Abstract
Light (sub-GeV) dark matter has gained increasing interest in terms of direct detection. Accelerated dark matter is a promising candidate that can generate detectable nuclear recoil energy within the sub-GeV range. Because of the large kinetic energy, its interactions with the nucleus are predominantly governed by inelastic scattering, including quasi-elastic and deep inelastic scattering. In this work, we calculated the inelastic effects in dark matter-Earth scattering mediated by a vector particle. Our analysis revealed that the impact of inelastic scattering relies on the mediator mass and the kinetic energy spectrum of dark matter. The results exhibited considerable disparity: the upper bounds of the exclusion limit for the spin-independent cross-section between accelerated dark matter and nuclei via a heavy mediator differ by several tens of times when inelastic scattering is considered.
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References
R. L. Workman, et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2022, 083C01 (2022).
B. W. Lee, and S. Weinberg, Phys. Rev. Lett. 39, 165 (1977).
G. Jungman, M. Kamionkowski, and K. Griest, Phys. Rep. 267, 195 (1996).
Y. Meng, et al. (PandaX-4T Collaboration), Phys. Rev. Lett. 127, 261802 (2021), arXiv: 2107.13438.
J. Aalbers, et al. (LUX-ZEPLIN Collaboration), Phys. Rev. Lett. 131, 041002 (2023), arXiv: 2207.03764.
E. Aprile, et al. (XENON Collaboration), Phys. Rev. Lett. 131, 041003 (2023), arXiv: 2303.14729.
R. Essig, J. Mardon, and T. Volansky, Phys. Rev. D 85, 076007 (2012), arXiv: 1108.5383.
Y. Hochberg, Y. Zhao, and K. M. Zurek, Phys. Rev. Lett. 116, 011301 (2016), arXiv: 1504.07237.
R. Essig, M. Fernández-Serra, J. Mardon, A. Soto, T. Volansky, and T. T. Yu, J. High Energ. Phys. 5, 046 (2016).
R. Essig, T. Volansky, and T. T. Yu, Phys. Rev. D 96, 043017 (2017), arXiv: 1703.00910.
S. Knapen, T. Lin, and K. M. Zurek, Phys. Rev. D 96, 115021 (2017), arXiv: 1709.07882.
G. Bertone, and T. M. P. Tait, Nature 562, 51 (2018), arXiv: 1810.01668.
R. T. D’Agnolo, C. Mondino, J. T. Ruderman, and P. J. Wang, J. High Energ. Phys. 2018(08), 79 (2018).
J. Yang, A. Abdukerim, W. Chen, X. Chen, Y. Chen, C. Cheng, X. Cui, Y. Fan, D. Fang, C. Fu, M. Fu, L. Geng, K. Giboni, L. Gu, X. Guo, K. Han, C. He, S. He, D. Huang, Y. Huang, R. Huo, Y. Huang, Z. Huang, X. Ji, Y. Ju, S. Li, Q. Lin, H. Liu, J. Liu, X. Lu, W. Ma, Y. Ma, Y. Mao, Y. Meng, N. Shaheed, K. Ni, J. Ning, X. Ning, X. Ren, C. Shang, G. Shen, L. Si, A. Tan, A. Wang, H. Wang, M. Wang, Q. H. Wang, S. Wang, W. Wang, X. Wang, Z. Wang, M. Wu, S. Wu, W. Wu, J. Xia, M. Xiao, X. Xiao, P. Xie, B. Yan, Y. Yang, C. Yu, H. B. Yu, J. Yuan, Y. Yuan, X. Zeng, D. Zhang, T. Zhang, L. Zhao, Q. Zheng, J. Zhou, N. Zhou, X. Zhou, and PandaX-II Collaboration, Sci. China-Phys. Mech. Astron. 64, 111062 (2021), arXiv: 2104.14724.
L. Su, L. Wu, and B. Zhu, Phys. Rev. D 105, 055021 (2022), arXiv: 2105.06326.
R. Calabrese, M. Chianese, D. F. G. Fiorillo, and N. Saviano, Phys. Rev. D 105, L021302 (2022), arXiv: 2107.13001.
G. Elor, R. McGehee, and A. Pierce, Phys. Rev. Lett. 130, 031803 (2023).
H. B. Yang, X. Q. Li, Y. H. Yu, Y. Chen, J. Kong, Y. J. Zhang, S. W. Tang, J. H. Guo, B. Yang, F. J. Su, W. J. Sun, J. X. Wang, and C. X. Zhao, Nucl. Sci. Tech. 33, 65 (2022).
R. Calabrese, M. Chianese, D. F. G. Fiorillo, and N. Saviano, Phys. Rev. D 105, 103024 (2022), arXiv: 2203.17093.
A. Ambrosone, M. Chianese, D. F. G. Fiorillo, A. Marinelli, and G. Miele, Phys. Rev. Lett. 131, 111003 (2023), arXiv: 2210.05685.
