2016
DOI: 10.1103/physreve.93.043201
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Plasma scale-length effects on electron energy spectra in high-irradiance laser plasmas

Abstract: An analysis of an electron spectrometer used to characterize fast electrons generated by ultraintense (10 20 W cm −2 ) laser interaction with a preformed plasma of scale length measured by shadowgraphy is presented. The effects of fringing magnetic fields on the electron spectral measurements and the accuracy of density scale-length measurements are evaluated. 2D EPOCH PIC code simulations are found to be in agreement with measurements of the electron energy spectra showing that laser filamentation in plasma p… Show more

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Cited by 24 publications
(12 citation statements)
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“…It is seen that measured maximum energies increase up to a certain point and start decreases again which is in agreement with previous studies undertaken by Ross et al [13]. We have explained measured hot electron spectra and showed the decrease on hot electron temperature which is relevant to the plasma scale length and laser filamentation in plasmas [17,22]. These laser filamentations are also effect generated proton energy and temperature which explains the decrease on proton energy and temperature after a certain scale length.…”
Section: Resultssupporting
confidence: 91%
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“…It is seen that measured maximum energies increase up to a certain point and start decreases again which is in agreement with previous studies undertaken by Ross et al [13]. We have explained measured hot electron spectra and showed the decrease on hot electron temperature which is relevant to the plasma scale length and laser filamentation in plasmas [17,22]. These laser filamentations are also effect generated proton energy and temperature which explains the decrease on proton energy and temperature after a certain scale length.…”
Section: Resultssupporting
confidence: 91%
“…The produced hot electron flux with the energies up to 200 MeV is accelerated through to the laser axis (40 • to the target normal and RCF stack) [22]. Protons are attenuated in the stack of RCF films as they penetrate through the different films, with the exposure of the films giving the energy of proton flux sufficient to transmit through the RCF films.…”
Section: Resultsmentioning
confidence: 99%
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“…The amplitude of the magnetic fields at the target rear depends on the scale-length of the rear-side plasma. Consequently, 1D radiation hydrodynamics simulations using the HYADES code 41 were performed to obtain the scale-length of the plasma density profile at the target rear, assuming that the target rear was volume-heated to a temperature consistent with that observed for similar targets in previous experiments under similar conditions 42 , 43 . These simulations were run for a CH target for the time-period (1-10) ps following the main interaction pulse and the expansion velocity of the critical surface was found to be fairly constant at 9 × 10 6 cm/s during the simulation period equivalent to a scale-length of <1 μ m at 10 ps at the target rear, consistent with shadowgraphy measurements).…”
Section: Methodsmentioning
confidence: 99%