5,460 results on '"Dai C."'
Search Results
52. A multimodel assessment of drought characteristics and risks over the Huang-Huai-Hai River basin, China, under climate change
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Dai, C., Qin, X. S., Lu, W. T., and Zang, H. K.
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- 2020
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53. Using near-isogenic lines of common wheat (Triticum aestivum L.) to determine the relationship between GlutoPeak parameters and quality characteristics
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Song, W. F., Zhang, X. X., Zhang, Y. B., Chen, L., Yang, X. F., Zhao, L. J., Liu, D. J., Song, Q. J., Zhang, C. L., Xin, W. L., Xiao, Z. M., Dai, C. J., Li, H., Zhang, Y. M., and Li, J. L.
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- 2020
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- View/download PDF
54. CIPM key comparison CCPR-K1.a.2017 for spectral irradiance 250 nm to 2500 nm. Final report
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Khlevnoy, B. B. [0000-0001-9502-650X], Campos Acosta, Joaquín [0000-0001-6527-1440], Park, S. [0000-0001-9270-0183], Obein, G. [0000-0002-2577-6361], Valin, M. H. [0000-0003-1824-6175], Vissière, A. [0000-0001-9334-5400], Dai, C. [0000-0003-3417-0254], Yoon, H. [0000-0002-8999-9441], Zama, T. [0000-0002-3117-1000], Shitomi, H. [0000-0002-7164-0326], Gamouras, A. [0000-0003-0378-806X], Woods, D. J. [0000-0002-7394-1296], Khlevnoy, B. B., Solodilov, M. V., Kolesnikova, S. S., Otryaskin, D. A., Pons Aglio, Alicia, Campos Acosta, Joaquín, Shin, D. J., Park, S., Obein, G., Valin, M. H., Vissière, A., Dai, C., Wu, Z., Wang, Y., Li, L., Lin, Y., Yoon, H., Gibson, C., Liu, Y., Manson, P., Atkinson, E., Zama, T., Shitomi, H., Goodman, T., Servantes, W., Gamouras, A., Woods, D. J., Sperfeld, P., Pape, S., Khlevnoy, B. B. [0000-0001-9502-650X], Campos Acosta, Joaquín [0000-0001-6527-1440], Park, S. [0000-0001-9270-0183], Obein, G. [0000-0002-2577-6361], Valin, M. H. [0000-0003-1824-6175], Vissière, A. [0000-0001-9334-5400], Dai, C. [0000-0003-3417-0254], Yoon, H. [0000-0002-8999-9441], Zama, T. [0000-0002-3117-1000], Shitomi, H. [0000-0002-7164-0326], Gamouras, A. [0000-0003-0378-806X], Woods, D. J. [0000-0002-7394-1296], Khlevnoy, B. B., Solodilov, M. V., Kolesnikova, S. S., Otryaskin, D. A., Pons Aglio, Alicia, Campos Acosta, Joaquín, Shin, D. J., Park, S., Obein, G., Valin, M. H., Vissière, A., Dai, C., Wu, Z., Wang, Y., Li, L., Lin, Y., Yoon, H., Gibson, C., Liu, Y., Manson, P., Atkinson, E., Zama, T., Shitomi, H., Goodman, T., Servantes, W., Gamouras, A., Woods, D. J., Sperfeld, P., and Pape, S.
- Abstract
This report describes the Key Comparison of the Consultative Committee for Photometry and Radiometry CCPR-K1.a.2017 for Spectral Irradiance in the wavelength range of 250 nm to 2500 nm. Tungsten quartz halogen lamps of the FEL type (1000 W) were used as artefacts. Each participant used its own set of lamps. The star scheme of measurements was applied with the sequence participant - pilot - participant. Twelve National Metrology Institutes participated in the comparison. Each participant's measurement data were based on a totally independent spectral irradiance scale realisation. VNIIOFI (the Russian Federation) served as a pilot. The measurements were carried out from 2017 - 2020. The analysis of the comparison was performed following the step-by-step approach described in Appendix B of the Guidelines for CCPR Key Comparison Report Preparation (CCPR-G2 Rev.4). The key comparison reference values (KCRV) were calculated independently at each wavelength as the weighted means with cut-off. The measurement data of all participants were used for the KCRV excluding just a few outliers in the wavelength range of 1700 nm to 2500 nm. The relative uncertainties of the KCRV were minimal, 0.08 %, at the wavelengths of 900 nm to 1500 nm and increasing towards the limits of the spectral range up to 0.28 % at 250 nm and 0.20 % at 2500 nm. Consistency checks were satisfied at 17 of the 28 measured wavelengths, but failed at 11 wavelengths, mostly in the infrared range. For the latter wavelengths the Mandel-Paule method was applied resulting in an additional uncertainty that varied depending on wavelength from 0.11 % to 0.89 %. In general, the measurement uncertainties submitted by the participants in this comparison were less than those submitted in the previous CCPR-K1.a comparison. This is evidenced by the values of the cut-off, which had decreased at all wavelengths by a factor of 1.2 to 3.0 depending on wavelength. However, only for seven participants the degrees of equivalence
- Published
- 2023
55. Final model independent result of DAMA/LIBRA-phase1
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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., and Ye, Z. P.
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Astrophysics - Astrophysics of Galaxies ,High Energy Physics - Experiment - Abstract
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 the I.N.F.N. during 7 annual cycles (i.e. adding a further 0.17 ton x yr exposure) are presented. The DAMA/LIBRA-phase1 data give evidence for the presence of Dark Matter (DM) particles in the galactic halo, on the basis of the exploited model independent DM annual modulation signature by using highly radio-pure NaI(Tl) target, at 7.5 sigma C.L.. Including also the first generation DAMA/NaI experiment (cumulative exposure 1.33 ton x yr, corresponding to 14 annual cycles), the C.L. is 9.3 sigma and the modulation amplitude of the single-hit events in the (2-6) keV energy interval is: (0.0112 \pm 0.0012) cpd/kg/keV; the measured phase is (144 \pm 7) days and the measured period is (0.998 \pm 0.002) yr, values well in agreement with those expected for DM particles. No systematic or side reaction able to mimic the exploited DM signature has been found or suggested by anyone over more than a decade., Comment: 20 pages, 13 figures, 6 tables; in publication on Eur. Phys. J. C
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- 2013
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56. Dark Matter investigation by DAMA at Gran Sasso
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Bernabei, R., Belli, P., d'Angelo, S., Di Marco, A., Montecchia, F., Cappella, F., d'Angelo, A., Incicchitti, A., Caracciolo, V., Castellano, S., Cerulli, R., Dai, C. J., He, H. L., Ma, X. H., Sheng, X. D., Wang, R. G., and Ye, Z. P.
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Astrophysics - Galaxy Astrophysics ,High Energy Physics - Phenomenology - Abstract
Experimental observations and theoretical arguments at Galaxy and larger scales have suggested that a large fraction of the Universe is composed by Dark Matter particles. This has motivated the DAMA experimental efforts to investigate the presence of such particles in the galactic halo by exploiting a model independent signature and very highly radiopure set-ups deep underground. Few introductory arguments are summarized before presenting a review of the present model independent positive results obtained by the DAMA/NaI and DAMA/LIBRA set-ups at the Gran Sasso National Laboratory of the INFN. Implications and model dependent comparisons with other different kinds of results will be shortly addressed. Some arguments put forward in literature will be confuted., Comment: review article, 71 pages, 25 figures, 8 tables; v2: minor modifications. In publication on the International Journal of Modern Physics A
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- 2013
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57. New search for correlated e+e- pairs in the alpha decay of 241Am
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Bernabei, R., Belli, P., Cappella, F., Caracciolo, V., Castellano, S., Cerulli, R., Dai, C. J., d'Angelo, A., Di Marco, A., He, H. L., Incicchitti, A., Laubenstein, M., Ma, X. H., Montecchia, F., Sheng, X. D., Tretyak, V. I., Wang, R. G., and Ye, Z. P.
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Nuclear Experiment - Abstract
A new search for production of correlated e+e- pairs in the alpha decay of 241Am has been carried out deep underground at the Gran Sasso National Laboratory of the I.N.F.N. by using pairs of NaI(Tl) detectors of the DAMA/LIBRA set-up. The experimental data show an excess of double coincidences of events with energy around 511 keV in faced pairs of detectors, which are not explained by known side reactions. This measured excess gives a relative activity lambda = (4.70 \pm 0.63) \times 10^{-9} for the Internal Pair Production (IPP) with respect to alpha decay of 241Am; this value is of the same order of magnitude as previous determinations. In a conservative approach the upper limit lambda < 5.5 \times 10^{-9} (90% C.L.) can be derived. It is worth noting that this is the first result on IPP obtained in an underground experiment, and that the lambda value obtained in the present work is independent on the live-time estimate., Comment: 18 pages, 5 figures, 3 tables; version accepted for publication on Eur. Phys. J. A
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- 2013
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58. DAMA/LIBRA results and perspectives
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Bernabei, R., Belli, P., Di Marco, A., Cappella, F., d'Angelo, A., Incicchitti, A., Caracciolo, V., Cerulli, R., Dai, C. J., He, H. L., Ma, X. H., Sheng, X. D., Wang, R. G., Montecchia, F., and Ye, Z. P.
