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A publicação pode ser exportada nos seguintes formatos: referência da APA (American Psychological Association), referência do IEEE (Institute of Electrical and Electronics Engineers), BibTeX e RIS.

Exportar Referência (APA) 
Shulka, N, Schoeffler, K. M., Vieira, J., Fonseca, R. A., Boella, E & Silva, L. O. (2022). Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects. Physical Review E. 105 (3)
Exportar Referência (IEEE) 
N. Shukla et al.,  "Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects", in Physical Review E, vol. 105, no. 3, 2022
Exportar BibTeX 
@article{shukla2022_1784476682363,
	author = "Shulka, N and Schoeffler, K. M. and Vieira, J. and Fonseca, R. A. and Boella, E and Silva, L. O.",
	title = "Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects",
	journal = "Physical Review E",
	year = "2022",
	volume = "105",
	number = "3",
	doi = "10.1103/PhysRevE.105.035204",
	url = "https://journals.aps.org/pre/"
}
Exportar RIS 
TY  - JOUR
TI  - Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects
T2  - Physical Review E
VL  - 105
IS  - 3
AU  - Shulka, N
AU  - Schoeffler, K. M.
AU  - Vieira, J.
AU  - Fonseca, R. A.
AU  - Boella, E
AU  - Silva, L. O.
PY  - 2022
SN  - 1539-3755
DO  - 10.1103/PhysRevE.105.035204
UR  - https://journals.aps.org/pre/
AB  - The nonlinear evolution of electromagnetic instabilities driven by the interpenetration of two e-,e+ plasma clouds is explored using ab initio kinetic plasma simulations. We show that the plasma clouds slow down due to both oblique and Weibel generated electromagnetic fields, which deflect the particle trajectories, transferring bulk forward momentum into transverse momentum and thermal velocity spread. This process causes the flow velocity vinst to decrease approximately by a factor of 1/3 in a time interval ?t?B?p∼c/(vfl?B), where ?B is the magnetic equipartition parameter determined by the nonlinear saturation of the instabilities, vfl is the initial flow speed, and ?p is the plasma frequency. For the ?B measured in our simulations, ?t?B is close to 10 times the instability growth time. We show that as long as the plasma slab length L>vfl?t?B, the plasma flow is expected to slow down by a factor close to 1/3. 
ER  -