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Featured researches published by S. Telfer.


Physical Review D | 2017

First search for a dark matter annual modulation signal with NaI(Tl) in the Southern Hemisphere by DM-Ice17

E. Barbosa de Souza; J. Cherwinka; A. Cole; A. C. Ezeribe; D. Grant; F. Halzen; K. M. Heeger; L. Hsu; A. J. F. Hubbard; J.H. Jo; A. Karle; M. Kauer; V.A. Kudryavtsev; K. E. Lim; Calum Michael Macdonald; Reina Maruyama; F. Mouton; S. M. Paling; W. Pettus; Z.P. Pierpoint; B. N. Reilly; M. Robinson; F.R. Rogers; P. Sandstrom; A. Scarff; N.J.C. Spooner; S. Telfer; L. Yang

The first search for a dark matter annual modulation signal with NaI(Tl) target material in the Southern Hemisphere conducted with the DM-Ice17 experiment is presented. DM-Ice17 consists of 17 kg of NaI(Tl) scintillating crystal under 2200 m.w.e. overburden of Antarctic glacial ice. The analysis presented here utilizes a 60.8 kg yr exposure. While unable to exclude the signal reported by DAMA/LIBRA, the DM-Ice17 data are consistent with no modulation in the energy range of 4-20 keV, providing the strongest limits on WIMP candidates from a direct detection experiment located in the Southern Hemisphere. Additionally, the successful deployment and stable operation of 17 kg of NaI(Tl) crystal over 3.5 years establishes the South Pole ice as a viable location for future underground, low-background experiments.


Journal of Instrumentation | 2014

Radon in the DRIFT-II directional dark matter TPC: emanation, detection and mitigation

James Battat; J. Brack; E. Daw; A. Dorofeev; A. C. Ezeribe; J. R. Fox; J.-L. Gauvreau; M. Gold; L.J. Harmon; J. L. Harton; J. M. Landers; E. R. Lee; D. Loomba; J. A J Matthews; E. H. Miller; A. Monte; A. St. J. Murphy; S. M. Paling; N. Phan; M. Pipe; M. Robinson; S. W. Sadler; A. Scarff; D.P. Snowden-Ifft; N.J.C. Spooner; S. Telfer; D. Walker; D. Warner; L. Yuriev

Radon gas emanating from materials is of interest in environmental science and also a major concern in rare event non-accelerator particle physics experiments such as dark matter and double beta decay searches, where it is a major source of background. Notable for dark matter experiments is the production of radon progeny recoils (RPRs), the low energy (~100 keV) recoils of radon daughter isotopes, which can mimic the signal expected from WIMP interactions. Presented here are results of measurements of radon emanation from detector materials in the 1 metre cubed DRIFT-II directional dark matter gas time projection chamber experiment. Construction and operation of a radon emanation facility for this work is described, along with an analysis to continuously monitor DRIFT data for the presence of internal 222Rn and 218Po. Applying this analysis to historical DRIFT data, we show how systematic substitution of detector materials for alternatives, selected by this device for low radon emanation, has resulted in a factor of ~10 reduction in internal radon rates. Levels are found to be consistent with the sum from separate radon emanation measurements of the internal materials and also with direct measurement using an attached alpha spectrometer. The current DRIFT detector, DRIFT-IId, is found to have sensitivity to 222Rn of 2.5 {\mu}Bq/l with current analysis efficiency, potentially opening up DRIFT technology as a new tool for sensitive radon assay of materials.


Journal of Instrumentation | 2014

Long-term study of backgrounds in the DRIFT-II directional dark matter experiment

J. Brack; E. Daw; A. Dorofeev; A. C. Ezeribe; J. R. Fox; J.-L. Gauvreau; M. Gold; L.J. Harmon; J. L. Harton; R. Lafler; J. M. Landers; R. Lauer; E. R. Lee; D. Loomba; J. A J Matthews; E. H. Miller; A. Monte; A. St. J. Murphy; S. M. Paling; N. Phan; M. Pipe; M. Robinson; S. W. Sadler; A. Scarff; D.P. Snowden-Ifft; N.J.C. Spooner; S. Telfer; D. Walker; L. Yuriev

