Constraints on Spin-Independent Nucleus Scattering with sub-GeV Weakly Interacting Massive Particle Dark Matter from the CDEX-1B Experiment at the China Jinping Underground Laboratory

Constraints on Spin-Independent Nucleus Scattering with sub-GeV Weakly Interacting Massive Particle Dark Matter from the CDEX-1B Experiment at the China Jinping Underground Laboratory

We report results on the searches of weakly interacting massive particles (WIMPs) with sub-GeV masses (mχ) via WIMP-nucleus spin-independent scattering with Migdal effect incorporated. Analysis on time-integrated (TI) and annual modulation (AM) effects on CDEX-1B data are performed, with 737.1 kg da...

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Veröffentlicht in:Physical review letters 2019-10, Vol.123 (16), p.1-161301, Article 161301
Hauptverfasser: Liu, Z. Z., Yue, Q., Yang, L. T., Kang, K. J., Li, Y. J., Wong, H. T., Agartioglu, M., An, H. P., Chang, J. P., Chen, J. H., Chen, Y. H., Cheng, J. P., Deng, Z., Du, Q., Gong, H., Guo, X. Y., Guo, Q. J., He, L., He, S. M., Hu, J. W., Hu, Q. D., Huang, H. X., Jia, L. P., Jiang, H., Li, H. B., Li, H., Li, J. M., Li, J., Li, X., Li, X. Q., Li, Y. L., Liao, B., Lin, F. K., Lin, S. T., Liu, S. K., Liu, Y. D., Liu, Y. Y., Ma, H., Ma, J. L., Mao, Y. C., Ning, J. H., Pan, H., Qi, N. C., Ren, J., Ruan, X. C., Sharma, V., She, Z., Singh, L., Singh, M. K., Sun, T. X., Tang, C. J., Tang, W. Y., Tian, Y., Wang, G. F., Wang, L., Wang, Q., Wang, Y., Wang, Y. X., Wu, S. Y., Wu, Y. C., Xing, H. Y., Xu, Y., Xue, T., Yi, N., Yu, C. X., Yu, H. J., Yue, J. F., Zeng, M., Zeng, Z., Zhang, F. S., Zhao, M. G., Zhou, J. F., Zhou, Z. Y., Zhu, J. J.
Format: Artikel
Sprache:eng
Schlagworte:
Confidence intervals
Dark matter
Scattering
Weakly interacting massive particles
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Beschreibung
Zusammenfassung:We report results on the searches of weakly interacting massive particles (WIMPs) with sub-GeV masses (mχ) via WIMP-nucleus spin-independent scattering with Migdal effect incorporated. Analysis on time-integrated (TI) and annual modulation (AM) effects on CDEX-1B data are performed, with 737.1 kg day exposure and 160 eVee threshold for TI analysis, and 1107.5 kg day exposure and 250 eVee threshold for AM analysis. The sensitive windows in mχ are expanded by an order of magnitude to lower DM masses with Migdal effect incorporated. New limits on σχNSI at 90% confidence level are derived as 2×10−32∼7×10−35  cm2 for TI analysis at mχ∼50–180  MeV/c2, and 3×10−32∼9×10−38  cm2 for AM analysis at mχ∼75  MeV/c2–3.0  GeV/c2.
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.123.161301