A. Galindo-Uribarri
Oak Ridge National Laboratory
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Featured researches published by A. Galindo-Uribarri.
Advances in High Energy Physics | 2014
N. Abgrall; E. Aguayo; Frank T. Avignone; A. S. Barabash; F. E. Bertrand; Melissa Boswell; V. Brudanin; M. Busch; A. S. Caldwell; Y.D. Chan; C. D. Christofferson; D. C. Combs; J. A. Detwiler; P. J. Doe; Y. V. Efremenko; V. Egorov; H. Ejiri; S. R. Elliott; J. Esterline; J. E. Fast; P. Finnerty; F. M. Fraenkle; A. Galindo-Uribarri; G. K. Giovanetti; J. Goett; M. P. Green; J. Gruszko; V. E. Guiseppe; K. Gusev; A. L. Hallin
The MAJORANA DEMONSTRATOR will search for the neutrinoless double-beta decay of the isotope Ge with a mixed array of enriched and natural germanium detectors. The observation of this rare decay would indicate that the neutrino is its own antiparticle, demonstrate that lepton number is not conserved, and provide information on the absolute mass scale of the neutrino. The DEMONSTRATOR is being assembled at the 4850-foot level of the Sanford Underground Research Facility in Lead, South Dakota. The array will be situated in a low-background environment and surrounded by passive and active shielding. Here we describe the science goals of the DEMONSTRATOR and the details of its design.
Science | 2017
D. Akimov; J. B. Albert; P. An; C. Awe; P.S. Barbeau; B. Becker; V. Belov; A. Brown; A. Bolozdynya; B. Cabrera-Palmer; M. Cervantes; J. I. Collar; R. J. Cooper; R.L. Cooper; C. Cuesta; D.J. Dean; J. A. Detwiler; A. Eberhardt; Y. V. Efremenko; S. R. Elliott; E. M. Erkela; L. Fabris; M. Febbraro; N. Fields; W. Fox; Z. Fu; A. Galindo-Uribarri; M. P. Green; M. Hai; M.R. Heath
A 14.6-kilogram sodium-doped CsI scintillator is used to detect a neutrino scattering process with a 6.7σ confidence level. Nailing down an elusive process Detecting neutrinos—elementary particles that barely interact with other matter—usually requires detectors of enormous size. A particular interaction of neutrinos with atomic nuclei, called the coherent elastic neutrino-nucleus scattering (CEνNS), is predicted to occur with relatively high probability, and it could be used to drastically reduce the size of neutrino detectors. However, observing this interaction requires a source of low-energy neutrinos and detectors that contain nuclei of optimal mass. Akimov et al. observed CEνNS with a 6.7σ confidence by using a comparatively tiny, 14.6-kg sodium-doped CsI scintillator exposed to neutrinos from a spallation neutron facility (see the Perspective by Link). The discovery places tighter bounds on exotic, beyond-the-standard-model interactions involving neutrinos. Science, this issue p. 1123; see also p. 1098 The coherent elastic scattering of neutrinos off nuclei has eluded detection for four decades, even though its predicted cross section is by far the largest of all low-energy neutrino couplings. This mode of interaction offers new opportunities to study neutrino properties and leads to a miniaturization of detector size, with potential technological applications. We observed this process at a 6.7σ confidence level, using a low-background, 14.6-kilogram CsI[Na] scintillator exposed to the neutrino emissions from the Spallation Neutron Source at Oak Ridge National Laboratory. Characteristic signatures in energy and time, predicted by the standard model for this process, were observed in high signal-to-background conditions. Improved constraints on nonstandard neutrino interactions with quarks are derived from this initial data set.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2000
C. J. Gross; Thomas Nelson Ginter; D. Shapira; W.T. Milner; J. W. McConnell; A.N. James; J.W. Johnson; J. F. Mas; P.F. Mantica; R.L. Auble; J.J. Das; J.L. Blankenship; Jonathan H. Hamilton; R.L. Robinson; Y.A. Akovali; C. Baktash; J. C. Batchelder; Carrol R Bingham; M.J. Brinkman; H.K. Carter; R.A. Cunningham; Thomas Davinson; J.D. Fox; A. Galindo-Uribarri; R. Grzywacz; J.F. Liang; B. D. MacDonald; Jim MacKenzie; S.D. Paul; A. Piechaczek
The recently commissioned Recoil Mass Spectrometer (RMS) at the Holifield Radioactive Ion Beam Facility (HRIBF) is described. Consisting of a momentum separator followed by an E-D-E Rochester-type mass spectrometer, the RMS is the centerpiece of the nuclear structure endstation at the HRIBF. Designed to transport ions with rigidities near K = 100, the RMS has acceptances of +/- 10% in energy and +/- 4.9% in mass-to-charge ratio. Recent experimental results are used to illustrate the detection capabilities of the RMS, which is compatible with many detectors and devices
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2016
N. Abgrall; I. J. Arnquist; F. T. Avignone; H. O. Back; A. S. Barabash; F. E. Bertrand; Melissa Boswell; A. W. Bradley; V. Brudanin; M. Busch; M. Buuck; D. Byram; A. S. Caldwell; Y.D. Chan; C. D. Christofferson; Pinghan Chu; C. Cuesta; J. A. Detwiler; J. A. Dunmore; Yu. Efremenko; H. Ejiri; S. R. Elliott; P. Finnerty; A. Galindo-Uribarri; V. M. Gehman; T. Gilliss; G. K. Giovanetti; J. Goett; M. P. Green; J. Gruszko
Abstract The Majorana collaboration is constructing the Majorana Demonstrator at the Sanford Underground Research Facility at the Homestake gold mine, in Lead, SD. The apparatus will use Ge detectors, enriched in isotope 76 Ge, to demonstrate the feasibility of a large-scale Ge detector experiment to search for neutrinoless double beta decay. The long half-life of this postulated process requires that the apparatus be extremely low in radioactive isotopes whose decays may produce backgrounds to the search. The radioassay program conducted by the collaboration to ensure that the materials comprising the apparatus are sufficiently pure is described. The resulting measurements from gamma-ray counting, neutron activation and mass spectroscopy of the radioactive-isotope contamination for the materials studied for use in the detector are reported. We interpret these numbers in the context of the expected background for the experiment.
