| ELECTROMAGNETISM, OPTICS, ACOUSTICS, HEAT TRANSFER, CLASSICAL MECHANICS, AND FLUID DYNAMICS |
Prev
Next
|
|
|
Transition signatures for electron-positron pair creation in space-time inhomogeneous electric field |
| Chuan-Ke Li(李传可)1, Xian-Xian Zhou(周鲜鲜)2, Qiang Chen(陈强)3, Bang An(安邦)4, Ying-Jun Li(李英骏)4,5, Nan-Sheng Lin(林南省)5,†, and Yang Wan(万阳)1,‡ |
1 Laboratory of Zhongyuan Light, School of Physics, Zhengzhou University, Zhengzhou 450001, China; 2 School of Management Science and Engineering, Anhui University of Finance and Economics, Bengbu 233030, China; 3 National Supercomputing Center in Zhengzhou, Zhengzhou University, Zhengzhou 450001, China; 4 State Key Laboratory for Tunnel Engineering, China University of Mining and Technology, Beijing 100083, China; 5 School of Science, China University of Mining and Technology, Beijing 100083, China |
|
|
|
|
Abstract The process of electron–positron pair creation through multi-photon absorption in a space–time dependent electric field is analyzed using computational quantum field theory. Our findings reveal two distinct pair creation channels: the symmetric and asymmetric transition channels. We propose that the asymmetric transition channel arises from the inherent spatial inhomogeneity of intense laser pulses. By mapping the field-theoretical model of laser-assisted multi-photon pair creation onto a quantum-mechanical time-dependent framework, a semi-analytical solution that captures the asymmetric transition signatures of vacuum decay is derived. Additionally, it is demonstrated that neglecting spatial inhomogeneity leads to erroneous transition amplitudes and incorrect identification of pair creation channels. Furthermore, we have established that asymmetric transition channels substantially enhance the creation of electron–positron pairs for a given laser pulse energy.
|
Received: 24 October 2025
Revised: 20 December 2025
Accepted manuscript online: 25 December 2025
|
|
PACS:
|
42.25.Bs
|
(Wave propagation, transmission and absorption)
|
| |
03.65.-w
|
(Quantum mechanics)
|
| |
12.20.-m
|
(Quantum electrodynamics)
|
|
| Fund: Project supported by the National Natural Science Foundation of China (NSFC) (Grant Nos. 12447120 and 12204001) and the Natural Science Foundation of Henan Province, China (Grant No. 252300423526). |
Corresponding Authors:
Nan-Sheng Lin, Yang Wan
E-mail: phy.nslin@gmail.com;yangwan23@zzu.edu.cn
|
Cite this article:
Chuan-Ke Li(李传可), Xian-Xian Zhou(周鲜鲜), Qiang Chen(陈强), Bang An(安邦), Ying-Jun Li(李英骏), Nan-Sheng Lin(林南省), and Yang Wan(万阳) Transition signatures for electron-positron pair creation in space-time inhomogeneous electric field 2026 Chin. Phys. B 35 054201
|
[1] Di Piazza A, Muller C, Hatsagortsyan K Z and Keitel C H 2012 Rev. Mod. Phys. 84 1177 [2] Fedotov A, Ilderton A, Karbsteinet F, King B, Seiptc D, Taya H and Torgrimsson G 2023 Phys. Rep. 1010 1 [3] Yu T P, Liu K, Zhao J, Zhu X L, Lu Y, Cao Y, Zhang H, Shao F Q and Sheng Z M 2024 Rev. Mod. Plasma Phys. 8 24 [4] Schwinger J 1951 Phys. Rev. 82 664 [5] Jin W Y, Yeong G K, Ⅱ W C, Sung J H, Lee H W, Lee S K and Nam C H 2021 Optica 8 630 [6] Brezin E and Itzykson C 1970 Phys. Rev. D 2 1191 [7] Burke D L, Field R C, Horton-Smithet G, Spencer J E, Walz D, Berridge S C, Bugg W M, Shmakov K, Weidemann A W, Bula C, McDonald K T, Prebys E J, Bamber C, Boege S J, Koffas