to-photon conversion and Bragg scattering inside the crystal.