The controllable electron-heating by external magnetic fields at relativistic laser-solid interactions in the presence of large scale pre-plasmas
The controllable electron-heating by external magnetic fields at relativistic laser-solid interactions in the presence of large scale pre-plasmas
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在存在大规模前等离子体的情况下,相对论性激光-固体相互作用中外部磁场的可控电子加热
DOI:
10.1088/1361-6587/aa69a9
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发表时间:
2016-02
影响因子:
2.2
通讯作者:
He X. T.
中科院分区:
文献类型:
--
作者:
Wu D.;Luan S. X.;Wang J. W.;Yu W.;Gong J. X.;Cao L. H.;Zheng C. Y.;He X. T.
The two-stage electron acceleration/heating model (Wu et al 2017 Nucl. Fusion 57 016007 and Wu et al 2016 Phys. Plasmas 23 123116) is extended to the study of laser magnetized-plasmas interactions at relativistic intensities and in the presence of large-scale preformed plasmas. It is shown that the electron-heating efficiency is a controllable value by the external magnetic fields. Detailed studies indicate that for a right-hand circularly polarized laser, the electron heating efficiency depends on both strength and directions of external magnetic fields. The electron-heating is dramatically enhanced when the external magnetic field is of B ≡ ω c / ω 0 > 1 . When magnetic field is of negative direction, i.e. B < 0 , it trends to suppress the electron heating. The underlining physics—the dependences of electron-heating on both the strength and directions of the external magnetic fields—is uncovered. With − ∞ < B < 1 , the electron-heating is explained by the synergetic effects by longitudinal charge separation electric field and the reflected ‘envelop-modulated’ CP laser. It is indicated that the ‘modulation depth’ of reflected CP laser is significantly determined by the external magnetic fields, which will in turn influence the efficiency of the electron-heating. While with B > 1 , a laser front sharpening mechanism is identified at relativistic laser magnetized-plasmas interactions, which is responsible for the dramatical enhancement of electron-heating.
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影响因子:
4
作者:
Zhuo, H. B.;Ma, Y. Y.;Shao, F. Q.;Borghesi, M.
通讯作者:
Borghesi, M.
DOI:
10.1103/physreve.95.023207
发表时间:
2016-07
期刊:
Physical review. E
影响因子:
--
作者:
D. Wu;Xiangqun He;W. Yu;S. Fritzsche
通讯作者:
D. Wu;Xiangqun He;W. Yu;S. Fritzsche
影响因子:
4
作者:
Zhu B. J.;Li Y. T.;Yuan D. W.;Li Y. F.;Li F.;Liao G. Q.;Zhao J. R.;Zhong J. Y.;Xue F. B.;He S. K.;Wang W. W.;Lu F.;Zhang F. Q.;Yang L.;Zhou K. N.;Xie N.;Hong W.;Wei H. G.;Zhang K.;Han B.;Pei X. X.;Liu C.;Zhang Z.;Wang W. M.;Zhu J. Q.;Gu Y. Q.;Zhao Z. Q.;Z
通讯作者:
Z
影响因子:
8.6
作者:
Wang W. -M.;Gibbon P.;Sheng Z. -M.;Li Y. -T.
通讯作者:
Li Y. -T.
影响因子:
2.2
作者:
D. Wu;D. Wu;B. Qiao;B. Qiao;C. McGuffey;Xiantu He;F. Beg
通讯作者:
D. Wu;D. Wu;B. Qiao;B. Qiao;C. McGuffey;Xiantu He;F. Beg