underdense plasma
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2021 ◽  
Vol 28 (12) ◽  
pp. 122104
Author(s):  
P. Valenta ◽  
G. M. Grittani ◽  
C. M. Lazzarini ◽  
O. Klimo ◽  
S. V. Bulanov

2021 ◽  
Vol 87 (3) ◽  
Author(s):  
Nicolas Crouseilles ◽  
Paul-Antoine Hervieux ◽  
Yingzhe Li ◽  
Giovanni Manfredi ◽  
Yajuan Sun

We propose a numerical scheme to solve the semiclassical Vlasov–Maxwell equations for electrons with spin. The electron gas is described by a distribution function $f(t,{\boldsymbol x},{{{\boldsymbol p}}}, {\boldsymbol s})$ that evolves in an extended 9-dimensional phase space $({\boldsymbol x},{{{\boldsymbol p}}}, {\boldsymbol s})$ , where $\boldsymbol s$ represents the spin vector. Using suitable approximations and symmetries, the extended phase space can be reduced to five dimensions: $(x,{{p_x}}, {\boldsymbol s})$ . It can be shown that the spin Vlasov–Maxwell equations enjoy a Hamiltonian structure that motivates the use of the recently developed geometric particle-in-cell (PIC) methods. Here, the geometric PIC approach is generalized to the case of electrons with spin. Total energy conservation is very well satisfied, with a relative error below $0.05\,\%$ . As a relevant example, we study the stimulated Raman scattering of an electromagnetic wave interacting with an underdense plasma, where the electrons are partially or fully spin polarized. It is shown that the Raman instability is very effective in destroying the electron polarization.


Author(s):  
Thomas Cunningham Wilson ◽  
Zheng-Ming Sheng ◽  
Bengt Erik Eliasson ◽  
Paul McKenna

2021 ◽  
Vol 23 (5) ◽  
pp. 055001
Author(s):  
Xiaobo ZHANG ◽  
Xin QIAO ◽  
Aixia ZHANG ◽  
Jukui XUE

2021 ◽  
Vol 28 (2) ◽  
pp. 023112
Author(s):  
K. V. Lezhnin ◽  
K. Qu ◽  
N. J. Fisch

2020 ◽  
Vol 3 (1) ◽  
Author(s):  
Chen-Kang Huang ◽  
Chaojie Zhang ◽  
Zan Nie ◽  
Kenneth A. Marsh ◽  
Chris E. Clayton ◽  
...  

AbstractSpin and orbital angular momentum of an optical beam are two independent parameters that exhibit distinct effects on mechanical objects. However, when laser beams with angular momentum interact with plasmas, one can observe the interplay between the spin and the orbital angular momentum. Here, by measuring the helical phase of the second harmonic 2ω radiation generated in an underdense plasma using a known spin and orbital angular momentum pump beam, we verify that the total angular momentum of photons is conserved and observe the conversion of spin to orbital angular momentum. We further determine the source of the 2ω photons by analyzing near field intensity distributions of the 2ω light. The 2ω images are consistent with these photons being generated near the largest intensity gradients of the pump beam in the plasma as predicted by the combined effect of spin and orbital angular momentum when Laguerre-Gaussian beams are used.


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