arXiv: Instrumentation and Detectors | 2017
N. Abgrall; A. Abramov; N. Abrosimov; I. Abt; M. Agostini; M. Agartioglu; A. Ajjaq; S. I. Alvis; F. T. Avignone; X. Bai; M. Balata; I. Barabanov; A. S. Barabash; P. J. Barton; L. Baudis; L. Bezrukov; T. Bode; A. Bolozdynya; D. Borowicz; A. J. Boston; H. Boston; S. T.P. Boyd; R. Breier; V. Brudanin; R. Brugnera; M. Busch; M. Buuck; A. Caldwell; T. S. Caldwell; T. Camellato
The observation of neutrinoless double-beta decay (0νββ) would show that lepton number is violated, reveal that neu-trinos are Majorana particles, and provide information on neutrino mass. A discovery-capable experiment covering the inverted ordering region, with effective Majorana neutrino masses of 15 - 50 meV, will require a tonne-scale experiment with excellent energy resolution and extremely low backgrounds, at the level of ∼0.1 count /(FWHM·t·yr) in the region of the signal. The current generation 76Ge experiments GERDA and the Majorana Demonstrator, utilizing high purity Germanium detectors with an intrinsic energy resolution of 0.12%, have achieved the lowest backgrounds by over an order of magnitude in the 0νββ signal region of all 0νββ experiments. Building on this success, the LEGEND collaboration has been formed to pursue a tonne-scale 76Ge experiment. The collaboration aims to develop a phased 0νββ experimental program with discovery potential at a half-life approaching or at 1028 years, using existing resources as appropriate to expedite physics results.
arXiv: Instrumentation and Detectors | 2015
D. Akimov; A. Sosnovchev; J. I. Collar; S. Penttila; S. Suchyta; W. Lu; M. P. Green; P. An; R. Tayloe; R.T. Thornton; D. Rudik; A. Melikyan; N. Fields; L. J. Kaufman; A. Khromov; W.M. Snow; A. V. Kumpan; P. Naumov; B. Suh; A. Konovalev; K. Miller; N. Herman; A. Burenkov; B. Cabrera-Palmer; J. Newby; B. Becker; S. Hedges; A. Bolozdynya; A. Tolstukhin; K. Vetter
The COHERENT collaborations primary objective is to measure coherent elastic neutrino-nucleus scattering (CEvNS) using the unique, high-quality source of tens-of-MeV neutrinos provided by the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory (ORNL). In spite of its large cross section, the CEvNS process has never been observed, due to tiny energies of the resulting nuclear recoils which are out of reach for standard neutrino detectors. The measurement of CEvNS has now become feasible, thanks to the development of ultra-sensitive technology for rare decay and weakly-interacting massive particle (dark matter) searches. The CEvNS cross section is cleanly predicted in the standard model; hence its measurement provides a standard model test. It is relevant for supernova physics and supernova-neutrino detection, and enables validation of dark-matter detector background and detector-response models. In the long term, precision measurement of CEvNS will address questions of nuclear structure. COHERENT will deploy multiple detector technologies in a phased approach: a 14-kg CsI[Na] scintillating crystal, 15 kg of p-type point-contact germanium detectors, and 100 kg of liquid xenon in a two-phase time projection chamber. Following an extensive background measurement campaign, a location in the SNS basement has proven to be neutron-quiet and suitable for deployment of the COHERENT detector suite. The simultaneous deployment of the three COHERENT detector subsystems will test the
arXiv: Instrumentation and Detectors | 2017
S. R. Elliott; B. R. Jasinski; S. Mertens; N. Abgrall; K. Vetter; R. Henning; S. Vasilyev; J. Gruszko; R. G. H. Robertson; E. Romero-Romero; B. Shanks; K. Rielage; M. F. Kidd; M. Shirchenko; V. Brudanin; G. K. Giovanetti; E. W. Hoppe; A. W. P. Poon; A. Fullmer; A. M. Suriano; Richard T. Kouzes; B. R. White; J. E. Trimble; Yu. Efremenko; S. J. Meijer; A. Galindo-Uribarri; H. Ejiri; J. MacMullin; C. Wiseman; Howe
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Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2015
N. Abgrall; E. Aguayo; F. T. Avignone; A. S. Barabash; F. E. Bertrand; V. Brudanin; M. Busch; D. Byram; A. S. Caldwell; Y-D. Chan; C. D. Christofferson; D. C. Combs; C. Cuesta; J. A. Detwiler; P. J. Doe; Yu. Efremenko; V. Egorov; H. Ejiri; S. R. Elliott; J. Esterline; J. E. Fast; P. Finnerty; F. M. Fraenkle; A. Galindo-Uribarri; G. K. Giovanetti; J. Goett; M. P. Green; J. Gruszko; V. E. Guiseppe; K. Gusev
dependence of the cross section and ensure an unambiguous discovery of CEvNS. This document describes concisely the COHERENT physics motivations, sensitivity and plans for measurements at the SNS to be accomplished on a four-year timescale.