P. W. Graham, D. E. Kaplan, S. Rajendran, and M. T. Walters, Phys. Dark Universe 1, 32 (2012), arXiv: 1203.2531.
Y. Hochberg, T. Lin, and K. M. Zurek, Phys. Rev. D 95, 023013 (2017), arXiv: 1608.01994.
I. M. Bloch, R. Essig, K. Tobioka, T. Volansky, and T. T. Yu, J. High Energ. Phys. 2017(06), 087 (2017).
R. M. J. Li, S. K. Liu, S. T. Lin, L. T. Yang, Q. Yue, C. H. Fang, H. T. Jia, X. Jiang, Q. Y. Li, Y. Liu, Y. L. Yan, K. K. Zhao, L. Zhang, C. J. Tang, H. Y. Xing, and J. J. Zhu, Nucl. Sci. Tech. 33, 57 (2022).
Y. Gu, L. Wu, and B. Zhu, Phys. Rev. D 106, 075004 (2022), arXiv: 2203.06664.
H. T. Jia, S. T. Lin, S. K. Liu, H. C. Chi, M. Deniz, C. H. Fang, P. Gu, X. Jiang, Y. K. Shu, Q. Y. Li, Y. Liu, R. M. J. Li, C. K. Qiao, C. J. Tang, H. T. K. Wong, H. Y. Xing, L. T. Yang, Q. Yue, Y. L. Yan, K. K. Zhao, and J. J. Zhu, Nucl. Sci. Tech. 33, 157 (2022).
Y. Hochberg, T. Lin, and K. M. Zurek, Phys. Rev. D 94, 015019 (2016), arXiv: 1604.06800.
Y. Hochberg, I. Charaev, S. W. Nam, V. Verma, M. Colangelo, and K. K. Berggren, Phys. Rev. Lett. 123, 151802 (2019), arXiv: 1903.05101.
S. M. Griffin, Y. Hochberg, K. Inzani, N. Kurinsky, T. Lin, and T. C. Yu, Phys. Rev. D 103, 075002 (2021), arXiv: 2008.08560.
Y. Hochberg, B. V. Lehmann, I. Charaev, J. Chiles, M. Colangelo, S. W. Nam, and K. K. Berggren, Phys. Rev. D 106, 112005 (2022), arXiv: 2110.01586.
C. Kouvaris, and J. Pradler, Phys. Rev. Lett. 118, 031803 (2017), arXiv: 1607.01789.
C. McCabe, Phys. Rev. D 96, 043010 (2017), arXiv: 1702.04730.
E. Aprile, et al. (XENON Collaboration), Phys. Rev. Lett. 123, 241803 (2019), arXiv: 1907.12771.
G. G. di Cortona, A. Messina, and S. Piacentini, J. High Energ. Phys. 2020(11), 34 (2020).
J. D. Vergados, and H. Ejiri, Phys. Lett. B 606, 313 (2005), arXiv: hep-ph/0401151.
C. C. Moustakidis, J. D. Vergados, and H. Ejiri, Nucl. Phys. B 727, 406 (2005), arXiv: hep-ph/0507123.
M. Ibe, W. Nakano, Y. Shoji, and K. Suzuki, J. High Energ. Phys. 2018(03), 194 (2018).
M. J. Dolan, F. Kahlhoefer, and C. McCabe, Phys. Rev. Lett. 121, 101801 (2018), arXiv: 1711.09906.
D. Baxter, Y. Kahn, and G. Krnjaic, Phys. Rev. D 101, 076014 (2020), arXiv: 1908.00012.
R. Essig, J. Pradler, M. Sholapurkar, and T. T. Yu, Phys. Rev. Lett. 124, 021801 (2020), arXiv: 1908.10881.
N. F. Bell, J. B. Dent, J. L. Newstead, S. Sabharwal, and T. J. Weiler, Phys. Rev. D 101, 015012 (2020), arXiv: 1905.00046.
Z. L. Liang, L. Zhang, F. Zheng, and P. Zhang, Phys. Rev. D 102, 043007 (2020), arXiv: 1912.13484.
K. D. Nakamura, K. Miuchi, S. Kazama, Y. Shoji, M. Ibe, and W. Nakano, Prog. Theor. Exp. Phys. 1, 013C01 (2021), arXiv: 2009.05939.