Low-pressure gas Time Projection Chambers being developed for directional dark matter searches offer a technology with strong particle identification capability combined with the potential to produce a definitive detection of Galactic Weakly Interacting Massive Particle (WIMP) dark matter. A source of events able to mimic genuine WIMP-induced nuclear recoil tracks arises in such experiments from the decay of radon gas inside the vacuum vessel. The recoils that result from associated daughter nuclei are termed Radon Progeny Recoils (RPRs). We present here experimental data from a long-term study using the DRIFT-II directional dark matter experiment at the Boulby Underground Laboratory of the RPRs, and other backgrounds that are revealed by relaxing the normal cuts that are applied to WIMP search data. By detailed examination of event classes in both spatial and time coordinates using 3.5 years of data, we demonstrate the ability to determine the origin of 4 specific background populations and describe development of new technology and mitigation strategies to suppress them.


International Journal of Greenhouse Gas Control | 2015

Simulation of muon radiography for monitoring CO2 stored in a geological reservoir

J. Klinger; Stewart J. Clark; Max Coleman; Jon Gluyas; V.A. Kudryavtsev; D. L. Lincoln; S. Pal; S. M. Paling; N.J.C. Spooner; S. Telfer; L. F. Thompson; D. Woodward

Current methods of monitoring subsurface CO2, such as repeat seismic surveys, are episodic and require highly skilled personnel to acquire the data. Simulations based on simplified models have previously shown that muon radiography could be automated to continuously monitor CO2 injection and migration, in addition to reducing the overall cost of monitoring. In this paper, we present a simulation of the monitoring of CO2 plume evolution in a geological reservoir using muon radiography. The stratigraphy in the vicinity of a nominal test facility is modelled using geological data, and a numerical fluid flow model is used to describe the time evolution of the CO2 plume. A planar detection region with a surface area of 1000 m2 is considered, at a vertical depth of 776 m below the seabed. We find that 1 year of constant CO2 injection leads to changes in the column density of ≲1%, and that the CO2 plume is already resolvable with an exposure time of less than 50 days.


Physics Procedia | 2015

Background Assay and Rejection in DRIFT

Jeff Brack; Ed Daw; A. Dorofeev; Anthony Ezeribe; J.-L. Gauvreau; Michael Gold; J. L. Harton; R. Lafler; R. Lauer; E. R. Lee; D. Loomba; John A. J. Matthews; E. H. Miller; Alissa Monte; Alex Murphy; S. M. Paling; N. Phan; Steve Sadler; Andrew Scarff; D.P. Snowden-Ifft; N.J.C. Spooner; S. Telfer; Daniel Walker; Matthew Williams; Leonid Yuriev

The DRIFT-IId dark matter detector is a m3-scale low-pressure TPC with directional sensitivity to WIMP-induced nuclear recoils. Its primary backgrounds were due to alpha decays from contamination on the central cathode. Efforts to reduce these backgrounds led to replacing the 20 μm wire central cathode with one constructed from 0.9 μm aluminized mylar, which is almost totally transparent to alpha particles. Detailed modeling of the nature and origin of the remaining backgrounds led to an in-situ, ppt-sensitive assay of alpha decay backgrounds from the central cathode. This led to further improvements in the thin-film cathode resulting in over 2 orders of magnitude reduction in backgrounds compared to the wire cathode. Finally, the addition of O2 to CS2 gas was found to produce multiple species of electronegative charge carriers, providing a method to determine the absolute position of nuclear recoils and reject all known remaining backgrounds while retaining a high efficiency for nuclear recoil detection.


