Zobrazeno 1 - 10
of 126
pro vyhledávání: '"Cozzini, C."'
Autor:
Chauhan, V., Harikishore, K., Girdhar, S., Kaushik, S., Wiesinger, F., Cozzini, C., Carl, M., Fung, M., Mehta, B.B., Thomas, B., Kesavadas, C.
Publikováno v:
In Clinical Radiology August 2024
Autor:
Astrom, J., Di Stefano, P. C. F., Proebst, F., Stodolsky, L., Timonen, J., Bucci, C., Cooper, S., Cozzini, C., Feilitzsch, F. v., Kraus, H., Marchese, J., Meier, O., Nagel, U., Ramachers, Y., Seidel, W., Sisti, M., Uchaikin, S., Zerle, L.
Publikováno v:
Phys.Lett. A356 (2006) 262-266
In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very
Externí odkaz:
http://arxiv.org/abs/physics/0504151
Autor:
Majorovits, B., Angloher, G., Bucci, C., Christ, P., Cozzini, C., von Feilitzsch, F., Hauff, D., Henry, S., Jagemann, Th., Jochum, J., Kraus, H., Mikhailik, V., Ninkovic, J., Petricca, F., Potzel, W., Proebst, F., Ramachers, Y., Razeti, M., Rau, W., Seidel, W., Stark, M., Stodolsky, L., Tolhurst, A. J. B., Wahl, D., Westphal, W., Wulandari, H.
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten re
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411396
Autor:
Cozzini, C., Angloher, G., Bucci, C., von Feilitzsch, F., Hauff, D., Henry, S., Jagemann, Th., Jochum, J., Kraus, H., Majorovits, B., Mikhailik, V., Ninkovic, J., Petricca, F., Potzel, W., Proebst, F., Ramachers, Y., Rau, W., Razeti, M., Seidel, W., Stark, M., Stodolsky, L., Tolhurst, A. J. B., Westphal, W., Wulandari, H.
Publikováno v:
Phys.Rev.C70:064606,2004
The natural alpha decay of 180W has been unambiguously detected for the first time. The alpha peak is found in a (gamma,beta and neutron)-free background spectrum. This has been achieved by the simultaneous measurement of phonon and light signals wit
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0408006
Autor:
Angloher, G., Bucci, C., Christ, P., Cozzini, C., von Feilitzsch, F., Hauff, D., Henry, S., Jagemann, Th., Jochum, J., Kraus, H., Majorovits, B., Ninkovic, J., Petricca, F., Potzel, W., Pröbst, F., Ramachers, Y., Razeti, M., Rau, W., Seidel, W., Stark, M., Stodolsky, L., Tolhurst, A. J. B., Westphal, W., Wulandari, H.
Publikováno v:
Astropart.Phys.23:325-339,2005
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Data from early 2004 with two 300 g CRESST-II prototype detector modules
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408006
Autor:
Di Stefano, P. C. F., Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., Proebst, F., Rutzinger, S., Seidel, W., Stodolsky, L., Schmidt, J.
Publikováno v:
Journal of Applied Physics, Vol. 94, No. 10, 6887, 15 November 2003
We apply the standard photovoltaic technique of texturing to reduce the reflectivity of silicon cryogenic calorimetric light detectors. In the case of photons with random incidence angles, absorption is compatible with the increase in surface area. F
Externí odkaz:
http://arxiv.org/abs/physics/0307042
Autor:
Altmann, M., Angloher, G., Bruckmayer, M., Bucci, C., Cooper, S., Cozzini, C., DiStefano, P., von Feilitzsch, F., Frank, T., Hauff, D., Jagemann, Th., Jochum, J., Keeling, R., Kraus, H., Macallister, J., Proebst, F., Ramachers, Y., Schnagl, J., Seidel, W., Sergeyev, I., Stark, M., Stodolsky, L., Wulandari, H.
Data taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits on WIMP dark matter in the Galactic Halo. The detector is especially sensitive for low-mass WIMPS with spin-dependent cross section
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106314
Autor:
Di Stefano, P., Bruckmayer, M., Bucci, C., Cooper, S., Cozzini, C., von Feilitzsch, F., Frank, T., Hauff, D., Jagemann, T., Jochum, J., Keeling, R., Kraus, H., Marchese, J., Pergolesi, D., Proebst, F., Ramachers, Y., Schnagl, J., Seidel, W., Sergeyev, I., Stark, M., Stodolsky, L., Uchaikin, S., Wulandari, H.
The CRESST experiment seeks hypothetical WIMP particles that could account for the bulk of dark matter in the Universe. The detectors are cryogenic calorimeters in which WIMPs would scatter elastically on nuclei, releasing phonons. The first phase of
Externí odkaz:
http://arxiv.org/abs/hep-ex/0011064
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Akademický článek
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