Dynamics of Self-Generated, Large Amplitude Magnetic Fields Following High-Intensity Laser Matter Interaction


Autoria(s): Sarri, G.; Macchi, A.; Cecchetti, C. A.; Kar, S.; Liseykina, T. V.; Yang, X. H.; Dieckmann, M. E.; Fuchs, J.; Galimberti, M.; Gizzi, L. A.; Jung, R.; Kourakis, I.; Osterholz, J.; Pegoraro, F.; Robinson, A. P. L.; Romagnani, L.; Willi, O.; Borghesi, M.
Data(s)

16/11/2012

Resumo

The dynamics of magnetic fields with an amplitude of several tens of megagauss, generated at both sides of a solid target irradiated with a high-intensity (~1019W/cm2) picosecond laser pulse, has been spatially and temporally resolved using a proton imaging technique. The amplitude of the magnetic fields is sufficiently large to have a constraining effect on the radial expansion of the plasma sheath at the target surfaces. These results, supported by numerical simulations and simple analytical modeling, may have implications for ion acceleration driven by the plasma sheath at the rear side of the target as well as for the laboratory study of self-collimated high-energy plasma jets. © 2012 American Physical Society.

Formato

application/pdf

Identificador

http://pure.qub.ac.uk/portal/en/publications/dynamics-of-selfgenerated-large-amplitude-magnetic-fields-following-highintensity-laser-matter-interaction(847e93c0-5ebc-4478-ad9a-bceb2bd5e5e7).html

http://dx.doi.org/10.1103/PhysRevLett.109.205002

http://pure.qub.ac.uk/ws/files/2725992/PhysRevLett.109.205002.pdf

http://www.scopus.com/inward/record.url?partnerID=yv4JPVwI&eid=2-s2.0-84869066878&md5=512272777ceeee97f6203162ea9e291e

Idioma(s)

eng

Direitos

info:eu-repo/semantics/openAccess

Fonte

Sarri , G , Macchi , A , Cecchetti , C A , Kar , S , Liseykina , T V , Yang , X H , Dieckmann , M E , Fuchs , J , Galimberti , M , Gizzi , L A , Jung , R , Kourakis , I , Osterholz , J , Pegoraro , F , Robinson , A P L , Romagnani , L , Willi , O & Borghesi , M 2012 , ' Dynamics of Self-Generated, Large Amplitude Magnetic Fields Following High-Intensity Laser Matter Interaction ' Physical Review Letters , vol 109 , no. 20 , 205002 , pp. 1-5 . DOI: 10.1103/PhysRevLett.109.205002

Tipo

article