Detecting «dark matter» using a liquid xenon scintillation detector
暂无分享，去创建一个
[1] P. Belli,et al. Performances of a detector for high precision monitoring of a low energy γ-ray beam , 1989 .
[2] D. Hoppe,et al. Total Synthesis of Protected D-altro- and D-galacto-3,6-Dideoxy-3-C-methylhexoses; Key Intermediates of a Rifamycin S Synthesis , 1989 .
[3] Griest,et al. Calculations of rates for direct detection of neutralino dark matter. , 1988, Physical review letters.
[4] Caldwell,et al. Laboratory limits on galactic cold dark matter. , 1988, Physical review letters.
[5] V. Trimble. Dark matter in the universe: where, what, and why? , 1988 .
[6] M. Spiro,et al. Experimental particle physics without accelerators , 1987 .
[7] I. Barabanov,et al. Liquid xenon scintillation spectrometer , 1987 .
[8] W. Press,et al. Solar models with energy transport by weakly interacting particles , 1986 .
[9] Goodman,et al. Detectability of certain dark-matter candidates. , 1985, Physical review. D, Particles and fields.
[10] T. O. Niinikoski,et al. Low-temperature calorimetry for rare decays , 1984 .
[11] J. Ostriker,et al. The Mass distribution within our Galaxy: A Three component model , 1981 .
[12] D. Freedman. Coherent effects of a weak neutral current , 1974 .