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Constraints on dark matter boosted by supernova shock within the effective field theory framework from the CDEX-10 experiment

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Wang, J. Z., Yang, L. T., Yue, Q., Kang, K. J., Li, Y. J., An, H. P., C., Greeshma, Chang, J. P., Chen, H., Chen, Y. H., Cheng, J. P., Dai, W. H., Deng, Z., Fang, C. H., Geng, X. P., Gong, H., Guo, Q. J., Guo, T., Guo, X. Y., He, L., He, J. R., Huang, H. X., Huang, T. C., Karmakar, S., Li, H. B., Li, H. Y., Li, J. M., Li, J., Li, M. C., Li, Q. Y., Li, R. M. J., Li, X. Q., Li, Y. L., Liang, Y. F., Liao, B., Lin, F. K., Lin, S. T., Liu, J. X., Liu, R. Z., Liu, S. K., Liu, Y. D., Liu, Y., Liu, Y. Y., Ma, H., Mao, Y. C., Mureed, A., Nie, Q. Y., Pan, H., Qi, N. C., Ren, J., Ruan, X. C., Shen, M. B., Shi, H. Y., Singh, M. K., Sun, T. X., Sun, W. L., Tang, C. J., Tian, Y., Wan, H. F., Wang, G. F., Wang, L., Wang, Q., Wang, Y. F., Wang, Y. X., Wong, H. T., Wu, Y. C., Xing, H. Y., Xiong, K. Z., Xu, R., Xu, Y., Xue, T., Yan, Y. L., Yi, N., Yu, C. X., Yu, H. J., Yu, X., Zeng, M., Zeng, Z., Zhang, F. S., Zhang, P., Zhang, Z. H., Zhang, Z. Y., Zhao, M. G., Zhou, J. F., Zhou, Z. Y., Zhu, J. J.
Natura:	Preprint
Pubblicazione:	2025
Soggetti:	High Energy Physics - Phenomenology High Energy Physics - Experiment Instrumentation and Detectors
Accesso online:	Acceder al recurso
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author	Wang, J. Z. Yang, L. T. Yue, Q. Kang, K. J. Li, Y. J. An, H. P. C., Greeshma Chang, J. P. Chen, H. Chen, Y. H. Cheng, J. P. Dai, W. H. Deng, Z. Fang, C. H. Geng, X. P. Gong, H. Guo, Q. J. Guo, T. Guo, X. Y. He, L. He, J. R. Huang, H. X. Huang, T. C. Karmakar, S. Li, H. B. Li, H. Y. Li, J. M. Li, J. Li, M. C. Li, Q. Y. Li, R. M. J. Li, X. Q. Li, Y. L. Liang, Y. F. Liao, B. Lin, F. K. Lin, S. T. Liu, J. X. Liu, R. Z. Liu, S. K. Liu, Y. D. Liu, Y. Liu, Y. Y. Ma, H. Mao, Y. C. Mureed, A. Nie, Q. Y. Pan, H. Qi, N. C. Ren, J. Ruan, X. C. Shen, M. B. Shi, H. Y. Singh, M. K. Sun, T. X. Sun, W. L. Tang, C. J. Tian, Y. Wan, H. F. Wang, G. F. Wang, L. Wang, Q. Wang, Q. Wang, Y. F. Wang, Y. X. Wong, H. T. Wu, Y. C. Xing, H. Y. Xiong, K. Z. Xu, R. Xu, Y. Xue, T. Yan, Y. L. Yi, N. Yu, C. X. Yu, H. J. Yu, X. Zeng, M. Zeng, Z. Zhang, F. S. Zhang, P. Zhang, Z. H. Zhang, Z. Y. Zhao, M. G. Zhou, J. F. Zhou, Z. Y. Zhu, J. J.
author_facet	Wang, J. Z. Yang, L. T. Yue, Q. Kang, K. J. Li, Y. J. An, H. P. C., Greeshma Chang, J. P. Chen, H. Chen, Y. H. Cheng, J. P. Dai, W. H. Deng, Z. Fang, C. H. Geng, X. P. Gong, H. Guo, Q. J. Guo, T. Guo, X. Y. He, L. He, J. R. Huang, H. X. Huang, T. C. Karmakar, S. Li, H. B. Li, H. Y. Li, J. M. Li, J. Li, M. C. Li, Q. Y. Li, R. M. J. Li, X. Q. Li, Y. L. Liang, Y. F. Liao, B. Lin, F. K. Lin, S. T. Liu, J. X. Liu, R. Z. Liu, S. K. Liu, Y. D. Liu, Y. Liu, Y. Y. Ma, H. Mao, Y. C. Mureed, A. Nie, Q. Y. Pan, H. Qi, N. C. Ren, J. Ruan, X. C. Shen, M. B. Shi, H. Y. Singh, M. K. Sun, T. X. Sun, W. L. Tang, C. J. Tian, Y. Wan, H. F. Wang, G. F. Wang, L. Wang, Q. Wang, Q. Wang, Y. F. Wang, Y. X. Wong, H. T. Wu, Y. C. Xing, H. Y. Xiong, K. Z. Xu, R. Xu, Y. Xue, T. Yan, Y. L. Yi, N. Yu, C. X. Yu, H. J. Yu, X. Zeng, M. Zeng, Z. Zhang, F. S. Zhang, P. Zhang, Z. H. Zhang, Z. Y. Zhao, M. G. Zhou, J. F. Zhou, Z. Y. Zhu, J. J.
