CRESST-III实验关于低质量暗物质的首批结果
宇宙学与河外天体物理
2017-11-22 v1 天体物理仪器与方法
摘要
CRESST实验位于意大利格兰萨索国家实验室，通过暗物质粒子在靶材料中的弹性散射来搜寻暗物质粒子。CRESST靶由闪烁的CaWO晶体组成，作为低温量热计在毫开尔文温度下运行。CaWO靶晶体中的每次相互作用都会产生一个声子信号和一个由第二个低温量热计测量的光信号。自2015年CRESST-II结果以来，该实验一直引领着质量低于1.7\,GeV/的暗物质直接搜寻领域，将直接搜寻的范围扩展到亚GeV/质量区域。对于2016年7月启动第一阶段的CRESST-III，探测器已优化以达到进一步以空前灵敏度探测低质量区域所需的性能。本报告中将讨论CRESST-III探测器的成果以及第一阶段的初步结果和展望。
引用
@article{arxiv.1711.07692,
title = {First results on low-mass dark matter from the CRESST-III experiment},
author = {CRESST collaboration and F. Petricca and G. Angloher and P. Bauer and A. Bento and C. Bucci and L. Canonica and X. Defay and A. Erb and F. v. Feilitzsch and N. Ferreiro Iachellini and P. Gorla and A. Gütlein and D. Hauff and J. Jochum and M. Kiefer and H. Kluck and H. Kraus and J. C. Lanfranchi and A. Lagenkämper and J. Loebell and M. Mancuso and E. Mondragon and A. Münster and C. Pagliarone and W. Potzel and F. Pröbst and R. Puig and F. Reindl and J. Rothe and K. Schäffner and J. Schieck and S. Schönert and W. Seidel and M. Stahlberg and L. Stodolsky and C. Strandhagen and R. Strauss and A. Tanzke and H. H. Trinh Thi and C. Türkoğlu and A. Ulrich and I. Usherov and S. Wawoczny and M. Willers and M. Wüstrich},
journal= {arXiv preprint arXiv:1711.07692},
year = {2017}
}
备注
XV International Conference on Topics in Astroparticle and Underground Physics, TAUP2017, submitted to Journal of Physics: Conference Series (JPCS)