arXiv: Instrumentation and Detectors | 2017
J. Gruszko; N. Abgrall; I. J. Arnquist; F. T. Avignone; A. S. Barabash; F. E. Bertrand; A. W. Bradley; Brudanin; M. Busch; M. Buuck; T. S. Caldwell; Y.D. Chan; C. D. Christofferson; P.-H. Chu; C. Cuesta; J. A. Detwiler; C. Dunagan; Y.-U. Efremenko; H. Ejiri; S. R. Elliott; A. Fullmer; A. Galindo-Uribarri; T. Gilliss; G. K. Giovanetti; M. P. Green; I. S. Guinn; V. E. Guiseppe; R. Henning; E. W. Hoppe; M. A. Howe
Author(s): Elliott, SR; Abgrall, N; Arnquist, IJ; Avignone, FT; Barabash, AS; Bertrand, FE; Bradley, AW; Brudanin, V; Busch, M; Buuck, M; Caldwell, TS; Chan, YD; Christofferson, CD; Chu, PH; Cuesta, C; Detwiler, JA; Dunagan, C; Efremenko, Y; Ejiri, H; Fullmer, A; Galindo-Uribarri, A; Gilliss, T; Giovanetti, GK; Green, MP; Gruszko, J; Guinn, IS; Guiseppe, VE; Henning, R; Hoppe, EW; Howe, MA; Jasinski, BR; Keeter, KJ; Kidd, MF; Konovalov, SI; Kouzes, RT; Leon, J; Lopez, AM; Macmullin, J; Martin, RD; Massarczyk, R; Meijer, SJ; Mertens, S; Orrell, JL; OShaughnessy, C; Poon, AWP; Radford, DC; Rager, J; Rielage, K; Robertson, RGH; Romero-Romero, E; Shanks, B; Shirchenko, M; Suriano, AM; Tedeschi, D; Trimble, JE; Varner, RL; Vasilyev, S; Vetter, K; Vorren, K; White, BR; Wilkerson, JF; Wiseman, C; Xu, W; Yakushev, E; Yu, CH; Yumatov, V; Zhitnikov, I | Abstract:
arXiv: Instrumentation and Detectors | 2015
S. Mertens; N. Abgrall; F. T. Avignone; A. S. Barabash; F. E. Bertrand; V. Brudanin; M. Busch; M. Buuck; D. Byram; A. S. Caldwell; Y.D. Chan; C. D. Christofferson; C. Cuesta; J. A. Detwiler; Yu. Efremenko; H. Ejiri; S. R. Elliott; A. Galindo-Uribarri; G. K. Giovanetti; J. Goett; M. P. Green; J. Gruszko; I. S. Guinn; V. E. Guiseppe; R. Henning; E. W. Hoppe; S. Howard; M. A. Howe; B. R. Jasinski; K. Keeter
The Majorana Demonstrator is an ultra-low background physics experiment searching for the neutrinoless double beta decay of 76 Ge. The Majorana Parts Tracking Database is used to record the history of components used in the construction of the Demonstrator. The tracking implementation takes a novel approach based on the schema-free database technology CouchDB. Transportation, storage, and processes undergone by parts such as machining or cleaning are linked to part records. Tracking parts provides a great logistics benefit and an important quality a ssurance reference during construction. In addition, the l ocation history of parts provides an estimate of their exposure to cosmic radiation. A web application for data entry and a radiation exposure calculator have been developed as tools for achieving the extreme radio-purity required for this rare decay search.