Dynamics of dark hollow Gaussian laser pulses in relativistic plasma


Autoria(s): Sharma, A.; Misra, S.; Mishra, S.K.; Kourakis, I.
Data(s)

25/06/2013

Resumo

Optical beams with null central intensity have potential applications in the field of atom optics. The spatial and temporal evolution of a central shadow dark hollow Gaussian (DHG) relativistic laser pulse propagating in a plasma is studied in this article for first principles. A nonlinear Schrodinger-type equation is obtained for the beam spot profile and then solved numerically to investigate the pulse propagation characteristics. As series of numerical simulations are employed to trace the profile of the focused and compressed DHG laser pulse as it propagates through the plasma. The theoretical and simulation results predict that higher-order DHG pulses show smaller divergence as they propagate and, thus, lead to enhanced energy transport. © 2013 American Physical Society.

Identificador

http://pure.qub.ac.uk/portal/en/publications/dynamics-of-dark-hollow-gaussian-laser-pulses-in-relativistic-plasma(7b484bef-7acc-4ac7-8623-585c4d636d97).html

http://dx.doi.org/10.1103/PhysRevE.87.063111

http://www.scopus.com/inward/record.url?eid=2-s2.0-84879832588&partnerID=8YFLogxK

Idioma(s)

eng

Direitos

info:eu-repo/semantics/restrictedAccess

Fonte

Sharma , A , Misra , S , Mishra , S K & Kourakis , I 2013 , ' Dynamics of dark hollow Gaussian laser pulses in relativistic plasma ' Physical Review E , vol 87 , no. 6 . DOI: 10.1103/PhysRevE.87.063111

Tipo

article