Fracture Processes Observed with A Cryogenic Detector

(2005)

Authors:

J Astrom, PCF Di Stefano, F Proebst, L Stodolsky, J Timonen, C Bucci, S Cooper, C Cozzini, FV Feilitzsch, H Kraus, J Marchese, O Meier, U Nagel, Y Ramachers, W Seidel, M Sisti, S Uchaikin, L Zerle

Limits on WIMP dark matter using scintillating CaWO4 cryogenic detectors with active background suppression

Astroparticle Physics 23 (2005) 325-339

Authors:

H Kraus, G Angloher, F Proebst, S Henry

Tuning into UHE Neutrinos in Antarctica - The ANITA Experiment

ArXiv astro-ph/0503304 (2005)

Authors:

P Miocinovic, SW Barwick, JJ Beatty, DZ Besson, WR Binns, B Cai, JM Clem, A Connolly, S Coutu, DF Cowen, PF Dowkontt, MA DuVernois, PA Evenson, D Goldstein, PW Gorham, CL Hebert, MH Israel, JG Learned, KM Liewer, JT Link, S Matsuno, JW Nam, CJ Naudet, R Nichol, KJ Palladino, M Rosen, D Saltzberg, D Seckel, A Silvestri, GS Varner, D Williams

Abstract:

The Antarctic Impulsive Transient Antenna (ANITA) experiment is being developed to search for ultra-high-energy (UHE) neutrino interactions ($>3\times10^{18}$ eV) in the Antarctic ice cap. A neutrino interaction in the ice will produce a radio pulse by the means of the Askaryan effect. The large radio transparency of ice allows for such a pulse to be recorded by a cluster of balloon-borne antennas. The details of the ANITA instrument, now in a construction phase, and the science we hope to achieve is discussed. In order to prepare for the main mission, we have flown ANITA-lite during the 2003/04 austral season. ANITA-lite consisted of two quad-ridge horn antennas and a prototype RF (radio frequency) triggering and recording system. Here we present the results of an impulsive RF background survey of Antarctica, as well as proof-of-principle gain, tracking, and timing calibrations conducted by observing solar radio emissions and calibration radio-pulses. A preliminary UHE neutrino flux limit based on ANITA-lite data is also presented.

Luminescence studies of Ti-doped Al2 O3 using vacuum ultraviolet synchrotron radiation

Applied Physics Letters 86:10 (2005) 1-3

Authors:

VB Mikhailik, H Kraus, D Wahl, MS Mykhaylyk

Abstract:

In this study, we examined the luminescence response of Ti-doped Al2 O3 crystals to high-energy vacuum ultraviolet (UV) excitation. In addition to the thoroughly studied emission band of Ti3+ in the near-infrared region and blue emission at 420 nm, we detected a UV emission band at 290 nm. The excitation spectra of all emission bands were measured over the 4-20 eV spectral range. Our results indicate that intrinsic anion defects are involved in the process of the excitation of the 420 nm emission assigned to the charge transfer transitions 2p O2- →3d Ti4+. Analysis of the spectral and decay characteristics of the UV emission enables us to suggest that this band is associated with radiative decay of excitons localized at Ti ions. © 2005 American Institute of Physics.

Feasibility study of a ZnWO4 scintillator for exploiting materials signature in cryogenic WIMP Dark Matter searches

Physics Letters B 610 (2005) 37-44

Authors:

H Kraus, V B Mikhailik, Y Ramachers, D Day