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Astrophysics - Galaxy Astrophysics ,High Energy Physics - Phenomenology - Abstract
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 NaI(Tl). It is mainly devoted to the investigation of Dark Matter (DM) particles in the Galactic halo by exploiting the model independent DM annual modulation signature. The present DAMA/LIBRA experiment and the former DAMA/NaI one (the first generation experiment having an exposed mass of about 100 kg) have released so far results corresponding to a total exposure of 1.17 ton yr over 13 annual cycles. They provide a model independent evidence of the presence of DM particles in the galactic halo at 8.9 sigma C.L.. A short summary of the obtained results is presented and future perspectives of the experiment mentioned., Comment: 12 pages, Proceed. of the 15th Bled Workshop "What Comes Beyond Standard Models" (December 2012), Vol. 13, No. 2
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- 2013
59. A mechanism for basal vacancy loop formation in zirconium
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Dai, C., Saidi, P., Topping, M., Béland, L.K., Yao, Z., and Daymond, M.R.
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- 2019
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60. A study on the cultivation model of information-based teaching ability of English majors state-funded normal students
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Dai, C., primary
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- 2021
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61. Health assessment for urban rivers based on the pressure, state and response framework—A case study of the Shiwuli River
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Zhao, Y.W., Zhou, L.Q., Dong, B.Q., and Dai, C.
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- 2019
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62. A few final comments to arXiv:1210.7548[hep-ph]
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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., and Ye, Z. P.
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High Energy Physics - Phenomenology ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
A few final comments on arXiv:1210.7548 are given to confute incorrect arguments claimed there.
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- 2012
63. Comment on 'On an unverified nuclear decay and its role in the DAMA experiment' (arXiv:1210.5501)
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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., and Ye, Z. P.
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High Energy Physics - Phenomenology ,Astrophysics - High Energy Astrophysical Phenomena ,Nuclear Experiment - Abstract
We briefly remind references and arguments, already discussed in the past, which confute erroneous claims in arXiv:1210.5501.
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- 2012
64. No role for muons in the DAMA annual modulation results
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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., and Ye, Z. P.
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Astrophysics - Galaxy Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment - Abstract
This paper gathers arguments and reasons why muons surviving the Gran Sasso mountain cannot mimic the Dark Matter annual modulation signature exploited by the DAMA/NaI and DAMA/LIBRA experiments. A number of these items have already been presented in individual papers. Further arguments have been addressed here in order to present a comprehensive collection and to enable a wider community to correctly approach this point., Comment: 26 pages, 9 figures. Few arguments added; version accepted for publication on Eur. Phys. J. C
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- 2012
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65. Technical aspects in dark matter investigations
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Cerulli, R., Bernabei, R., Belli, P., Cappella, F., 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., and Ye, Z. P.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
Some theoretical and experimental aspects regarding the direct dark matter field are mentioned. In particular some arguments, which play a relevant role in the evaluation of model dependent interpretations of experimental results and in comparisons, are shortly addressed., Comment: Proceedings of TAUP 2011 Conference
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- 2012
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66. Particle Dark Matter in DAMA/LIBRA
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., d'Angelo, A., He, H. L., Incicchitti, A., Ma, X. H., Montecchia, F., Nozzoli, F., Prosperi, D., Sheng, X. D., Ye, Z. P., and Wang, R. G.
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Astrophysics - Cosmology and Extragalactic Astrophysics ,High Energy Physics - Phenomenology - Abstract
The present DAMA/LIBRA experiment and the former DAMA/NaI have cumulatively released so far the results obtained with the data collected over 13 annual cycles (total exposure: 1.17 ton $\times$ yr). They give a model independent evidence of the presence of DM particles in the galactic halo on the basis of the DM annual modulation signature at 8.9 $\sigma$ C.L. for the cumulative exposure., Comment: Contribution to the Vulcano Workshop 2010 "Frontier Objects in Astrophysics and Particle Physics", Vulcano (Italy) May 2010. Recent DAMA/LIBRA results are summarized; some misleading arguments recently addressed are also quantitatively commented and erased
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- 2010
67. New results from DAMA/LIBRA
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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., and Ye, Z. P.
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Astrophysics - Galaxy Astrophysics ,Astrophysics - Cosmology and Extragalactic Astrophysics ,High Energy Physics - Experiment - Abstract
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 x yr are presented. They refer to two further annual cycles collected one before and one after the first DAMA/LIBRA upgrade occurred on September/October 2008. The cumulative exposure with those previously released by the former DAMA/NaI and by DAMA/LIBRA is now 1.17 ton x yr, corresponding to 13 annual cycles. The data further confirm the model independent evidence of the presence of Dark Matter (DM) particles in the galactic halo on the basis of the DM annual modulation signature (8.9 sigma C.L. for the cumulative exposure). In particular, with the cumulative exposure the modulation amplitude of the single-hit events in the (2 -- 6) keV energy interval measured in NaI(Tl) target is (0.0116 +- 0.0013) cpd/kg/keV; the measured phase is (146 +- 7) days and the measured period is (0.999 +- 0.002) yr, values well in agreement with those expected for the DM particles., Comment: presented at the Int. Conf. Beyond the Standard Models of Particle Physics, Cosmology and Astrophysics (BEYOND 2010), 1-6 February 2010, Cape Town, South Africa
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- 2010
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68. Technical aspects and dark matter searches
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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., and Ye, Z. P.
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Physics - Instrumentation and Detectors ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment - Abstract
A variety of detectors has been proposed for dark matter direct detection, but most of them -- by the fact -- are still at R&D stage. In many cases, it is claimed that the lack of an adequate detectors' radio-purity might be compensated through heavy uses of MonteCarlo simulations, subtractions and handlings of the measured counting rates, in order to claim higher sensitivity (just for a particular scenario). The relevance of a correct evaluation of systematic effects in the use of MonteCarlo simulations at very low energy (which has always been safely discouraged in the field so far) and of multiple subtractions and handling procedures applied to the measured counting rate is shortly addressed here at some extent. Many other aspects would also deserve suitably deep investigations., Comment: Proceedings of TAUP2009, talk presented by F.Nozzoli
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- 2009
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69. Particle Dark Matter and DAMA/LIBRA
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., d'Angelo, A., He, H. L., Incicchitti, A., Ma, X. H., Montecchia, F., Nozzoli, F., Prosperi, D., Sheng, X. D., Wang, R. G., and Ye, Z. P.