contents	Supernova shocks can boost dark matter (DM) particles to high, yet nonrelativistic, velocities, providing a suitable mechanism for analysis within the framework of the nonrelativistic effective field theory (NREFT). These accelerated DM sources extend the experimental ability to scan the parameter space of light DM into the sub-GeV region. In this study, we specifically analyze DM accelerated by the Monogem Ring supernova remnant, whose age ($\sim 68000$ yr) and distance to Earth ($\sim 300$ parsec) are strategically matched to enable detection with current terrestrial detectors. Utilizing the 205.4 kg$\cdot$day data obtained from the CDEX-10 experiment at the China Jinping Underground Laboratory, we derive new constraints on boosted DM within the NREFT framework. The NREFT coupling constant exclusion regions now penetrate the sub-GeV mass range, with optimal sensitivity achieved for operators $\mathcal{O}_{3}$, $\mathcal{O}_{6}$, $\mathcal{O}_{15}$ in the 0.4--0.6 GeV mass range.
format	Preprint
id	arxiv_https___arxiv_org_abs_2504_03559
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	Constraints on dark matter boosted by supernova shock within the effective field theory framework from the CDEX-10 experiment Wang, J. Z. Yang, L. T. Yue, Q. Kang, K. J. Li, Y. J. An, H. P. C., Greeshma Chang, J. P. Chen, H. Chen, Y. H. Cheng, J. P. Dai, W. H. Deng, Z. Fang, C. H. Geng, X. P. Gong, H. Guo, Q. J. Guo, T. Guo, X. Y. He, L. He, J. R. Huang, H. X. Huang, T. C. Karmakar, S. Li, H. B. Li, H. Y. Li, J. M. Li, J. Li, M. C. Li, Q. Y. Li, R. M. J. Li, X. Q. Li, Y. L. Liang, Y. F. Liao, B. Lin, F. K. Lin, S. T. Liu, J. X. Liu, R. Z. Liu, S. K. Liu, Y. D. Liu, Y. Liu, Y. Y. Ma, H. Mao, Y. C. Mureed, A. Nie, Q. Y. Pan, H. Qi, N. C. Ren, J. Ruan, X. C. Shen, M. B. Shi, H. Y. Singh, M. K. Sun, T. X. Sun, W. L. Tang, C. J. Tian, Y. Wan, H. F. Wang, G. F. Wang, L. Wang, Q. Wang, Q. Wang, Y. F. Wang, Y. X. Wong, H. T. Wu, Y. C. Xing, H. Y. Xiong, K. Z. Xu, R. Xu, Y. Xue, T. Yan, Y. L. Yi, N. Yu, C. X. Yu, H. J. Yu, X. Zeng, M. Zeng, Z. Zhang, F. S. Zhang, P. Zhang, Z. H. Zhang, Z. Y. Zhao, M. G. Zhou, J. F. Zhou, Z. Y. Zhu, J. J. High Energy Physics - Phenomenology High Energy Physics - Experiment Instrumentation and Detectors Supernova shocks can boost dark matter (DM) particles to high, yet nonrelativistic, velocities, providing a suitable mechanism for analysis within the framework of the nonrelativistic effective field theory (NREFT). These accelerated DM sources extend the experimental ability to scan the parameter space of light DM into the sub-GeV region. In this study, we specifically analyze DM accelerated by the Monogem Ring supernova remnant, whose age ($\sim 68000$ yr) and distance to Earth ($\sim 300$ parsec) are strategically matched to enable detection with current terrestrial detectors. Utilizing the 205.4 kg$\cdot$day data obtained from the CDEX-10 experiment at the China Jinping Underground Laboratory, we derive new constraints on boosted DM within the NREFT framework. The NREFT coupling constant exclusion regions now penetrate the sub-GeV mass range, with optimal sensitivity achieved for operators $\mathcal{O}_{3}$, $\mathcal{O}_{6}$, $\mathcal{O}_{15}$ in the 0.4--0.6 GeV mass range.
title	Constraints on dark matter boosted by supernova shock within the effective field theory framework from the CDEX-10 experiment
topic	High Energy Physics - Phenomenology High Energy Physics - Experiment Instrumentation and Detectors
url	https://arxiv.org/abs/2504.03559