Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For young people
    • For teachers
    • For the public
    • For alumni
    • For business
  • Support
Menu
Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Samuel Henry

Detector Development Scientist

Research theme

  • Instrumentation
  • Fundamental particles and interactions

Sub department

  • Particle Physics

Research groups

  • ATLAS
  • ePIC
Samuel.Henry@physics.ox.ac.uk
Telephone: 01865 (2)73378
Denys Wilkinson Building, room 624
  • About
  • Research
  • Public Engagement
  • Teaching
  • Publications

ZnWO4 scintillators for cryogenic dark matter experiments

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 600:3 (2009) 594-598

Authors:

H Kraus, FA Danevich, S Henry, VV Kobychev, VB Mikhailik, VM Mokina, SS Nagorny, OG Polischuk, VI Tretyak

Abstract:

The scintillation properties of a zinc tungstate crystal, shaped as a hexagonal prism (height 40 mm, diagonal 40 mm) were determined. An energy resolution of 10.7% for the 662 keV γ-line of 137Cs was measured with the scintillator placed in a light collection setup similar to that used by the CRESST dark matter search. The light output and decay kinetics of ZnWO4 were examined over the temperature range 7-300 K and confirmed to be competitive with those of CaWO4. The radioactive contaminations of the ZnWO4 scintillator measured in the Solotvina Underground Laboratory do not exceed 0.1-10 mBq/kg (depending on radionuclide). Our study highlights the excellent feasibility of this ZnWO4 scintillator for a cryogenic dark matter experiment. © 2008 Elsevier B.V. All rights reserved.
More details from the publisher
More details

Eureca - The future of cryogenic dark matter detection in Europe

Eas Publications Series 36 (2009) 249-255

Authors:

H Kraus, B Armengaud, M Bauer, I Bavykina, A Benoit, A Bento, J Blümer, L Bornschein, A Broniatowski, G Burghart, P Camus, A Chantelauze, M Chapellier, G Chardin, C Ciemniak, C Coppi, N Coron, O Crauste, FA Danevich, M De Jésus, P De Marcillac, E Daw, X Defay, G Deuter, J Domange, P Di Stefano, G Drexlin, L Dumoulin, K Eitel, F Von Feilitzsch, D Filosofov, P Gandit, E Garcia, J Gascon, G Gerbier, J Gironnet, H Godfrin, S Grohmann, M Gros, M Hannewald, D Hauff, F Haug, S Henry, P Huff, J Imber, S Ingleby, C Isaila, J Jochum, A Juillard, M Kiefer, M Kimmerle, H Kluck, VV Kobychev, V Kozlov, VM Kudovbenko, AV Kudryavtsev, T Lachenmaier, JC Lanfranchi, RF Lang, P Loaiza, A Lubashevsky, M Malek, S Marnieros, R McGowan, V Mikhailik, A Monfardini, XF Navick, T Niinikoski, AS Nikolaiko, L Oberauer, E Olivieri, Y Ortigoza, E Pantic, P Pari, B Paul, G Perinic, F Petricca, S Pfister, C Pobes, DV Poda, RB Podviyanuk, OG Polischuk, W Potzel, F Pröbst, J Puimedon, M Robinson, S Roth, K Rottler, S Rozov, C Sailer, A Salinas, V Sanglard, ML Sarsa, K Schäffner, S Scholl, S Scorza, A Smolnikov, W Seidel, S Semikh, M Stern

Abstract:

EURECA (European Underground Rare Event Calorimeter Array) is an astro-particle physics facility aiming to directly detect galactic dark matter. The Laboratoire Souterrain de Modane has been selected as host laboratory. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. EURECA will use a target mass of up to one ton, enough to explore WIMP - nucleon scalar scattering cross sections in the region of 10-9 - 10-10 picobarn. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification). © EAS, EDP Sciences 2009.
More details from the publisher
More details

Searching for dark matter with CRESST

Proceedings of the 5th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2009 (2009) 11-15

Authors:

H Kraus, G Angloher, M Bauer, I Bavykina, A Bento, A Brown, C Bucci, C Ciemniak, C Coppi, G Deuter, F Von Feilitzsch, D Hauff, S Henry, P Huff, J Imber, S Ingleby, C Isaila, J Jochum, M Kiefer, M Kimmerle, JC Lanfranchi, RF Lang, B Majorovits, M Malek, R McGowan, VB Mikhailik, E Pantic, F Petricca, S Pfister, W Potzel, F Pröbst, S Roth, K Rottler, C Sailer, K Schäffner, J Schmaler, S Scholl, W Seidel, M Von Sivers, L Stodolsky, C Strandhagen, R Strauss, AJB Tolhurst, I Usherov, W Westphal

Abstract:

The CRESST II experiment is a dark matter search using cryogenic phonon-scintillation detectors, aiming to detect WIMP dark matter particle interactions. The detector consists of individual, modular and scintillating (CaWO4or ZnWO4) target crystals, each equipped with a phonon sensor for precise determination of the energy deposited in the crystals. Each module is further equipped with a separate cryogenic scintillation light detector, allowing event-by-event background discrimination. An extended commissioning run during 2007 has set an upper limit on theWIMP-nucleon scattering cross section. Attention is currently focussed on the interpretation of a few remaining nuclear recoils candidate events.
More details from the publisher

Oxide scintillators to search for dark matter and double beta decay

2008 IEEE NUCLEAR SCIENCE SYMPOSIUM AND MEDICAL IMAGING CONFERENCE (2008 NSS/MIC), VOLS 1-9 (2009) 2541-+

Authors:

LL Nagornaya, FA Danevich, AM Dubovik, BV Grinyov, S Henry, V Kapustyanyk, H Kraus, D Poda, VM Mokina, VB Mikhailik, M Panasyuk, OG Polischuk, V Rudyk, V Tsybulskyi, IA Tupitsyna, Yu Ya Vostretsov
More details

EURECA - The future of cryogenic dark matter detection in Europe

Proceedings of Science (2008)

Authors:

H Kraus, E Armengaud, M Bauer, I Bavykina, A Benoit, A Bento, J Blümer, L Bornschein, A Broniatowski, G Burghart, P Camus, A Chantelauze, M Chapellier, G Chardin, C Ciemniak, C Coppi, N Coron, O Crauste, FA Danevich, M De Jésus, P Marcillac, E Daw, X Defay, G Deuter, J Domange, P Di Stefano, G Drexlin, L Dumoulin, K Eitel, F Von Feilitzsch, D Filosofov, P Gandit, E Garcia, J Gascon, G Gerbier, J Gironnet, H Godfrin, S Grohmann, M Gros, M Hannewald, D Hauff, F Haug, S Henry, P Huff, J Imber, S Ingleby, C Isaila, J Jochum, A Juillard, M Kiefer, M Kimmerle, H Kluck, VV Kobychev, V Kozlov, VA Kudryavtsev, T Lachenmaier, JC Lanfranchi, RF Lang, P Loaiza, A Lubashevsky, M Malek, S Marnieros, R McGowan, V Mikhailik, VM Mokina, A Monfardini, XF Navick, T Niinikoski, AS Nikolaiko, L Oberauer, E Olivieri, Y Ortigoza, E Pantic, P Pari, B Paul, G Perinic, F Petricca, S Pfister, C Pobes, DV Poda, RB Podviyanuk, OG Polischuk, W Potzel, F Pröbst, J Puimedon, M Robinson, S Roth, K Rottler, S Rozov, C Sailer, A Salinas, V Sanglard, ML Sarsa, K Schäffner, S Scholl, S Scorza, A Smolnikov, W Seidel, S Semikh, M Stern

Abstract:

European Underground Rare Event Calorimeter Array (EURECA) will be an astro-particle physics facility in the Laboratoire Souterrain de Modane, aiming to directly detect galactic dark matter. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. The aim is to explore WIMP - nucleon scalar cross sections in the 10-9 - 10-10 picobarn region with a target mass of up to one ton. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification).

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 5
  • Page 6
  • Page 7
  • Page 8
  • Current page 9
  • Page 10
  • Page 11
  • Page 12
  • Page 13
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics
  • Current students
  • Staff intranet