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Astrophysics - Astrophysics of Galaxies - Abstract
The DAMA/LIBRA set-up (about 250 kg highly radiopure NaI(Tl) sensitive mass) is running at the Gran Sasso National Laboratory of the I.N.F.N.. The first DAMA/LIBRA results confirm the evidence for the presence of a Dark Matter particle component in the galactic halo, as pointed out by the former DAMA/NaI set-up; cumulatively the data support such evidence at 8.2 sigma C.L. and satisfy all the many peculiarities of the Dark Matter annual modulation signature. The main aspects and prospects of this model independent experimental approach will be outlined., Comment: Contributed paper to the Int. Conf. SciNeGHE 2009, Assisi, Italy, October 2009
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- 2009
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70. Intrinsic Capacity (IC) and Survival Amongst Older Adults with Cancer: CARE Registry
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Maheshwari, S., primary, Dai, C., additional, Giri, S., additional, Harmon, C., additional, Tucker, A., additional, Fowler, M., additional, Outlaw, D., additional, and Williams, G., additional
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- 2023
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71. OP07.06: Selective feticide in monochronic twin pregnancies using fetoscopy‐guided bipolar cord coagulation
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Tang, H., primary, Dai, C., additional, Li, J., additional, Ru, T., additional, Li, Y., additional, Xiao, X., additional, Hu, Y., additional, and Zheng, M., additional
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- 2023
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72. EP14.31: Laser treatment for twin–twin transfusion syndrome in a dizygotic monochorionic twins: case report and literature review
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Tang, H., primary, Dai, C., additional, Li, H., additional, Zhu, X., additional, Duan, H., additional, Xiao, X., additional, Jin, L., additional, Li, J., additional, and Zheng, M., additional
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- 2023
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73. A novel curcumin-loaded composite dressing facilitates wound healing due to its natural antioxidant effect
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Zhao Y, Dai C, Wang Z, Chen W, Liu J, Zhuo R, Yu A, and Huang S
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Curcumin ,Cyclodextrin inclusion complex ,Chitosan ,Alginate ,Cutaneous wound healing ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Yong Zhao,1 Chuanyu Dai,2 Zheng Wang,1 Weimin Chen,1 Jiaguo Liu,3 Renxi Zhuo,2 Aixi Yu,1 Shiwen Huang2 1Department of Orthopedic Trauma and Microsurgy, Zhongnan Hospital of Wuhan University, Wuhan 430070, Hubei, People’s Republic of China; 2Key Laboratory of Biomedical Polymers of Ministry of Education, Department of Chemistry, Wuhan University, Wuhan, Hubei 430072, People’s Republic of China; 3Department of Orthopedics, Hubei University of Medicine Affliated Taihe Hospital, Shiyan 442000, Hubei, People’s Republic of ChinaCorrespondence: Aixi YuDepartment of Orthopedic Trauma and Microsurgy, Zhongnan Hospital of Wuhan University, 169 Donghu Road, Wuchang District, Wuhan 430070, Hubei, People’s Republic of ChinaTel +86 1 350 718 7489Email yuaixi@whu.edu.cnShiwen HuangKey Laboratory of Biomedical Polymers of Ministry of Education, Department of Chemistry, Wuhan University, 16 Luojiashan Road, Wuchang District, Wuhan 430072, Hubei, People’s Republic of ChinaTel +86 186 2786 5822Email swhuang@whu.edu.cnPurpose: To prepare a novel wound dressing to facilitate cutaneous wound healing.Methods: Curcumin (Cur) was added to the ring-shaped β-cyclodextrin (CD) to form a β-CD–Cur inclusion complex (CD-Cur). CD-Cur was then integrated into a composite chitosan–alginate (CA) mix. Finally, CA-CD-Cur was generated with a freeze-drying technique. Water-uptake capacity, degradation rate, and drug-release kinetics of the newly formed dressing were investigated in vitro. In animal studies, cutaneous wounds in rats were created, treated with CA-CD-Cur, then compared to CA-Cur, CA, and gauze.Results: CA-CD-Cur–treated wounds showed accelerated closure rates, improved histopathological results, and lower SOD, lipid peroxidation, pI3K, and pAktkt levels than other groups. On the contrary, catalase, IκBα, and TGFβ1 levels were higher than others.Conclusion: CA-CD-Cur may facilitate cutaneous wound dressing that facilitate wound healing.Keywords: curcumin, cyclodextrin inclusion complex, chitosan, alginate, cutaneous wound healing
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- 2019
74. The DAMA/LIBRA apparatus
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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., and Ye, Z. P.
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Astrophysics - Abstract
The $\simeq$ 250 kg highly radiopure NaI(Tl) DAMA/LIBRA apparatus, running at the Gran Sasso National Laboratory (LNGS) of the I.N.F.N., is described., Comment: 37 pages, 27 figures
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- 2008
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75. First results from DAMA/LIBRA and the combined results with DAMA/NaI
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., d'Angelo, A., He, H. L., Incicchitti, A., Kuang, H. H., Ma, J. M., Montecchia, F., Nozzoli, F., Prosperi, D., Sheng, X. D., and Ye, Z. P.
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Astrophysics - Abstract
The highly radiopure $\simeq$ 250 kg NaI(Tl) DAMA/LIBRA set-up is running at the Gran Sasso National Laboratory of the I.N.F.N.. In this paper the first result obtained by exploiting the model independent annual modulation signature for Dark Matter (DM) particles is presented. It refers to an exposure of 0.53 ton$\times$yr. The collected DAMA/LIBRA data satisfy all the many peculiarities of the DM annual modulation signature. Neither systematic effects nor side reactions can account for the observed modulation amplitude and contemporaneously satisfy all the several requirements of this DM signature. Thus, the presence of Dark Matter particles in the galactic halo is supported also by DAMA/LIBRA and, considering the former DAMA/NaI and the present DAMA/LIBRA data all together (total exposure 0.82 ton$\times$yr), the presence of Dark Matter particles in the galactic halo is supported at 8.2 $\sigma$ C.L.., Comment: 40 pages, 21 figures, 6 tables
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- 2008
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76. Investigation on light dark matter
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., He, H. L., Incicchitti, A., Kuang, H. H., Ma, J. M., Ma, X. H., Montecchia, F., Nozzoli, F., Prosperi, D., Sheng, X. D., Ye, Z. P., Wang, R. G., and Zhang, Y. J.
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Astrophysics - Abstract
Some extensions of the Standard Model provide Dark Matter candidate particles with sub-GeV mass. These Light Dark Matter particles have been considered for example in Warm Dark Matter scenarios (e.g. the keV scale sterile neutrino, axino or gravitino). Moreover MeV scale DM candidates have been proposed in supersymmetric models and as source of the 511 keV line from the Galactic center. In this paper the possibility of direct detection of a Light Dark Matter candidate is investigated considering the inelastic scattering processes on the electron or on the nucleus targets. Some theoretical arguments are developed and related phenomenological aspects are discussed. Allowed volumes and regions for the characteristic phenomenological parameters of the considered scenarios are derived from the DAMA/NaI annual modulation data., Comment: 16 pages, 8 figures, submitted for publication. Corrected typos
- Published
- 2008
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77. Two-dimensional large strain consolidation prediction and incrementally deposited tailings
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Dai, C., primary and Pells, P. J. N., additional
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- 2020
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78. Science with the new generation high energy gamma- ray experiments
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Alvarez, M., D'Armiento, D., Agnetta, G., Alberdi, A., Antonelli, A., Argan, A., Assis, P., Baltz, E. A., Bambi, C., Barbiellini, G., Bartko, H., Basset, M., Bastieri, D., Belli, P., Benford, G., Bergstrom, L., Bernabei, R., Bertone, G., Biland, A., Biondo, B., Bocchino, F., Branchini, E., Brigida, M., Bringmann, T., Brogueira, P., Bulgarelli, A., Caballero, J. A., Caliandro, G. A., Camarri, P., Cappella, F., Caraveo, P., Carbone, R., Carvajal, M., Casanova, S., Castro-Tirado, A. J., Catalano, O., Catena, R., Celi, F., Celotti, A., Cerulli, R., Chen, A., Clay, R., Cocco, V., Conrad, J., Costa, E., Cuoco, A., Cusumano, G., Dai, C. J., Dawson, B., De Lotto, B., De Paris, G., Postigo, A. de Ugarte, Del Monte, E., Delgado, C., Di Ciaccio, A., Di Cocco, G., Di Falco, S., Di Persio, G., Dingus, B. L., Dominguez, A., Donato, F., Donnarumma, I., Doro, M., Edsjo, J., Navas, J. M. Espino, Santo, M. C. Espirito, Evangelista, Y., Evoli, C., Fargion, D., Favuzzi, C., Feroci, M., Fiorini, M., Foggetta, L., Fornengo, N., Froysland, T., Frutti, M., Fuschino, F., Gomez, J. L., Gomez, M., Gaggero, D., Galante, N., Gallardo, M. I., Galli, M., Garcia, J. E., Garczarczyk, M., Gargano, F., Gaug, M., Gianotti, F., Giarrusso, S., Giebels, B., Giglietto, N., Giommi, P., Giordano, F., Giuliani, A., Glicenstein, J., Goncalves, P., Grasso, D., Guerriero, M., He, H. L., Incicchitti, A., Kirk, J., Kuang, H. H., La Barbera, A., La Rosa, G., Labanti, C., Lamanna, G., Lapshov, I., Lazzarotto, F., Liberati, S., Liello, F., Lipari, P., Longo, F., Loparco, F., Lozano, M., De Sanctis, P. G. Lucentini, Ma, J. M., Maccarone, M. C., Maccione, L., Malvezzi, V., Mangano, A., Mariotti, M., Marisaldi, M., Martel, I., Masiero, A., Massaro, E., Mastropietro, M., Mattaini, E., Mauri, F., Mazziotta, M. N., Mereghetti, S., Mineo, T., Mizobuchi, S., Moiseev, A., Moles, M., Monte, C., Montecchia, F., Morelli, E., Morselli, A., Moskalenko, I., Nozzoli, F., Ormes, J. F., Peres-Torres, M. A., Pacciani, L., Pellizzoni, A., Perez-Bernal, F., Perotti, F., Picozza, P., Pieri, L., Pietroni, M., Pimenta, M., Pina, A., Pittori, C., Pontoni, C., Porrovecchio, G., Prada, F., Prest, M., Prosperi, D., Protheroe, R., Pucella, G., Quesada, J. M., Quintana, J. M., Quintero, J. R., Raino, S., Rapisarda, M., Rissi, M., Rodriguez, J., Rossi, E., Rowell, G., Rubini, A., Russo, F., Sanchez-Conde, M., Sacco, B., Scapin, V., Schelke, M., Segreto, A., Sellerholm, A., Sheng, X. D., Smith, A., Soffitta, P., Sparvoli, R., Spinelli, P., Stamatescu, V., Stark, L. S., Tavani, M., Thornton, G., Titarchuk, L. G., Tome, B., Traci, A., Trifoglio, M., Trois, A., Vallania, P., Vallazza, E., Vercellone, S., Vernetto, S., Vitale, V., Wild, N., Ye, Z. P., Zambra, A., Zandanel, F., and Zanello, D.
