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1.
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EURECA – setting the scene for scintillators
/ Kraus, H (Oxford U.) ; Armengau, E. (IRFU, Saclay) ; Bauer, M. (Tubingen U.) ; Bavykina, I. (Munich, Max Planck Inst.) ; Benoit, A. (Grenoble, CRTBT) ; Bento, A. (Munich, Max Planck Inst.) ; Blumer, J. (Karlsruhe U., EKP ; Karlsruhe, Forschungszentrum) ; Bornschein, L. (Karlsruhe U., EKP) ; Broniatowski, A. (CSNSM, Orsay) ; Burghart, G. (CERN) et al.
EURECA (European Underground Rare Event Calorimeter Array) will be an astro-particle physics facility aiming to directly detect galactic dark matter. The Laboratoire Souterrain de Modane has been selected as host laboratory. [...]
2009
In : 1st International Workshop on Radiopure Scintillators for EURECA, Kiev, Ukraine, 9 - 10 Sep 2008, pp.7-11
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2.
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3.
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An Electromagnetic Undulator for the Far Infrared at ELBE
/ Dekorsy, Thomas ; Fahmy, Karim ; Grosse, Eckart ; Michel, Peter ; Seidel, Wolfgang ; Wolf, Andreas ; Wuensch, Rudi
The first lasing in the mid IR at the ELBE FEL allows us to specify the parameters of a new undulator for longer wavelengths to complement the U27 undulator which is useful up to about 25 microns. In the longer wavelength region FELs constitute a unique radiation source with appealing properties. [...]
2004
External link: Published version from JACoW
In : 26th International Free Electron Laser Conference and 11th FEL User Workshop 2004, Trieste, Italy, 29 Aug - 3 Sep 2004, pp.e-proc. TUPOS04
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4.
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A Far-Infrared FEL for the Radiation Source ELBE
/ Seidel, W ; Grosse, E ; Lehnert, U ; Michel, P ; Schlenk, R ; Willkommen, U ; Wohlfarth, D ; Wünsch, R
After successfully commissioning the mid-infrared FEL (U27) and adjoining a second accelerator unit (up to 35 MeV) at ELBE we have modified our plan how to produce radiation in the far infrared.To ensure the continuous variation of the wavelength up to 150 microns we want to complement the U27 undulator by a permanent magnet undulator with a period of 100 mm (U100). The minimum gap of 24 mm and the hybrid construction consisting of Sm/Co magnets and soft iron poles ensures sufficient radiation resistance and allows rms undulator parameters up to 2.7. [...]
2005
External link: Published version from JACoW
In : 27th International Conference on Free Electron Lasers, Palo Alto, CA, USA, 21 - 26 Aug 2005, pp.290
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5.
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Optical Beam Properties and Performance of the MID-IR FEL at ELBE
/ Lehnert, U ; Michel, P ; Seidel, W ; Stehr, D ; Teichert, J ; Wohlfarth, D ; Wünsch, R
First lasing of the mid-infrared free-electron laser at ELBE was achieved on May 7, 2004. Since then stable lasing has been achieved in the IR range from 4 to 22~μm using electron beam energies from 15 to 35~MeV. [...]
2005
External link: Published version from JACoW
In : 27th International Conference on Free Electron Lasers, Palo Alto, CA, USA, 21 - 26 Aug 2005, pp.286
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6.
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Diagnostic Tools for Operation and Optimization of the ELBE-FEL
/ Michel, P ; Evtushenko, P ; Lehnert, U ; Schneider, C ; Schurig, R ; Seidel, W ; Teichert, J ; Wohlfarth, D
A FEL in the mid infrared range is one of the applications of the ELBE cw-electron accelerator. The successful operation of the lasing process for the different wavelength is mainly determined by the alignment of the optical cavities, the bunch length and the energy spread of the electron beam so as the transversal adjustment of the beam through the FEL. [...]
2005
External link: Published version from JACoW
In : 27th International Conference on Free Electron Lasers, Palo Alto, CA, USA, 21 - 26 Aug 2005, pp.102
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7.
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Critical revision of the ZEPLIN-I sensitivity to WIMP interactions
/ Benoît, A (Grenoble, CRTBT) ; Chapellier, M (Saclay) ; Chardin, G (DSM, DAPNIA, Saclay) ; Dumoulin, L (CSNSM, Orsay) ; Eitel, K (Karlsruhe, Forschungszentrum) ; Gascon, J (Lyon, IPN) ; Gerbier, G (DSM, DAPNIA, Saclay) ; Goldbach, C (Paris, Inst. Astrophys.) ; Jochum, J (Tubingen U.) ; de Lesquen, A (DSM, DAPNIA, Saclay) et al.
The ZEPLIN collaboration has recently published its first result presenting a maximum sensitivity of $1.1 \times 10^{-6}$ picobarn for a WIMP mass of $\approx$ 60 GeV. The analysis is based on a discrimination method using the different time distribution of scintillation light generated in electron recoil and nuclear recoil interactions. [...]
astro-ph/0512120; DAPNIA-2005-357.-
Saclay : DAPNIA, 2006 - 8 p.
- Published in : Phys. Lett. B 637 (2006) 156-160
Access to fulltext document: PDF; External link: astro-ph/0512120 PDF
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8.
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Results of CRESST phase I
/ Cozzini, C ; Altmann, M ; Angloher, G ; Bruckmayer, M ; Bucci, C ; Cooper, S ; Di Stefano, P ; Feilitzsch, F V ; Frank, T ; Hauff, D et al.
2001
In : 9th International Workshop on Low Temperature Detectors, Madison, WI, USA, 23 - 27 Jul 2001, pp.481-484
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9.
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Performance of CRESST detectors and status of the experiment
/ Sisti, M ; Bucci, C ; Bühler, M ; Cooper, S ; Feilitzsch, F ; Höhne, J ; Jörgens, V ; Loidl, M ; Meier, O ; Nagel, U et al.
1997
In : 7th International Workshop on Low-Temperature Detectors, Munich, Germany, 27 Jul - 2 Aug 1997, pp.232-236
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10.
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Quasiparticle diffusion in a tungsten/aluminum proximity layer
/ Loidl, M ; Cooper, S ; Ferger, P ; Meier, O ; Pröbst, F ; Seidel, W ; Sisti, M
1997
In : 7th International Workshop on Low-Temperature Detectors, Munich, Germany, 27 Jul - 2 Aug 1997, pp.155-157
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