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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01s1784p968
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dc.contributor.advisorFisch, Nathaniel J
dc.contributor.authorLezhnin, Kirill
dc.contributor.otherAstrophysical Sciences—Plasma Physics Program Department
dc.date.accessioned2022-12-02T20:55:29Z-
dc.date.available2022-12-02T20:55:29Z-
dc.date.created2022-01-01
dc.date.issued2022
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01s1784p968-
dc.description.abstractOver the past few decades, laser technology has developed dramatically, achieving ultrahigh peak laser powers. Currently operating laser facilities (e.g., NIF, OMEGAEP, and BELLA) may deliver up to 1 petawatt peak laser power, while up andcoming ELI-Beamlines and ELI-Nuclear Physics projects will reach 10 petawatt level soon. Such high power pulses are capable of creating ultrahigh electric (up to 1 gigavolt/micron) and magnetic (up to 1 megatesla) fields, which open up an opportunity for a wide range of applications, from fundamental investigations of strong-field QED and astrophysically relevant phenomena in the controlled laboratory environment to development of secondary sources of charged particles and radiation. In the present thesis, I will discuss laser power transmission and seed focusability problems in plasma-based laser amplification, some approaches towards the creation of laser-based fast ion and gamma ray sources, and applications of high power lasers to the studies of magnetic reconnection and electron acceleration by magnetized collisionless shocks.
dc.format.mimetypeapplication/pdf
dc.language.isoen
dc.publisherPrinceton, NJ : Princeton University
dc.subject.classificationAstrophysics
dc.subject.classificationPlasma physics
dc.titleUsing high power lasers as a tool for secondary sources and laboratory astrophysics
dc.typeAcademic dissertations (Ph.D.)
pu.date.classyear2022
pu.departmentAstrophysical Sciences—Plasma Physics Program
Appears in Collections:Plasma Physics

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