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Astrophysics ,General Relativity and Quantum Cosmology ,High Energy Physics - Phenomenology ,Physics - Space Physics - Abstract
This Conference is the fifth of a series of Workshops on High Energy Gamma- ray Experiments, following the Conferences held in Perugia 2003, Bari 2004, Cividale del Friuli 2005, Elba Island 2006. This year the focus was on the use of gamma-ray to study the Dark Matter component of the Universe, the origin and propagation of Cosmic Rays, Extra Large Spatial Dimensions and Tests of Lorentz Invariance., Comment: 328 pages, 7.8Mb, Proceedings of the 5th SCINEGHE Workshop, June 18-20, 2007 http://www.roma2.infn.it/SciNeGHE07/
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- 2007
79. Investigating electron interacting dark matter
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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., and Zhang, Y. J.
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Astrophysics - Abstract
Some extensions of the Standard Model provide Dark Matter candidate particles which can have a dominant coupling with the lepton sector of the ordinary matter. Thus, such Dark Matter candidate particles ($\chi^{0}$) can be directly detected only through their interaction with electrons in the detectors of a suitable experiment, while they are lost by experiments based on the rejection of the electromagnetic component of the experimental counting rate. These candidates can also offer a possible source of the 511 keV photons observed from the galactic bulge. In this paper this scenario is investigated. Some theoretical arguments are developed and related phenomenological aspects are discussed. Allowed intervals and regions for the characteristic phenomenological parameters of the considered model and of the possible mediator of the interaction are also derived considering the DAMA/NaI data., Comment: 16 pages, 6 figures. Accepted for publication in PRD. One typo corrected
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- 2007
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80. Possible implications of the channeling effect in NaI(Tl) crystals
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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., and Zhang, Y. J.
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Astrophysics - Abstract
The channeling effect of low energy ions along the crystallographic axes and planes of NaI(Tl) crystals is discussed in the framework of corollary investigations on WIMP Dark Matter candidates. In fact, the modeling of this existing effect implies a more complex evaluation of the luminosity yield for low energy recoiling Na and I ions. In the present paper related phenomenological arguments are developed and possible implications are discussed at some extent., Comment: 16 pages, 10 figures, preprint ROM2F/2007/15, submitted for publication
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- 2007
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81. On electromagnetic contributions in WIMP quests
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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., Sheng, X. D., and Ye, Z. P.
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Astrophysics - Abstract
The effect pointed out by A. B. Migdal in the 40's (hereafter named Migdal effect) has so far been usually neglected in the direct searches for WIMP Dark Matter candidates. This effect consists in the ionization and the excitation of bound atomic electrons induced by the recoiling atomic nucleus. In the present paper the related theoretical arguments are developed and some consequences of the proper accounting for this effect are discussed by some examples of practical interest., Comment: 14 pages, 6 figures, 2 tables, Int. J. Mod. Phys. A (in publication)
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- 2007
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82. Investigating halo substructures with annual modulation signature
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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., Sheng, X. D., Ye, Z. P., Martinez, M., and Giuffrida, G.
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Astrophysics - Abstract
Galaxy hierarchical formation theories, numerical simulations, the discovery of the Sagittarius Dwarf Elliptical Galaxy (SagDEG) in 1994 and more recent investigations suggest that the dark halo of the Milky Way can have a rich phenomenology containing non thermalized substructures. In the present preliminary study, we investigate the case of the SagDEG (the best known satellite galaxy in the Milky Way crossing the solar neighbourhood) analyzing the consequences of its dark matter stream contribution to the galactic halo on the basis of the DAMA/NaI annual modulation data. The present analysis is restricted to some WIMP candidates and to some of the astrophysical, nuclear and particle Physics scenarios. Other candidates such as e.g. the light bosonic ones, we discussed elsewhere, and other non thermalized substructures are not yet addressed here., Comment: 17 pages, 10 figures, to appear in Eur. Phys. J. C
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- 2006
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83. Investigating pseudoscalar and scalar dark matter
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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., and Ye, Z. P.
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Astrophysics - Abstract
In this paper another class of Dark Matter candidate particles: the pseudoscalar and scalar light bosonic candidates, is discussed. Particular care is devoted to the study of the processes for their detection (which only involves electrons and photons/X-rays) in a suitable underground experimental set-up. For this purpose the needed calculations are developed and various related aspects and phenomenologies are discussed. In particular, it is shown that - in addition to the WIMP cases already discussed elsewhere - there is also possibility for a bosonic candidate to account for the 6.3 sigma C.L. model independent evidence for the presence of a particle DM component in the galactic halo observed by DAMA/NaI. Allowed regions in these scenarios are presented also paying particular care on the cosmological interest of the bosonic candidate., Comment: 23 pages, 6 figures, 1 table, Int. J. Mod. Phys. A (in press)
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- 2005
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84. Dark Matter particles in the galactic halo: results and implications from DAMA/NaI
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Montecchia, F., Nozzoli, F., Incicchitti, A., Prosperi, D., Dai, C. J., Kuang, H. H., Ma, J. M., and Ye, Z. P.
