Search Results - "Sheng, X.D"

Possible implications of the channeling effect in NaI(Tl) crystals by Bernabei, R., Belli, P., Montecchia, F., Nozzoli, F., Cappella, F., Incicchitti, A., Prosperi, D., Cerulli, R., Dai, C.J., He, H.L., Kuang, H.H., Ma, J.M., Ma, X.H., Sheng, X.D., Ye, Z.P., Wang, R.G., Zhang, Y.J.

“…The channeling effect of low energy ions along the crystallographic axes and planes of NaI(Tl) crystals is discussed in the framework of corollary…”
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DAMA/LIBRA results and perspectives by Bernabei, R., Belli, P., Di Marco, A., Montecchia, F., d’Angelo, A., Incicchitti, A., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., He, H.L., Kuang, H.H., Ma, X.H., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The DAMA/LIBRA experiment (~ 250 kg sensitive mass composed by highly radio-pure NaI(Tl)) is in data taking in the underground Laboratory of Gran Sasso (LNGS)…”
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DAMA/LIBRA Results and Perspectives by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d'Angelo, A., Di Marco, A., He, H.L., Incicchitti, A., Kuang, H.H., Ma, X.H., Montecchia, F., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The DAMA/LIBRA experiment (~ 250 kg sensitive mass composed by highly radio-pure NaI(Tl)) is in data taking in the underground Laboratory of Gran Sasso (LNGS)…”
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Highlights on signals from Dark Matter particles by Bernabei, R., Belli, P., Di Marco, A., Montecchia, F., d'Angelo, A., Incicchitti, A., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., He, H.L., Kuang, H.H., Ma, X.H., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…Many experimental observations and theoretical arguments have pointed out that a large fraction of the Universe is composed by Dark Matter particles. Many…”
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DAMA/LIBRA-phase1 results and perspectives of the phase2 by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d'Angelo, A., d'Angelo, S., Marco, A. Di, He, H.L., Incicchitti, A., Kuang, H.H., Ma, X.H., Montecchia, F., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The DAMA/LIBRA experiment (∼ 250 kg of highly radio-pure NaI(Tl)) is running deep underground at the Gran Sasso National Laboratory (LNGS) of the I.N.F.N. Here…”
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The Dark Matter annual modulation results from DAMA/LIBRA by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d’Angelo, A., Di Marco, A., He, H.L., Incicchitti, A., Ma, X.H., Montecchia, F., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The DAMA/LIBRA experiment, running at the Gran Sasso National Laboratory of the I.N.F.N. in Italy, has a sensitive mass of about 250 kg highly radiopure…”
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Highlights of DAMA/LIBRA by Bernabei, R., Belli, P., d’Angelo, A., d’Angelo, S., Di Marco, A., Montecchia, F., Incicchitti, A., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., He, H.L., Kuang, H.H., Ma, X.H., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The DAMA project develops and uses new/improved low background scintillation detectors to investigate the Dark Matter (DM) particle component(s) in the…”
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DAMA/LIBRA-phase1 results and perspectives of the phase2 by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d’Angelo, A., d’Angelo, S., Di Marco, A., He, H.L., Incicchitti, A., Kuang, H.H., Ma, X.H., Montecchia, F., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The results obtained with the total exposure of 1.04 ton × yr collected by DAMA/LIBRA–phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of…”
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New results and perspectives of DAMA/LIBRA by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Castellano, S., Cerulli, R., Dai, C.J., d’Angelo, A., d’Angelo, S., Di Marco, A., He, H.L., Incicchitti, A., Kuang, H.H., Ma, X.H., Montecchia, F., Sheng, X.D., Wang, R.G., Ye, Z.P.

“…The results obtained with the total exposure of 1.04 ton x yr collected by DAMA/LIBRA-phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of…”
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Final model independent result of DAMA/LIBRA–phase1 by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Castellano, S., Cerulli, R., Dai, C. J., d’Angelo, A., d’Angelo, S., Di Marco, A., He, H. L., Incicchitti, A., Kuang, H. H., Ma, X. H., Montecchia, F., Prosperi, D., Sheng, X. D., Wang, R. G., Ye, Z. P.

“…The results obtained with the total exposure of 1.04 ton × yr collected by DAMA/LIBRA–phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of…”
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The DAMA project: Achievements, implications and perspectives by Bernabei, R., Belli, P., Bussolotti, A., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d’Angelo, A., Di Marco, A., Ferrari, N., Incicchitti, A., Ma, X.H., Mattei, A., Merlo, V., Montecchia, F., Sheng, X.D., Ye, Z.P.