Mineralogical Magazine | 2015

Geological repositories: scientific priorities and potential high-technology transfer from the space and physics sectors

Susana O. L. Direito; Samantha Clark; Claire R. Cousins; Yoshiko Fujita; Jon Gluyas; Simon L. Harley; Richard J. Holmes; Ian B. Hutchinson; V.A. Kudryavtsev; Jon R. Lloyd; Ian G. Main; Mark Naylor; Sam Payler; Nick Smith; N.J.C. Spooner; S. Telfer; L. F. Thompson; Katinka Wouters; Joanna Wragg; Charles S. Cockell

Abstract The use of underground geological repositories, such as in radioactive waste disposal (RWD) and in carbon capture (widely known as Carbon Capture and Storage; CCS), constitutes a key environmental priority for the 21st century. Based on the identification of key scientific questions relating to the geophysics, geochemistry and geobiology of geodisposal of wastes, this paper describes the possibility of technology transfer from high-technology areas of the space exploration sector, including astrobiology, planetary sciences, astronomy, and also particle and nuclear physics, into geodisposal. Synergies exist between high technology used in the space sector and in the characterization of underground environments such as repositories, because of common objectives with respect to instrument miniaturization, low power requirements, durability under extreme conditions (in temperature and mechanical loads) and operation in remote or otherwise difficult to access environments.


Archive | 2016

Muon Tomography for Carbon Storage and Monitoring

S. Pal; Stewart J. Clark; Max Coleman; Jon Gluyas; V.A. Kudryavtsev; J. Klinger; S. M. Paling; N.J.C. Spooner; S. Telfer; L. F. Thompson; D. Woodward

Levels of atmospheric carbon dioxide could be reduced through CO\(_2\) capture and storage (CCS) technologies. Careful characterisation and management of storage sites will prevent leakages, but monitoring is required to track the migration of CO\(_2\) during the injection, emplacement and storage phases. In this paper, we present muon tomography which could provide continuous subsurface CO\(_2\) monitoring system at relatively low cost.


4th EAGE CO2 Geological Storage Workshop 2014: Demonstrating Storage Integrity and Building Confidence in CCS | 2014

The Application of Muon Tomography to Carbon Storage Monitoring

L. F. Thompson; Christopher J. Benton; Stewart J. Clark; Max Coleman; Jon Gluyas; V.A. Kudryavtsev; J. Klinger; Cathryn N. Mitchell; S. Pal; S. M. Paling; N.J.C. Spooner; S. Telfer

Post-injection monitoring of stored super-critical carbon dioxide will play a crucial role in the carbon capture and storage (CCS) industry. To date a number of monitoring methods have been proposed such as repeat seismic surveys. The application of a technique known as muon tomography is discussed. The technique proposes the instrumentation of suitable voids surrounding the storage volumes with detectors capable of detecting cosmic ray muons. The observed fluxes of muons and their arrival directions are taken along with known muon fluxes at sea level from which the density of the overburden (in this case the storage volume) can be interpreted. The theoretical modelling and potential configuration of muon detectors are discussed.


Physics of the Dark Universe | 2015

First background-free limit from a directional dark matter experiment: results from a fully fiducialised DRIFT detector

James Battat; J. Brack; E. Daw; A. Dorofeev; A. C. Ezeribe; J.-L. Gauvreau; M. Gold; J. L. Harton; J. M. Landers; E. Law; E. R. Lee; D. Loomba; A. Lumnah; J. A J Matthews; E. H. Miller; A. Monte; F. Mouton; A. St. J. Murphy; S. M. Paling; N. Phan; M. Robinson; S. W. Sadler; A. Scarff; F. G. Schuckman Ii; D.P. Snowden-Ifft; N.J.C. Spooner; S. Telfer; S.E. Vahsen; D. Walker; D. Warner


Philosophical transactions of the Royal Society A : mathematical, physical and engineering sciences, 2018 [Peer Reviewed Journal] | 2018

Passive, continuous monitoring of carbon dioxide geostorage using muon tomography.

Jon Gluyas; L. F. Thompson; Dave Allen; Charlotte Benton; P. M. Chadwick; Sam Clark; Joel Klinger; V.A. Kudryavtsev; Darren Lincoln; Ben Maunder; Cathryn Mitchell; S. J. Nolan; S. M. Paling; N.J.C. Spooner; Lazar Staykov; S. Telfer; David Woodward; Max Coleman

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S. M. Paling

Rutherford Appleton Laboratory

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A. Scarff

University of Sheffield

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M. Robinson

University of Sheffield

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A. Dorofeev

Colorado State University

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D. Loomba

University of New Mexico

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