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Astrophysics - Abstract
The DAMA/NaI experiment (about 100 kg highly radiopure NaI(Tl)) was proposed, designed and realised to effectively investigate in a model independent way the presence of a Dark Matter particle component in the galactic halo by exploiting the annual modulation signature. With a total exposure of 107731 kg day, collected over seven annual cycles deep underground at the Gran Sasso National Laboratory of the I.N.F.N., it has pointed out -- at 6.3 sigma C.L. -- an effect which satisfies all the peculiarities of the signature and neither systematic effects nor side reactions able to mimic the signature were found. Moreover, several (but still few with respect to the possibilities) corollary model dependent quests for the candidate particle have been carried out. In this paper the obtained results are summarized and some perspectives are discussed at some extent., Comment: 32 pages, 15 figures, 3 tables, in publication on Int. J. Mod. Phys. D
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- 2005
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85. Rivaroxaban or aspirin for patent foramen ovale and embolic stroke of undetermined source: a prespecified subgroup analysis from the NAVIGATE ESUS trial
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Abdelhamid, N, Abdul Rahman, D, Abdul-Saheb, M, Abreu, P, Abroskina, M, Abu Ahmad, F, Accassat, S, Acciaresi, M, Adami, A, Ahmad, N, Ahmed, F, Alberto Hawkes, M, Alemseged, F, Ali, A, Altavilla, R, Alwis, L, Amarenco, P, Amaro, S, Amaya Sanchez, LE, Amelia Pinto, A, Ameriso, SF, Amin, H, Amino, T, Amjad, AK, Anagnostou, E, Andersen, G, Anderson, C, Anderson, DC, Andrea Falco, M, Andres Mackinnon, F, Andreu, D, Androulakis, M, Angel Gamero, M, Angel Saredo, G, Angeles Diaz, R, Angels Font, M, Anticoli, S, Arauz, A, Arauz Gongora, AA, Araya, P, Arenillas Lara, JF, Arias Rivas, S, Arnold, M, Augustin, S, Avelar, W, Azevedo, E, Babikian, V, Bacellar, A, Badalyan, K, Bae, HJ, Baez Martinez, EM, Bagelmann, H, Bailey, P, Bak, Z, Baker, M, Balazs, A, Baldaranov, D, Balogun, I, Balueva, T, Bankuti, Z, Bar, M, Baranowska, A, Bardutzky, J, Barker Trejo, S, Barlinn, J, Baronnet, F, Barroso, C, Barteys, M, Bartolottiova, T, Barulin, A, Bas, M, Bashir, S, Basile, V, Bathe-Peters, R, Bathula, R, Batista, C, Batur Caglayan, H, Baumgartner, P, Bazan, R, Bazhenova, O, Beaudry, M, Beer, J, Behnam, Y, Beilei, C, Beinlich, A, Bejot, Y, Belkin, A, Benavente, OR, Benjamin, A, Berardi, V, Bereczki, D, Berkowitz, SD, Berlingieri, J, Berrios, W, Berrouschot, J, Bhandari, M, Bhargavah, M, Bicker, H, Bicsak, T, Bilik, M, Bindila, D, Birchenall, J, Birnbaum, L, Black, T, Blacker, D, Blacquiere, D, Blanc-Labarre, C, Blank, C, Blazejewska-Hyzorek, B, Bloch, S, Bodiguel, E, Bogdanov, E, Boos, L, Borcsik, L, Bornstein, N, Bouly, S, Braga, G, Bragado, I, Bravi, MC, Brokalaki, C, Brola, W, Brouns, R, Bruce, D, Brzoska-Mizgalska, J, Buck, B, Buksinska-Lisik, M, Burke, J, Burn, M, Bustamante, G, Cabrejo, L, Cai, K, Cajaraville, S, Calejo, M, Calvet, D, Campillo, J, Campos Costa, E, Camps, P, Can Alaydin, H, Candeloro, E, Canepa, C, Cantu Brito, CG, Cappellari, M, Carcel, C, Cardona Portela, P, Cardoso, F, Carek, M, Carletti, M, Carlos Portilla, J, Caruso, P, Casado-Naranjo, I, Castellini, P, Castro, D, Castro Meira, F, Cavallini, A, Cayuela Caudevilla, N, Cenciarelli, S, Cereda, C, Cerrone, P, Chakrabarti, A, Chaloulos-Iakovidis, P, Chamorro, A, Chandrasena, D, Chang, DI, Che, C, Chembala, J, Chen, J, Chen, Z, Chen, T, Chen, H, Chen, X, Chen, G, Chen, L, Chen, S, Cheripelli, B, Chin, M, Chiquete Anaya, E, Chorazy, M, Christensen, H, Christensen, T, Christian, L, Chu, F, Chung, CS, Clark, W, Clarke, R, Claverie, S, Clemente Agostoni, E, Clissold, B, Coelho, J, Cohen, D, Colakoglu, S, Collas, D, Condurso, R, Connolly, SJ, Consoli, D, Constantin, C, Constantino Silva, AB, Contardo, L, Corlobe, A, Correia, M, Correia, C, Cortijo Garcia, E, Coull, B, Coutts, S, Coveney, S, Cras, P, Crols, R, Crozier, S, Csanyi, A, Csiba, L, Csontos, K, Csuha, R, Cui, L, Cunha, L, Curtze, S, Czerska, M, Czlonkowska, A, Czurko, M, Czuryszkiewicz, M, Dagnino, M, Dai, C, Daineko, A, Dalek, G, Damgaard, D, Danese, A, Dani, K, Danku, V, Dario Toledo, W, Dávalos, A, De Havenon, A, De Keyser, J, De Klippel, N, De La Torre, J, De Pauw, A, De Smedt, A, De Torres, R, De Vries Basson, MM, Dearborn, J, Deganutto, R, Degeorgia, M, Deguchi, I, Del Giudice, A, Delcourt, C, Delgado-Mederos, R, Della Marca, G, Delpont, B, Deltour, S, Demets, DL, Dennis, M, Desai, J, Devine, J, Dhollander, I, Di Mascio, MT, Diaconu, M, Diaz Otero, F, Dietzel, J, Diez-Tejedor, E, Ding, N, Ding, J, Diomedi, M, Dioszeghy, P, Distefano, M, Domigo, V, Dorodnicov, E, Dossi, D, Doubal, F, Druzenko, I, Du, P, Du, J, Duman, T, Duodu, Y, Dutta, D, Dylewicz, L, Eckstein, J, Ehrensperger, E, Ehrlich, S, Einer Allende, G, Elena Halac, B, Elyas, S, Endres, M, Engelbrecht, JM, Engelter, S, Epinat, M, Eren, F, Esbjornsson, M, Escribano, B, Escudero, I, Esisi, B, Essa, B, Esterbauer, M, Evans, N, Eveson, D, Fabio, S, Fang, L, Fanta, S, Fares, M, Fatar, M, Faust, K, Favate, A, Fazekas, F, Federica Denaro, M, Fedin, A, Felipe Amaya, P, Feng, J, Ferencova, K, Fernanda Gilli, M, Fernandez, MD, Fernandez Pirrone, PN, Fernandez Vera, J, Ferrari, J, Ferreira, A, Ferreira Junior, G, Fidler, M, Field, D, Field, T, Figueroa, C, Fiksa, J, Filipov, A, Firstenfeld, A, Fisch, L, Fischer, U, Fisselier, M, Fiszer, U, Fluri, F, Fortea, G, Fotherby, K, Fraczek, A, France, E, Freitas, G, Frey, S, Frick, M, Friedman, A, Friedrich, M, Frisullo, G, Fryze, W, Fuentes Gimeno, B, Fujigasaki, H, Fukuyama, K, Furlan, A, Furlanis, G, Furnace, J, Gabriel, M, Gabriel Reich, E, Gagliardi, RJ, Galati, F, Galli Giqueauk, E, Gallina, A, Gallinella, E, Gallo, J, Gangadharan, S, Gao, Y, Garcia Lopez, R, Garcia Pastor, A, Garcia Sanchez, SM, Garnauf, M, Garnier, P, Gasecki, D, Gasic, K, Gasiorek, K, Gasser, S, Gaugg, M, Gebreyohanns, M, Gebura, K, Geng, J, Geniz Clavijo, M, Georg Haeusler, K, Geran, R, Geremek, M, Gerocs, Z, Ghia, D, Giannandrea, D, Giatsidis, F, Gien Lopez, JA, Gil Nunez, A, Gimenez, L, Giralt, E, Glabinski, A, Gladstone, D, Gliem, M, Gluszkiewicz, M, Goddeau, R, Gogoleva, E, Gokce, M, Goldemund, D, Golikov, K, Gomes Neto, A, Gomez Schneider, M, Gomez-Choco, M, Gomis, M, Gongora-Rivera, JF, Gonysheva, Y, Gonzalez, L, Gonzalez Toledo, ME, Gottschal, M, Gozdzik, I, Grabowski, S, Graf, S, Green, D, Greer, D, Gregorio, T, Greisenegger, S, Greshnova, I, Griebe, M, Grzesik, M, Guan, J, Guarda, S, Gueguen, A, Guidoux, C, Guillermo Povedano, P, Guillon, B, Guiraudg, V, Gunathilagan, G, Guryanova, N, Gusev, V, Gustavo Persi, G, Gutiérrez, R, Guyler, P, Gyuker, N, Hachinski, V, Hajas, A, Hallevi, H, Hankey, G, Hankey, GJ, Hanouskova, L, Hao, L, Haraguchi, K, Haralur