Zobrazeno 1 - 10
of 735
pro vyhledávání: '"Lam, C W"'
Autor:
Arapis, A., Constantoudis, V., Kontziampasis, D., Milionis, A., Lam, C. W. E., Tripathy, A., Poulikakos, D., Gogolides, E.
Nanostructured surfaces usually exhibit complicated morphologies that cannot be described in terms of Euclidean geometry. Simultaneously, they do not constitute fully random noise fields to be characterized by simple stochastics and probability theor
Externí odkaz:
http://arxiv.org/abs/2202.00957
Autor:
XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Brown, E., Cardoso, J. M. R., Choi, B., Cline, D., Fattori, S., Ferella, A. D., Giboni, K. L., Kish, A., Lam, C. W., Lang, R. F., Lim, K. E., Lopes, J. A. M., Undagoitia, T. Marrodan, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C., Santorelli, R., Santos, J. M. F. dos, Schumann, M., Shagin, P., Teymourian, A., Tziaferi, E., Wang, H., Yamashita, M.
Publikováno v:
Astropart. Phys. 35 (2012), 573-590
The XENON100 dark matter experiment uses liquid xenon (LXe) in a time projection chamber (TPC) to search for Xe nuclear recoils resulting from the scattering of dark matter Weakly Interacting Massive Particles (WIMPs). In this paper we present a deta
Externí odkaz:
http://arxiv.org/abs/1107.2155
Autor:
Arisaka, K., Beltrame, P., Lam, C. W., Smith, P. F., Ghag, C., Cline, D. B., Lung, K., Meng, Y., Pantic, E., Scovell, P. R., Teymourian, A., Wang, H.
Publikováno v:
Astroparticle Physics 36 (2012) 93-122
We study a three stage dark matter and neutrino observatory based on multi-ton two-phase liquid Xe and Ar detectors with sufficiently low backgrounds to be sensitive to WIMP dark matter interaction cross sections down to 10E-47 cm^2, and to provide b
Externí odkaz:
http://arxiv.org/abs/1107.1295
Autor:
XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Bruch, T., Bruno, G., Cardoso, J. M. R., Chen, W. -T., Choi, B., Cline, D., Duchovni, E., Fattori, S., Ferella, A. D., Gao, F., Giboni, K. -L., Gross, E., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Levy, C., Lim, K. E., Lin, Q., Lindemann, S., Lindner, M., Lopes, J. A. M., Lung, K., Undagoitia, T. Marrodán, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Persiani, R., Plante, G., Ribeiro, A. C. C., Santorelli, R., Santos, J. M. F. dos, Sartorelli, G., Schumann, M., Selvi, M., Shagin, P., Simgen, H., Teymourian, A., Thers, D., Vitells, O., Wang, H., Weber, M., Weinheimer, C.
Publikováno v:
Phys.Rev.D84:061101,2011
The XENON100 experiment has recently completed a dark matter run with 100.9 live-days of data, taken from January to June 2010. Events in a 48kg fiducial volume in the energy range between 8.4 and 44.6 keVnr have been analyzed. A total of three event
Externí odkaz:
http://arxiv.org/abs/1104.3121
Autor:
XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Bruch, T., Bruno, G., Cardoso, J. M. R., Chen, W. -T., Choi, B., Cline, D., Duchovni, E., Fattori, S., Ferella, A. D., Gao, F., Giboni, K. -L., Gross, E., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Levy, C., Lim, K. E., Lin, Q., Lindemann, S., Lindner, M., Lopes, J. A. M., Lung, K., Undagoitia, T. Marrodan, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Persiani, R., Plante, G., Ribeiro, A. C. C., Santorelli, R., Santos, J. M. F. dos, Sartorelli, G., Schumann, M., Selvi, M., Shagin, P., Simgen, H., Teymourian, A., Thers, D., Vitells, O., Wang, H., Weber, M., Weinheimer, C.