“…Experimental observations and theoretical arguments at galactic and larger scales pointed out that a large fraction of the Universe is composed of Dark Matter…”
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New results from DAMA/LIBRA by Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., d’Angelo, A., He, H. L., Incicchitti, A., Kuang, H. H., Ma, X. H., Montecchia, F., Nozzoli, F., Prosperi, D., Sheng, X. D., Wang, R. G., Ye, Z. P.

“…DAMA/LIBRA is running at the Gran Sasso National Laboratory of the I.N.F.N. Here the results obtained with a further exposure of 0.34 ton × yr are presented…”
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First model independent results from DAMA/LIBRA-phase2 by Bernabei, R., Belli, P., Bussolotti, A., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d’Angelo, A., Di Marco, A., He, H.L., Incicchitti, A., Ma, X.H., Mattei, A., Merlo, V., Montecchia, F., Sheng, X.D., Ye, Z.P.

“…The first model independent results obtained by the DAMA/LIBRA-phase2 experiment are presented. The data have been collected over 6 annual cycles corresponding…”
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The DAMA/LIBRA apparatus by Bernabei, R., Belli, P., Bussolotti, A., Cappella, F., Cerulli, R., Dai, C.J., d’Angelo, A., He, H.L., Incicchitti, A., Kuang, H.H., Ma, J.M., Mattei, A., Montecchia, F., Nozzoli, F., Prosperi, D., Sheng, X.D., Ye, Z.P.

“…The ≃ 250 kg highly radiopure NaI(Tl) DAMA/LIBRA apparatus, running at the Gran Sasso National Laboratory (LNGS) of the INFN, is described…”
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No role for neutrons, muons and solar neutrinos in the DAMA annual modulation results by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C. J., d’Angelo, A., d’Angelo, S., Di Marco, A., He, H. L., Incicchitti, A., Kuang, H. H., Ma, X. H., Montecchia, F., Sheng, X. D., Wang, R. G., Ye, Z. P.

“…This paper summarizes in a simple and intuitive way why the neutrons, the muons and the solar neutrinos cannot give any significant contribution to the DAMA…”
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Model independent result on possible diurnal effect in DAMA/LIBRA-phase1 by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Castellano, S., Cerulli, R., Dai, C. J., d’Angelo, A., d’Angelo, S., Di Marco, A., He, H. L., Incicchitti, A., Kuang, H. H., Ma, X. H., Montecchia, F., Prosperi, D., Sheng, X. D., Wang, R. G., Ye, Z. P.

“…The results obtained in the search for possible diurnal effect in the single-hit low energy data collected by DAMA/LIBRA-phase1 (total exposure 1.04 ton ×…”
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No role for muons in the DAMA annual modulation results by Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C. J., d’Angelo, A., Di Marco, A., He, H. L., Incicchitti, A., Ma, X. H., Montecchia, F., Sheng, X. D., Wang, R. G., Ye, Z. P.

“…This paper gathers arguments and reasons why muons surviving the Gran Sasso mountain cannot mimic the Dark Matter annual modulation signature exploited by the…”
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Search for charge non-conserving processes in [sup.127]I by coincidence technique by Bernabei, R, Belli, P, Cappella, F, Cerulli, R, Dai, C.J, d'Angelo, A, d'Angelo, S, Di Marco, A, He, H.L, Incicchitti, A, Ma, X.H, Montecchia, F, Sheng, X.D, Wang, R.G, Ye, Z.P

“…New lifetime limits on the charge non-conserving (CNC) electron capture with excitation of the 417.9 keV nuclear level in the [sup.127]I are established by…”
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First results from DAMA/LIBRA–phase2 by Bernabei, R., Belli, P., Bussolotti, A., Cappella, F., Caracciolo, V., Cerulli, R., Dai, C.J., d'Angelo, A., Di Marco, A., He, H.L., Incicchitti, A., Ma, X.H., Mattei, A., Merlo, V., Montecchia, F., Sheng, X.D., Ye, Z.P.

“…The first results obtained by the DAMA/LIBRA–phase2 experiment with the data collected deep underground at the Gran Sasso National Laboratory over 6…”
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Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode by Bartoli, B., Bernardini, P., Bi, X. J., Cao, Z., Catalanotti, S., Chen, S. Z., Chen, T. L., Cui, S. W., Dai, B. Z., D'Amone, A., Danzengluobu, Mitri, I. De, Piazzoli, B. D'Ettorre, Girolamo, T. Di, Sciascio, G. Di, Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gao, W., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Li, H. J., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Mastroianni, S., Montini, P., Ning, C. C., Perrone, L., Pistilli, P., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q.

“…The ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a "full coverage" (central carpet with an active…”
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