Sreekantaiah, Y, Haratz, S, Hargroves, D, Harkness, K, Harmel, P, Harrasser, M, Hart, RG, Harvey, M, Hasan, R, Hasegawa, Y, Hassan, A, Hattori, M, Hatzitolios, A, Hauk, M, Hayashi, T, Hayhoe, H, Hedna, VS, Heine, M, Held, V, Hellwig, S, Henkner, J, Henninger, N, Hermans, S, Hernandez, J, Herrero, D, Hervieu-Begue, M, Herzig, R, Hicken, L, Hieber, M, Hill, M, Hirose, M, Hobeanu, MC, Hobson, B, Hochstetter, M, Hoe Heo, J, Hoffmann, M, Holmstedt, C, Hon, P, Hong, KS, Honma, Y, Horev, A, Horgan, G, Horvath, L, Horvath, M, Hoyer, C, Huang, D, Huang, H, Huber, B, Huhtakangas, J, Hussain, M, Igarashi, S, Iglesias Mohedano, AM, Ignacio Tembl, J, Impellizzeri, M, Inanc, Y, Ioli, P, Irina Aniculaesei, A, Ishida, K, Itabashi, R, Iversen, H, Jagolino, A, Jakab, K, Jander, S, Janka, H, Jankovych, J, Jansen, J, Jasek, L, Javier Alet, M, Javor, L, Jin, X, Jing, P, Joachim, B, Joan Macleod, M, Johnson, M, Jose Martin, J, Joyner, C, Judit Szabo, K, Jun-Oconnell, A, Jura, R, Kaczorowska, B, Kadlcikova, J, Kahles, T, Kakaletsis, N, Kakuk, I, Kalinowska, K, Kaminska, K, Kaneko, C, Kanellos, I, Kapeller, P, Kapica-Topczewska, K, Karasz, O, Karlinski, M, Karlsson, JE, Kasa, K, Kashaeva, E, Kasner, SE, Kaste, M, Kasza, J, Katalin Iljicsov, A, Katsurayama, M, Kaur, S, Kawanishi, M, Kaygorodtseva, S, Ke, K, Kei, A, Keilitz, J, Kellner, J, Kelly, P, Kelly, S, Kemlink, D, Kerekgyarto, M, Keskinarkaus, I, Khairutdinova, D, Khanna, A, Khaw, A, Kholopov, M, Khoumri, C, Kirpicheva, S, Kirshner, H, Kitagawa, K, Kittner, S, Kivioja, R, Klein, F, Kleindorfer, D, Kleinig, T, Klivenyi, P, Knecht, S, Kobayashi, Y, Kobayashi, A, Koch, M, Koehler, L, Koivu, M, Kolianov, V, Koltsov, I, Kondo, T, Konkov, I, Kopecky, S, Korompoki, E, Korpela, J, Kosarz-Lanczek, K, Koutroubi, A, Kovacs, K, Kovacs, T, Kovacs, H, Kowalczyk, K, Kowalska, M, Krajickova, D, Kral, M, Krarup Hansen, C, Kraska, J, Krebs, S, Krejci, V, Kremer, C, Kreuzpointer, R, Krzyzanowska, M, Kucken, D, Kulakowska, A, Kunzmann, J, Kurenkova, N, Kuris, A, Kurkowska-Jastrzebska, I, Kurtenkova, N, Kurushina, O, Kusnick, G, Kustova, M, Kuwashiro, T, Kwan Cha, J, Lago, A, Lagutenko, M, Lajos, B, Lambeck, J, Lamy, C, Landolfi, A, Lanfranconi, S, Lang, W, Lara Lezama, LB, Lara Rodriguez, B, Largo, T, Lasek-Bal, A, Latte, L, Lauer, V, Lavados, P, Le Bouc, R, Leal Cantu, R, Lechner, H, Lecouturier, K, Leder, S, Lee, J, Lee, BC, Leger, A, Leira, E, Leisse, I, Leker, R, Lembo, G, Lenskaya, L, Leyden, J, Li, G, Li, M, Li, S, Li, J, Liamis, G, Liang, H, Liang, Z, Ligot, N, Lin, H, Lindert, R, Lindgren, A, Linna, M, Litwin, T, Liu, K, Liu, X, Llull, L, Lohninger, B, Longoni, M, Loomis, C, Lopes, D, Lopez Fernandez, M, Lopez Garza, N, Lord, A, Louw, S, Lovasz, R, Lowenkopf, T, Lu, Z, Lubke-Detring, SC, Luder, R, Lujan, S, Luo, B, Lupinogina, L, Luschin, G, Lutsep, H, Lvova, A, Ly, J, Grosse, G.M., Ma, H, Ma, C, Machado, M, Machado, C, Macher, S, Machetanz, J, Macian-Montoro, F, Mackey, E, Mackey, A, Maclean, G, Maestre-Moreno, J, Magadan, A, Magyar, T, Mahagney, A, Majid, A, Majjhoo, A, Makaritsis, K, Mandzia, J, Mangas Guijarro, M, Mangion, D, Manios, E, Mann, S, Manning, L, Manno, C, Manuel Garcia, J, Maqueda, V, Mar Castellanos, M, Mar Freijo, M, Marando, C, Marcela Lepera, S, Marcos Couto, J, Maria Bruera, G, Maria Greco, L, Maria Lorenzo, A, Maria Obmann, S, Maria Roa, A, Marini, C, Marinkovic, I, Mario Sumay, G, Mario Torres, C, Marko, M, Markova, S, Markus, H, Marsh, R, Marsili, E, Marta Esnaola, M, Marta Moreno, J, Marti-Fabregas, J, Martina Angelocola, S, Martínez Sánchez, P, Martinez-Majander, N, Martins, S, Marzelik, O, Mastrocola, S, Matamala, G, Matoltsy, A, Matosevic, B, Matsumoto, S, Maud, A, Mauri Cabdevila, G, May, Z, Mayasi, Y, Mayr, A, Mazzoli, T, Mcarthur, K, Mccullough, L, Medina Pech, CE, Medlin, F, Mehdiratta, M, Mehta, S, Mehta, D, Mehta, B, Melis, M, Melnikova, E, Mendez, B, Mendonca, T, Mengual Chirifie, JJ, Menon, N, Mensch, A, Meseguer, E, Messe, S, Metcalf, K, Meyer, N, Michas, F, Micheletti, N, Mikulik, R, Milionis, H, Miller, B, Milling, T, Minelli, C, Minhas, J, Minns, M, Mircea, D, Mishra, S, Mismas, A, Mistri, A, Mitrovic, N, Miyake, H, Modrau, B, Moey, A, Molina, C, Molina, J, Molis, A, Moller, J, Molnar, S, Moniche, F, Monosi, C, Monzani, V, Moonis, M, Morais, R, Morales, L, Morales, A, Morar-Precup, D, Moreton, F, Moro, C, Morozova, E, Morton, M, Morvan, T, Morvan, E, Motko, T, Mowla, A, Mozhejko, E, Muddegowda, G, Mudhar, O, Mueller, T, Muhl, C, Muir, KW, Mundl, H, Munoz, S, Murphy, C, Murphy, S, Murtuzova, A, Musuka, T, Mutzenbach, J, Myint, M, Mysliwy, W, Naccarato, M, Naeije, G, Nagakane, Y, Natarajan, I, Navaratnam, D, Nave, A, Nazliel, B, Nedeltchev, K, Nel, J, Nell, H, Nemeth, R, Nemeth, L, Neto, O, Ng, K, Ngeh, J, Nicolas Chialvo, L, Nieminen, T, Nikkanen, M, Nikl, J, Nikoforova, M, Nishino, S, Nishiyama, Y, Njovane, X, Nogawa, S, Nombela, F, Norrving, B, Nosek, K, Nowak, B, Nowakowska-Sledz, E, Ntaios, G, Numminen, H, Nunez, F, Obadia, M, Oberndorfer, S, Obrezan, A, Ochiai, J, Oczkowski, W, O'Donnell, MJ, Odyniec, A, Oh, K, Ohira, M, Okamoto, Y, Okpala, M, Okubo, S, Olah, L, Olavarria, V, Oleszek, J, Onat Demirci, N, Ondar, V, Ongun, G, Ooyama, K, Orosz, V, Ortiz, R, Osseby, G, Österlund-Tauriala, E, Ovesen, C, Ozcekic Demirhan, S, Ozdoba-Rot, J, Ozturk, S, Ozyurt, E, Pablo Grecco, M, Pablo Povedano, G, Paciaroni, M, Padiglioni, C, Pagola, J, Palasik, W, Panczel, G, Panos, L, Papadopoulos, G, Papadopoulou, E, Papagiannis, A, Papavasileiou, V, Papina, M, Pardo De Donlebun, JR, Parisi, V, Park, JM, Pasten, J, Patel, N, Pavlik, O, Pawelczyk, M, Peacock, WF, Pei, H, Peisker, T, Pena Sedna, LF, Penn, A, Pentek, S, Pepper, E, Pereira, L, Perera, K, Perez, Y, Perez, S, Perez Leguizamon, P, Pernicka, M, Perry, R, Persico, A, Pesant, Y, Peska, S, Peters, D, Peters, G, Pettigrew, L, Phan, T, Philippi, S, Phinney, T, Pico, F, Pidal, A, Piechowski-Jozwiak, B, Pieroni, A, Pineiro, S, Piras, V, Pizova, N, Polanco, J, Polin, M, Polyakov, A, Polychronopoulou, E, Polymeris, A, Popov, D, Poppe, A, Postorino, P, Pozzerese, C, Pradhan, M, Prats, L, Prazdnichkova, E, Prendl, B, Pretorius, M, Profice, P, Prokopenko, S, Pudov, E, Pujol Lereis, V, Punzo Bravo, G, Purroy, F, Qiu, J, Qu, X, Quenardelle, V, Quesada Garcia, H, Radrizzani, L, Radtke, A, Raffelsberger, T, Ramirez Moreno, JM, Ramos-Estebanez, C, Rani, A, Rapantova, P, Rashed, K, Rasheed Nihara, A, Rasmussen, J, Redondo Robles, L, Reif, M, Reiner, P, Rekova, P, Renu, A, Repetto, M, Reyes, P, Reyes Morales, S, Rha, JH, Ribeiro, J, Ricci, S, Richard, C, Rigual, R, Rinaldi, C, Riveira Rodriguez, C, Rizzato, B, Robinson, TG, Rocco, A, Rodrigues, M, Rodriguez, G, Rodriguez Campello, A, Rodriguez Lucci, F, Rodriguez Yanez, M, Roesler, C, Roffe, C, Roine, R, Roine, S, Roldan, A, Romana Pezzella, F, Romano, M, Roos, JS, Rosso, C, Rostrup Kruuse, C, Roth, Y, Roukens, R, Roveri, L, Rozanski, D, Rozniecki, J, Rozsa, C, Rudilosso, S, Ruiz