T, Kotseroglou T, Melissinos A C, Meyerhofer D D, Reis D A and Ragg W 1997 Phys. Rev. Lett. 79 1626 [8] See https://eli-laser.eu. [9] See https://corels.ibs.re.kr. [10] See https://facet.slac.stanford.edu. [11] Keitel C H, Di Piazza A, Paulus G G, Stoehlker T, Clark E L, Mangles S, Najmudin Z, Krushelnick K, Schreiber J, Borghesi M, Dromey B, Geissler M, Riley D, Sarri G and Zepf M 2021 arXiv: 2103.06059 [physics.plasm-ph] [12] See http://www.hibef.eu. [13] Li W Q, Gan Z B, Yu L H, Wang C, Liu Y Q, Guo Z, Xu L, Xu M, Hang Y, Xu Y, Wang J Y, Huang P, Cao H, Yao B, Zhang X B, Chen L R, Tang Y H, Li S, Liu X Y, Li S M, He M Z, Yin D J, Liang X Y, Leng Y X, Li R X and Xu Z Z 2018 Opt. Lett. 43 5681 [14] Bulanov S S, Narozhny N B, Mur V D and Popov V S 2006 J. Exp. Theor. Phys. 102 9 [15] Kohlfurst C, Gies H and Alkofer R 2014 Phys. Rev. Lett. 112 050402 [16] H. Taya, T. Fujimori, T. Misumi, Nitta M and Sakai N 2021 J. High Energ. Phys. 2021 82 [17] Jiang R Z, Gong C, Li Z L and Li Y J 2023 Phys. Rev. D 108 076015 [18] Hu L N, Amat O, Wang L, Sawut A, Fan H H and Xie B S 2023 Phys. Rev. D 107 116010 [19] Ruf M, Mocken G R, Muller C, Hatsagortsyan K Z and Keitel C H 2009 Phys. Rev. Lett. 102 080402 [20] Krajewska K and Kaminski J Z 2010 Phy. Rev. A 82 013420 [21] Kohlfurst C and Alkofer R 2018 Phys. Rev. D 97 036026 [22] Lv Q Z, Dong S, Li Y T, Sheng Z M, Su Q and Grobe R 2018 Phys. Rev. A 97 022515 [23] Kohlfurst C 2020 Phys. Rev. D 101 096003 [24] Chen Q, Xiao J Y and Fan P F 2021 J. High Energ. Phys. 2021 127 [25] Wang L, Li L J, Mohamedsedik M, An R, Li J J, Xie B S and Zhang F S 2023 Chin. Phys. B 32 010301 [26] Li C K, Lin N S, Zhou X X, Jiang M, Li Y J 2023 Chin. Phys. B 32 094202 [27] Wollert A, Bauke H and Keitel C H 2015 Phys. Rev. D 91 125026 [28] Jiang J J, Dai Y N, Zhuang K H, Gao Y Q, Tang S and Chen Y Y 2024 Phys. Rev. D 109 036030 [29] Amat O, Fan H H, Tang S, Huang Y F and Xie B S 2025 Phys. Rev. D 111 056020 [30] Chen Z Y, Amat O, Bai J H and Bake M A 2025 Phys. Rev. D 111 116005 [31] Li Y F, Chen Y Y, Wang W M and Hu H S 2020 Phys. Rev. Lett. 125 044802 [32] Song H H, Wang W M, Li Y F, Li B J, Li Y T, Sheng Z M and Zhang J 2021 New J. Phys. 23 075005 [33] Song H H, Wang W M and Li Y T 2022 Phys. Rev. Lett. 129 035001 [34] Xue K, Sun T, Wei K J, Li Z P, Zhao Q, Wan F, Lv C, Zhao Y T, Xu Z F and Li J X 2023 Phys. Rev. Lett. 131 175101 [35] Zhu X L, Liu W Y, Yu T P, Chen M, Weng S M, Wang W M and Sheng Z M 2024 Phys. Rev. Lett. 132 235001 [36] Song H H, Wang W M and Li Y T 2021 Phys. Rev. Research 3 033245 [37] Bechler A, Cajiao Velez F, Krajewska K and Kami nski J Z 2023 Acta Phys. Pol. A 143 S18 [38] Majczak M M, Krajewska K and Kaminski J Z and Bechler A 2024 Phys. Rev. D 110 116025 [39] Fan H H, Zhang C W, Tang T and Xie B S 2025 Phys. Rev. D 111 076017 [40] Jiang M, Grobe R and Su Q 2023 Phys. Rev. A 108 022813 [41] Krekora P, Su Q and Grobe R 2004 Phys. Rev. Lett. 92 040406 [42] Cheng T, Su Q and Grobe R 2010 Cont. Phys. 51 315 [43] Li C K, Su D D, Li Y J, Su Q and Grobe R 2023 Europhys. Lett. 141 55001 [44] Gerry C C, Su Q and Grobe R 2006 Phys. Rev. A 74 044103 [45] Mocken G R, Ruf M, Muller C and Keitel C H 2010 Phys. Rev. A 81 022122 [46] Xie B S, Li Z L and Tang S 2017 Matter and Radiation at Extremes 2 225 |
| No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|