Z. L. Liang, C. Mo, F. Zheng, and P. Zhang, Phys. Rev. D 104, 056009 (2021), arXiv: 2011.13352.
V. V. Flambaum, L. Su, L. Wu, and B. Zhu, Sci. China-Phys. Mech. Astron. 66, 271011 (2023).
J. F. Acevedo, J. Bramante, and A. Goodman, Phys. Rev. D 105, 023012 (2022), arXiv: 2108.10889.
W. Wang, K. Y. Wu, L. Wu, and B. Zhu, Nucl. Phys. B 983, 115907 (2022), arXiv: 2112.06492.
N. F. Bell, J. B. Dent, R. F. Lang, J. L. Newstead, and A. C. Ritter, Phys. Rev. D 105, 096015 (2022), arXiv: 2112.08514.
P. Cox, M. J. Dolan, C. McCabe, and H. M. Quiney, Phys. Rev. D 107, 035032 (2023).
K. V. Berghaus, A. Esposito, R. Essig, and M. Sholapurkar, J. High Energ. Phys. 2023(01), 23 (2023).
J. Li, L. Su, L. Wu, and B. Zhu, J. Cosmol. Astropart. Phys. 4, 020 (2023), arXiv: 2210.15474.
D. Adams, D. Baxter, H. Day, R. Essig, and Y. Kahn, Phys. Rev. D 107, L041303 (2023), arXiv: 2210.04917.
N. F. Bell, P. Cox, M. J. Dolan, J. L. Newstead, and A. C. Ritter, arXiv: 2305.04690.
M. Qiao, C. Xia, and Y. F. Zhou, J. Cosmol. Astropart. Phys. 2023(11), 079 (2023), arXiv: 2307.12820.
T. Bringmann, and M. Pospelov, Phys. Rev. Lett. 122, 171801 (2019), arXiv: 1810.10543.
Y. Ema, F. Sala, and R. Sato, Phys. Rev. Lett. 122, 181802 (2019), arXiv: 1811.00520.
C. V. Cappiello, and J. F. Beacom, Phys. Rev. D 100, 103011 (2019), arXiv: 1906.11283.
W. Wang, L. Wu, J. M. Yang, H. Zhou, and B. Zhu, J. High Energ. Phys. 2020(12), 72 (2020).
S. F. Ge, J. Liu, Q. Yuan, and N. Zhou, Phys. Rev. Lett. 126, 091804 (2021), arXiv: 2005.09480.
C. Xia, Y. H. Xu, and Y. F. Zhou, Nucl. Phys. B 969, 115470 (2021), arXiv: 2009.00353.
Y. Ema, F. Sala, and R. Sato, SciPost Phys. 10, 072 (2021), arXiv: 2011.01939.
N. F. Bell, J. B. Dent, B. Dutta, S. Ghosh, J. Kumar, J. L. Newstead, and I. M. Shoemaker, Phys. Rev. D 104, 076020 (2021), arXiv: 2108.00583.
J. C. Feng, X. W. Kang, C. T. Lu, Y. L. S. Tsai, and F. S. Zhang, J. High Energ. Phys. 2022(04), 080 (2022).
W. Wang, L. Wu, W. N. Yang, and B. Zhu, Phys. Rev. D 107, 073002 (2023).
X. Cui, et al. (PandaX-II Collaboration), Phys. Rev. Lett. 128, 171801 (2022), arXiv: 2112.08957.
T. N. Maity, and R. Laha, arXiv: 2210.01815.
K. I. Nagao, S. Higashino, T. Naka, and K. Miuchi, J. Cosmol. Astropart. Phys. 2023(07), 061 (2023), arXiv: 2211.13399.
K. Agashe, Y. Cui, L. Necib, and J. Thaler, J. Cosmol. Astropart. Phys. 2014(10), 062 (2014), arXiv: 1405.7370.
J. Berger, Y. Cui, and Y. Zhao, J. Cosmol. Astropart. Phys. 2015(02), 005 (2015), arXiv: 1410.2246.
K. Agashe, Y. Cui, L. Necib, and J. Thaler, J. Phys.-Conf. Ser. 718, 042041 (2016), arXiv: 1512.03782.
J. Alvey, M. D. Campos, M. Fairbairn, and T. You, Phys. Rev. Lett. 123, 261802 (2019), arXiv: 1905.05776.
L. Su, W. Wang, L. Wu, J. M. Yang, and B. Zhu, Phys. Rev. D 102, 115028 (2020), arXiv: 2006.11837.
C. A. Arguëlles, V. Muñoz, I. M. Shoemaker, and V. Takhistov, Phys. Lett. B 833, 137363 (2022), arXiv: 2203.12630.
L. Darmé, Phys. Rev. D 106, 055015 (2022), arXiv: 2205.09773.
M. Du, R. Fang, and Z. Liu. arXiv: 2211.11469.
H. Sieber, D. V. Kirpichnikov, I. V. Voronchikhin, P. Crivelli, S. N. Gninenko, M. M. Kirsanov, N. V. Krasnikov, L. Molina-Bueno, and S. K. Sekatskii, Phys. Rev. D 108, 056018 (2023), arXiv: 2305.09015.