Publikováno v:
Phys. Rev. Lett. 107, 131302 (2011)
We present results from the direct search for dark matter with the XENON100 detector, installed underground at the Laboratori Nazionali del Gran Sasso of INFN, Italy. XENON100 is a two-phase time projection chamber with a 62 kg liquid xenon target. I
Externí odkaz:
http://arxiv.org/abs/1104.2549
Autor:
XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Cardoso, J. M. R., Choi, B., Cline, D., Fattori, S., Ferella, A. D., Giboni, K. L., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Lim, K. E., Lopes, J. A. M., Undagoitia, T. Marrodan, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C, Santorelli, R., Santos, J. M. F. dos, Schumann, M., Shagin, P., Teymourian, A., Thers, D., Tziaferi, E., Wang, H., Weinheimer, C., Laubenstein, M., Nisi, S.
Publikováno v:
Astropart.Phys.35:43-49,2011
Results of the extensive radioactivity screening campaign to identify materials for the construction of XENON100 are reported. This Dark Matter search experiment is operated underground at Laboratori Nazionali del Gran Sasso (LNGS), Italy. Several ul
Externí odkaz:
http://arxiv.org/abs/1103.5831
Autor:
Teymourian, A., Aharoni, D., Baudis, L., Beltrame, P., Brown, E., Cline, D., Ferella, A. D., Fukasawa, A., Lam, C. W., Lim, T., Lung, K., Meng, Y., Muramatsu, S., Pantic, E., Suyama, M., Wang, H., Arisaka, K.
Publikováno v:
Nucl. Instr. Meth. A 654 (2011) 184
Dark Matter and Double Beta Decay experiments require extremely low radioactivity within the detector materials. For this purpose, the University of California, Los Angeles and Hamamatsu Photonics have developed the QUartz Photon Intensifying Detecto
Externí odkaz:
http://arxiv.org/abs/1103.3689
Autor:
XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Bruch, T., Cardoso, J. M. R., Choi, B., Cline, D., Duchovni, E., Fattori, S., Ferella, A. D., Giboni, K. -L., Gross, E., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Lim, K. E., Lindemann, S., Lindner, M., Lopes, J. A. M., Undagoitia, T. Marrodán, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C., Santorelli, R., Santos, J. M. F. dos, Schumann, M., Shagin, P., Teymourian, A., Thers, D., Tziaferi, E., Vitells, O., Wang, H., Weber, M., Weinheimer, C.
Publikováno v:
Phys. Rev. D 84, 052003 (2011)
Many experiments that aim at the direct detection of Dark Matter are able to distinguish a dominant background from the expected feeble signals, based on some measured discrimination parameter. We develop a statistical model for such experiments usin
Externí odkaz:
http://arxiv.org/abs/1103.0303
Autor:
XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Cardoso, J. M. R., Choi, B., Cline, D., Fattori, S., Ferella, A. D., Giboni, K. -L., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Lim, K. E., Lin, Q., Lindemann, S., Lindner, M., Lopes, J. A. M., Lung, K., Undagoitia, T. Marrodan, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C., Santorelli, R., Santos, J. M. F. dos, Schumann, M., Shagin, P., Simgen, H., Teymourian, A., Thers, D., Tziaferi, E., Wang, H., Weber, M., Weinheimer, C.
Publikováno v:
Phys.Rev.D83:082001,2011. Erratum: Phys.Rev.D85:029904,2012
The XENON100 experiment, located at the Laboratori Nazionali del Gran Sasso (LNGS), aims to directly detect dark matter in the form of Weakly Interacting Massive Particles (WIMPs) via their elastic scattering off xenon nuclei. We present a comprehens
Externí odkaz:
http://arxiv.org/abs/1101.3866
Autor:
The XENON100 Collaboration, Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Brown, E., Cardoso, J. M. R., Choi, B., Cline, D. B., Fattori, S., Ferella, A. D., Giboni, K. -L., Hugenberg, K., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Lim, K. E., Lopes, J. A. M., Undagoitia, T. Marrodán, Mei, Y., Fernandez, A. J. Melgarejo, Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C., Santorelli, R., Santos, J. M. F. dos, Schumann, M., Shagin, P., Teymourian, A., Thers, D., Tziaferi, E., Wang, H., Weinheimer, C.
Publikováno v:
Phys.Rev.Lett.105:131302,2010
The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso in Italy, is designed to search for dark matter WIMPs scattering off 62 kg of liquid xenon in an ultra-low background dual-phase time projection chamber. In this letter,
Externí odkaz:
http://arxiv.org/abs/1005.0380