Ares, G, Ruiz Franco, A, Rum, G, Ruuskanen, J, Rybinnik, I, Ryota, K, Saarinen, J, Saavedra, V, Sabben, C, Sabet, A, Sagris, D, Sahlas, J, Sakai, N, Salamanca, P, Salgado, P, Salig, S, Salletmayr, T, Salnikov, M, Samoshkina, O, Samson, Y, Sanak, D, Sànchez Cerón, M, Santalucia, P, Santamaria Cadavid, M, Santiago, P, Santo, G, Sanz Cuesta, B, Sargento, J, Sarraj, A, Sas, K, Sas, A, Satoshi, O, Satsoglou, S, Sattar, N, Savitz, S, Savopoulos, C, Saw, J, Sawicka, M, Sawyer, R, Scandura, T, Schillinger, N, Schindler, J, Schlachetzki, F, Schneider, I, Schuppner, R, Schurig, J, Schwarzbach, CJ, Sebejova, M, Seidel, G, Sekaran, L, Selcuk, D, Selvarajah, J, Semerano, A, Semjen, J, Semushina, D, Sen, S, Seok Park, M, Serena, J, Serhat Tokgoz, O, Serles, W, Serrano, F, Sevin, M, Seynaeve, L, Shah, S, Shamalov, N, Shang, T, Sharma, M, Sharrief, A, Shazam Hussain, M, Shchukin, I, Shen, W, Shepeleva, E, Shinsuke, I, Shmonin, A, Shoamanesh, A, Shuaib, A, Shulga, A, Sibolt, G, Sibon, I, Sicilia, I, Siebert, M, Sieczkowska, E, Sila, C, Silva, AA, Silva, D, Silva, P, Silva, Y, Silvestrini, M, Simony, Z, Simpkins, A, Singh, B, Sinha, D, Sipos, I, Skoda, O, Skowron, P, Skowronska, M, Sliwinska, B, Slonkova, J, Smolkin, A, Smyth, A, Sobolewski, P, Sobota, A, Sohn, SI, Soldatov, M, Solganov, I, Soloveva, L, Solovyeva, E, Sonntag, N, Soors, P, Sorgun, M, Soriano, C, Spence, D, Spengos, K, Sposato, L, Staaf, G, Stadler, K, Stakhovskaya, L, Stamatelopoulos, K, Steinert, S, Stetkarova, I, Stiehm, M, Stocker, R, Stoinski, J, Stoll, A, Stotts, G, Stumpp, A, Sucapane, P, Suenaga, T, Sun, X, Sundararajan, S, Sung Kim, J, Suzuki, H, Svaneborg, N, Szasz, G, Szczuchniak, W, Szczyrba, S, Szegedi, N, Szekely, A, Szewczyk, Z, Szilagyi, G, Szlufik, S, Szoboszlai, K, Szpisjak, L, Sztajzel, R, Sztriha, L, Ta Wil, SE, Taggeselle, J, Takamatsu, K, Takao, M, Taki, W, Takizawa, S, Talahma, M, Tamayo, A, Tan, J, Tanne, D, Tapanainen, A, Tapiola, T, Tarasiuk, J, Tatlisumak, T, Tayal, A, Tcvetkova, S, Teal, P, Tejada Garcia, J, Tejada Meza, H, Tenora, D, Terceno, M, Terentiou, A, Tezcan, S, Thaler, D, Thomson, A, Thouvenot, E, Tiainen, M, Timberg, I, Timsit, S, Tinchon, A, Tirschwell, D, Togay Isikay, C, Tokunaga, K, Tolino, M, Toloza, C, Tomelleri, G, Tomoyuki, K, Tomppo, LM, Tong, Z, Tong, L, Toni, D, Torres, J, Tossavainen, C, Toth, G, Tountopoulou, A, Touze, E, Tovar, M, Toyoda, K, Trillo, S, Trommer, A, Tropepi, D, Tryambake, D, Tu, H, Tuetuencue, S, Tumova, R, Tumpula, O, Turc, G, Tutaj, A, Tynkkynen, J, Uchiyama, S, Uchwat, U, Uhrinyakova, L, Ulku Acar, R, Uluduz Ugurlu, D, Urra, X, Urui, S, Usero Ruiz, M, Vaclavik, D, Vahedi, K, Valikovics, A, Valpas, J, Van Acker, P, Van Daele, W, Vanderschueren, G, Vanina Jure, L, Varela, R, Varga, Z, Varvat, J, Varvyanskaya, N, Vasco Salgado, A, Vasko, P, Vass, L, Vassilopoulou, S, Vastagh, I, Vazquez, P, Vecsei, L, Veltkamp, R, Venti, M, Verdugo, M, Verocai, V, Veronica Marroquin, M, Veronica Simonsini, C, Veverka, T, Vigl, M, Vila, A, Vilar, C, Villanueva Osorio, JA, Virta, J, Vitkova, E, Voglsperger, B, Volna, J, Von Weitzel-Mudersbach, PA, Vora, N, Voznyuk, I, Wach-Klink, A, Wacongne, A, Walters, D, Wang, Y, Wang, J, Wang, L, Wang, X, Wang, W, Wang, N, Wang, D, Wang, H, Warnack, W, Wartenberg, K, Waters, R, Waters, M, Webb, T, Weber, J, Weiss, G, Weissenborn, K, Weitz, JI, Weller, B, Wen, G, Weng, G, Werner, P, Werring, D, Wester, P, Whiteley, W, Whiting, R, Wijeratne, T, Willems, C, Wilson, L, Wilson, C, Winder, T, Windt, J, Winkler, A, Winska-Tereszkiewicz, A, Wisniewska, A, Wittayer, M, Wlodek, A, Wojnarowska-Arendt, A, Wolf, M, Wolff, V, Wolter, C, Wong, A, Wook Nah, H, Worthmann, H, Wu, W, Wu, S, Wunderlich, S, Wurzinger, H, Wyse, DG, Xiao, B, Xiaopeng, W, Ximenez-Carrillo, A, Xiong, L, Xiong, Y, Xiong, W, Xu, Y, Xu, J, Xu, Z, Yalo, B, Yamada, T, Yamasaki, M, Yang, L, Yang, Y, Yang, X, Yang, Q, Yang, B, Yang, J, Yasuhiro, I, Yee Lam, M, Yegappan, C, Yip, S, Ylikallio, E, Ylikotila, P, Yongwon Jin, A, Yoon, BW, Yoshida, Y, Yperzeele, L, Yuan, H, Yuasa, H, Zalewska, J, Zanferrari, C, Zapata, E, Zboznovits, D, Zelenka, I, Zhang, C, Zhang, B, Zhang, S, Zhang, M, Zhang, X, Zhang, J, Zhao, L, Zhirnova, O, Zhou, L, Zielinska-Turek, J, Zinchenko, I, Ziomek, M, Zitzmann, A, Zweifler, R, Zwiernik, J, Kasner, Scott E, Swaminathan, Balakumar, Lavados, Pablo, Sharma, Mukul, Muir, Keith, Veltkamp, Roland, Ameriso, Sebastian F, Endres, Matthias, Lutsep, Helmi, Messé, Steven R, Spence, J David, Nedeltechev, Krassen, Perera, Kanjana, Santo, Gustavo, Olavarria, Veronica, Lindgren, Arne, Bangdiwala, Shrikant, Shoamanesh, Ashkan, Berkowitz, Scott D, Mundl, Hardi, Connolly, Stuart J, and Hart, Robert G
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- 2018
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86. Optimizing best management practices for nutrient pollution control in a lake watershed under uncertainty
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Dai, C., Qin, X.S., Tan, Q., and Guo, H.C.
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- 2018
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87. Dealing with equality and benefit for water allocation in a lake watershed: A Gini-coefficient based stochastic optimization approach
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Dai, C., Qin, X.S., Chen, Y., and Guo, H.C.
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- 2018
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88. DAMA/NaI results
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Bernabei, R., Belli, P., Cappella, F., Montecchia, F., Nozzoli, F., Incicchitti, A., Prosperi, D., Cerulli, R., Dai, C. J., Kuang, H. H., Ma, J. M., and Ye, Z. P.
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Astrophysics - Abstract
The DAMA/NaI set-up of the DAMA experiment has been operative during seven annual cycles and has investigated several rare processes. In particular, it has been realised in order to investigate the model independent annual modulation signature for Dark Matter particles in the galactic halo. With the total exposure collected in the seven annual cycles (107731 kg day) a model independent evidence for the presence of a Dark Matter particle component in the galactic halo has been pointed out at 6.3 sigma C.L.. Some of the many possible corollary model dependent quests for the candidate particle have been presented as well., Comment: Contributed paper to the Rencontres de Moriond "Electroweak Interactions and Unified Theories", La Thuile, Aosta Valley, Italy, March 2004
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- 2004
89. Results from DAMA/NaI and perspectives for DAMA/LIBRA
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Bernabei, R., Belli, P., Cappella, F., Montecchia, F., Nozzoli, F., Incicchitti, A., Prosperi, D., Cerulli, R., Dai, C. J., Kuang, H. H., Ma, J. M., and Ye, Z. P.
