# Search for Light Weakly-Interacting-Massive-Particle Dark Matter by   Annual Modulation Analysis with a Point-Contact Germanium Detector at the   China Jinping Underground Laboratory

**Authors:** L. T. Yang, H. B. Li, Q. Yue, H. Ma, K. J. Kang, Y. J. Li, H. T. Wong,, M. Agartioglu, H. P. An, J. P. Chang, J. H. Chen, Y. H. Chen, J. P. Cheng, Z., Deng, Q. Du, H. Gong, Q. J. Guo, L. He, J. W. Hu, Q. D. Hu, H. X. Huang, L., P. Jia, H. Jiang, H. Li, J. M. Li, J. Li, X. Li, X. Q. Li, Y. L. Li, B. Liao,, F. K. Lin, S. T. Lin, S. K. Liu, Y. D. Liu, Y. Y. Liu, Z. Z. Liu, J. L. Ma,, Y. C. Mao, H. Pan, J. Ren, X. C. Ruan, V. Sharma, Z. She, M. B. Shen, L., Singh, M. K. Singh, T. X. Sun, C. J. Tang, W. Y. Tang, Y. Tian, G. F. Wang,, J. M. Wang, L. Wang, Q. Wang, Y. Wang, Y. X. Wang, S. Y. Wu, Y. C. Wu, H. Y., Xing, Y. Xu, T. Xue, N. Yi, C. X. Yu, H. J. Yu, J. F. Yue, X. H. Zeng, M., Zeng, Z. Zeng, F. S. Zhang, Y. H. Zhang, M. G. Zhao, J. F. Zhou, Z. Y. Zhou,, J. J. Zhu, Z. H. Zhu

arXiv: 1904.12889 · 2019-11-27

## TL;DR

This study uses a germanium detector at China Jinping Underground Laboratory to search for light WIMP dark matter via annual modulation, setting new limits and excluding certain parameter regions with high confidence.

## Contribution

It provides the first annual modulation analysis for light WIMPs with a germanium detector at this scale, achieving the best sensitivity below 6 GeV/c^2.

## Key findings

- Excluded DAMA/LIBRA and CoGeNT AM regions at >99.99% and 98% C.L.
- Set new upper limits on WIMP-nucleus cross sections for masses below 6 GeV/c^2.
- Achieved the most sensitive AM measurement for light WIMPs to date.

## Abstract

We present results on light weakly interacting massive particle (WIMP) searches with annual modulation (AM) analysis on data from a 1-kg mass $p$-type point-contact germanium detector of the CDEX-1B experiment at the China Jinping Underground Laboratory. Datasets with a total live time of 3.2 yr within a 4.2 yr span are analyzed with analysis threshold of 250 eVee. Limits on WIMP-nucleus (${\chi}$-$N$) spin-independent cross sections as function of WIMP mass ($m_{\chi}$) at 90\% confidence level (C.L.) are derived using the dark matter halo model. Within the context of the standard halo model, the 90\% C.L. allowed regions implied by the DAMA/LIBRA and CoGeNT AM-based analysis are excluded at $>$99.99\% and 98\% C.L., respectively. These results correspond to the best sensitivity at $m_{\chi}$$<$6$~{\rm GeV}/c^2$ among WIMP AM measurements to date.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1904.12889/full.md

## References

39 references — full list in the complete paper: https://tomesphere.com/paper/1904.12889/full.md

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Source: https://tomesphere.com/paper/1904.12889