C. Kouvaris, and I. M. Shoemaker, Phys. Rev. D 90, 095011 (2014), arXiv: 1405.1729.
R. Foot, and S. Vagnozzi, Phys. Lett. B 748, 61 (2015), arXiv: 1412.0762.
B. J. Kavanagh, R. Catena, and C. Kouvaris, J. Cosmol. Astropart. Phys. 2017(01), 012 (2017), arXiv: 1611.05453.
B. J. Kavanagh, Phys. Rev. D 97, 123013 (2018), arXiv: 1712.04901.
J. Alvey, T. Bringmann, and H. Kolesova, J. High Energ. Phys. 2023(01), 123 (2023).
L. Su, L. Wu, N. Zhou, and B. Zhu, Phys. Rev. D 108, 035004 (2023), arXiv: 2212.02286.
X. Ning, et al. (PandaX Collaboration), Phys. Rev. Lett. 131, 041001 (2023), arXiv: 2301.03010.
C. A. Argüelles, A. Diaz, A. Kheirandish, A. Olivares-Del-Campo, I. Safa, and A. C. Vincent, Rev. Mod. Phys. 93, 035007 (2021), arXiv: 1912.09486.
M. J. Boschini, S. D. Torre, M. Gervasi, D. Grandi, G. Jóhannesson, M. Kachelriess, G. L. Vacca, N. Masi, I. V. Moskalenko, E. Orlando, S. S. Ostapchenko, S. Pensotti, T. A. Porter, L. Quadrani, P. G. Rancoita, D. Rozza, and M. Tacconi, Astrophys. J. 840, 115 (2017), arXiv: 1704.06337.
G. Guo, Y. L. S. Tsai, M. R. Wu, and Q. Yuan, Phys. Rev. D 102, 103004 (2020), arXiv: 2008.12137.
M. Fabbrichesi, E. Gabrielli, and G. Lanfranchi, arXiv: 2005.01515.
J. B. Dent, L. M. Krauss, J. L. Newstead, and S. Sabharwal, Phys. Rev. D 92, 063515 (2015), arXiv: 1505.03117.
D. Aristizabal Sierra, V. De Romeri, and N. Rojas, Phys. Rev. D 98, 075018 (2018), arXiv: 1806.07424.
A. Buckley, J. Ferrando, S. Lloyd, K. Nordström, B. Page, M. Rüfenacht, M. Schönherr, and G. Watt, Eur. Phys. J. C 75, 132 (2015), arXiv: 1412.7420.
R. Abdul Khalek, R. Gauld, T. Giani, E. R. Nocera, T. R. Rabemananjara, and J. Rojo, Eur. Phys. J. C 82, 507 (2022).
O. Benhar, N. Farina, H. Nakamura, M. Sakuda, and R. Seki, Phys. Rev. D 72, 053005 (2005), arXiv: hep-ph/0506116.
A. M. Ankowski, and J. T. Sobczyk, Phys. Rev. C 74, 054316 (2006), arXiv: nucl-th/0512004.
A. M. Ankowski, and J. T. Sobczyk, Phys. Rev. C 77, 044311 (2008), arXiv: 0711.2031.
A. M. Ankowski, O. Benhar, T. Mori, R. Yamaguchi, and M. Sakuda, Phys. Rev. Lett. 108, 052505 (2012), arXiv: 1110.0679.
A. M. Ankowski, and O. Benhar, Phys. Rev. D 88, 093004 (2013), arXiv: 1305.2068.
O. Benhar, D. Day, and I. Sick, Rev. Mod. Phys. 80, 189 (2008), arXiv: nucl-ex/0603029.
W. F. McDonough, Treatise on Geochemistry, In: H. D. Holland, and K. K. Turekian, eds. (Pergamon, Oxford, 2003), pp. 547–568.
J. Lundberg, and J. Edsjö, Phys. Rev. D 69, 123505 (2004), arXiv: astro-ph/0401113.
V. Gluscevic, and K. K. Boddy, Phys. Rev. Lett. 121, 081301 (2018), arXiv: 1712.07133.
W. L. Xu, C. Dvorkin, and A. Chael, Phys. Rev. D 97, 103530 (2018), arXiv: 1802.06788.
J. Ooba, H. Tashiro, and K. Kadota, J. Cosmol. Astropart. Phys. 2019(09), 020 (2019), arXiv: 1902.00826.
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This work was supported by the National Natural Science Foundation of China (Grant Nos. 12275134, 12275232, and 12335005). We are grateful to Artur M. Ankowski for a useful discussion.
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Su, L., Wu, L. & Zhu, B. An improved bound on accelerated light dark matter. Sci. China Phys. Mech. Astron. 67, 221012 (2024). https://doi.org/10.1007/s11433-023-2244-7
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DOI: https://doi.org/10.1007/s11433-023-2244-7