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Astrophysics - Abstract
The about 100 kg highly radiopure NaI(Tl) set-up of the DAMA project (DAMA/NaI) took data over seven annual cycles up to July 2002 and has achieved results on various rare processes. Its main aim has actually been the exploitation of the model independent WIMP annual modulation signature. After this conference the total exposure, collected during the seven annual cycles, was released. This cumulative exposure (107731 kg day) has given a model independent evidence for the presence of a Dark Matter particle component in the galactic halo at 6.3 sigma C.L.; this main result is summarised here. Some of the many possible corollary model dependent quests for the candidate particle are mentioned. At present, after about five years of new developments, a second generation low background set-up (DAMA/LIBRA with a mass of about 250 kg NaI(Tl)) was built and is taking data since March 2003. New R&D efforts toward a possible NaI(Tl) ton set-up, we proposed in 1996, have been funded and started in 2003., Comment: Contributed paper to the Conf. "Beyond the Desert 03", Rindberg Castle, Germany, June 2003
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- 2003
90. Dark Matter search
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Montecchia, F., Nozzoli, F., Incicchitti, A., Prosperi, D., Dai, C. J., Kuang, H. H., Ma, J. M., and Ye, Z. P.
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Astrophysics ,High Energy Physics - Experiment - Abstract
Main arguments on the Dark Matter particle direct detection approach are addressed on the basis of the work and of the results of the about 100 kg highly radiopure NaI(Tl) DAMA experiment (DAMA/NaI), which has been operative at the Gran Sasso National Laboratory of the I.N.F.N. for more than one decade, including the preparation. The effectiveness of the WIMP model independent annual modulation signature is pointed out by discussing the results obtained over 7 annual cycles (107731 kg day total exposure); the WIMP presence in the galactic halo is strongly supported at 6.3 standard deviation C.L. The complexity of the corollary model dependent quests for a candidate particle is also addressed and several of the many possible scenarios are examined., Comment: 77 pages, 32 figures
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- 2003
91. DAMA results
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Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Montecchia, F., Nozzoli, F., Incicchitti, A., Prosperi, D., Dai, C. J., Kuang, H. H., Ma, J. M., and Ye, Z. P.
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Astrophysics ,High Energy Physics - Experiment ,High Energy Physics - Phenomenology - Abstract
DAMA is an observatory for rare processes based on the development and use of various kinds of radiopure scintillators. Several low background set-ups have been realized with passing and many rare processes have been investigated. Main activities are briefly summarized in the following and the main arguments on the results achieved in the investigation of the WIMP annual modulation signature are addressed. Next perspectives are also mentioned., Comment: Contributed paper to X International Workshop on "Neutrino Telescopes", Venice 2003, ROM2F/2003/9
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- 2003
92. Quenching Evolution in a Quantum-Classical Hybrid System
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Shen, J., Wang, W., Dai, C. M., and Yi, X. X.
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- 2019
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93. WIMP Search by DAMA at Gran Sasso
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Bernabei, R., Amato, M., Belli, P., Cappella, F., Cerulli, R., Dai, C. J., He, H. L., Ignesti, G., Incicchitti, A., Kuang, H. H., Ma, J. M., Montecchia, F., Nozzoli, F., and Prosperi, D.
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Astrophysics - Abstract
DAMA is searching for rare processes by developing and using several kinds of radiopure scintillators: in particular, NaI(Tl), liquid Xenon and CaF$_2$(Eu). Here only the results released so far on the WIMP annual modulation signature are summarized and compared with results from other experiments, including the recent re-analysis of CDMS-I data. Next perspectives are also shortly addressed., Comment: Talk at DARK2002 Conference, Cape Town, South Africa, 4-9 Feb 2002
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- 2002
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94. WIMP search by the DAMA experiment at Gran Sasso
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Belli, P., Bernabei, R., Amato, M., Cappella, F., Cerulli, R., Dai, C. J., He, H. L., Ignesti, G., Incicchitti, A., Kuang, H. H., Ma, J. M., Montecchia, F., Nozzoli, F., and Prosperi, D.
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High Energy Physics - Phenomenology ,Astrophysics ,High Energy Physics - Experiment - Abstract
DAMA is searching for rare processes by developing and using several kinds of radiopure scintillators: in particular, NaI(Tl), liquid Xenon and CaF$_2$(Eu). The main results are here summarized with particular attention to the investigation of the WIMP annual modulation signature., Comment: Talk at COSMO-01 Workshop, Rovaniemi, Finland, August 30 - September 4, 2001
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- 2001
95. Prognostic values of HE4 expression in patients with cancer: a meta-analysis
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Dai C, Zheng Y, Li Y, Tian T, Wang M, Xu P, Deng Y, Hao Q, Wu Y, Zhai Z, Dai Z, and Lyu J
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HE4 ,cancer ,prognosis ,meta-analysis ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Cong Dai,1,2,* Yi Zheng,2,* Yuanjie Li,3 Tian Tian,2 Meng Wang,2 Peng Xu,2 Yujiao Deng,2 Qian Hao,2 Ying Wu,2 Zhen Zhai,2 Zhijun Dai,2 Jun Lyu1 1Clinical Research Center, First Affiliated Hospital of Xi’an Jiaotong University, Xi’an, Shaanxi, 710061, People’s Republic of China; 2Department of Oncology, Second Affiliated Hospital of Xi’an Jiaotong University, Xi’an, Shaanxi, 710004, People’s Republic of China; 3Department of Human Anatomy, Histology and Embryology, School of Basic Medical Sciences, Xi’an Jiaotong University, Xi’an, Shaanxi 710061, People’s Republic of China *These authors contributed equally to this work Background: To evaluate the prognostic impact of HE4 expression in patients with cancer.Materials and methods: We searched the PubMed, Web of Science, Chinese National Knowledge Infrastructure and WangFang databases for publications concerning HE4 expression in patients with cancer. The correlation of HE4 expression level with overall survival (OS), disease-free survival (DFS), and progression-free survival (PFS) was analyzed.Results: In this meta-analysis, 29 studies, with a total of 4,235 patients, were included. Our results showed that HE4 expression was significantly associated with poorer OS (hazard ratio [HR] =2.15, 95% confidence interval [CI] =1.77–2.62, P
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- 2018
96. Pooling analysis on prognostic value of PHH3 expression in cancer patients
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Hao Q, Dai C, Deng Y, Xu P, Tian T, Lin S, Wang M, Liu K, Song D, Wu Y, Guo Y, and Dai Z
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PHH3 ,prognosis ,human cancer ,meta-analysis ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Qian Hao,1,* Cong Dai,1,* Yujiao Deng,1,* Peng Xu,1 Tian Tian,1 Shuai Lin,1 Meng Wang,1 Kang Liu,1 Dingli Song,1 Ying Wu,1 Yan Guo,2 Zhijun Dai1 1Department of Oncology, Second Affiliated Hospital of Xi’an Jiaotong University, Xi’an, People’s Republic of China; 2School of Life Science and Technology, Xi’an Jiaotong University, Xi’an, People’s Republic of China *These authors contributed equally to this work Background: Various studies have evaluated the significance of phospho-histone-H3 (PHH3) expression in cancer patients, but controversy over its reliability remains. We conducted a meta-analysis to summarize the prognostic relevance of PHH3 expression in cancer patients. Patients and methods: Nineteen studies, including 4803 patients, were identified by searching PubMed, Web of Science, Embase, and Cochrane Library. The correlation of PHH3 expression level with overall survival (OS), disease-free survival, and recurrence-free survival was analyzed. Results: Overall, the results suggest that high expression of PHH3 can predict a poor OS (HR=2.66, 95% CI=1.74–4.08, P
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- 2018
97. Dark Matter: DAMA/LIBRA and its perspectives
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Bernabei, Rita, primary, Belli, Pierluigi, additional, Cappella, Fabio, additional, Caracciolo, Vincenzo, additional, Cerulli, R., additional, Dai, C. J., additional, d'Angelo, A., additional, Incicchitti, Antonella, additional, Leoncini, Alice, additional, Ma, X. H., additional, Merlo, Vittorio, additional, Montecchia, F., additional, Sheng, X. D., additional, and Ye, Z. P., additional
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- 2023
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98. Influence of Blowing Ratio on Flow Structures of an Inclined Jet in Crossflow
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Jia, L., Dai, C., Zhang, J., Mi, J., Zhou, Yu, editor, Lucey, A.D., editor, Liu, Yang, editor, and Huang, Lixi, editor
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- 2016
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99. Formation and Evolution of the Flow Structure of an Inclined Jet in Crossflow
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Dai, C., Jia, L., Zhang, J., Mi, J., Zhou, Yu, editor, Lucey, A.D., editor, Liu, Yang, editor, and Huang, Lixi, editor
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- 2016
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100. A test of a phenomenological model of size dependent melting in Au nanoparticles
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Dai, C., Saidi, P., Song, H., Yao, Z., Daymond, M.R., and Hoyt, J.J.
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- 2017
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