2015
DOI: 10.1016/j.hedp.2014.11.005
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Relativistic plasma astrophysics with intense lasers

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Cited by 16 publications
(7 citation statements)
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“…The 3D reconnection rate can be observed using multi-channel CTS measurements or electric/magnetic field measurements at the reconnection region with proton radiography 4,5,8 . Moreover, the experiment can be extended to relativistic regime using ultraintense laser pulses 42,43 and turbulent regime using multiple beams 44,45 . Laboratory experiments will contribute further understanding the magnetic reconnections.…”
mentioning
confidence: 99%
“…The 3D reconnection rate can be observed using multi-channel CTS measurements or electric/magnetic field measurements at the reconnection region with proton radiography 4,5,8 . Moreover, the experiment can be extended to relativistic regime using ultraintense laser pulses 42,43 and turbulent regime using multiple beams 44,45 . Laboratory experiments will contribute further understanding the magnetic reconnections.…”
mentioning
confidence: 99%
“…This can be a turbulent magnetic field. Recent PIC simulations in electron scale show magnetic field generation from the null field due to KHI (Alves et al 2012).If the KHI driven magnetic field can survive in ion scale, it is interesting to investigate this as an origin of magnetic field in the universe (Kuramitsu et al 2015).…”
Section: Discussion and Summarymentioning
confidence: 99%
“…We have developed large-area suspended graphene (LSG) for proton radiography intended to use laboratory astrophysics experiments with a relatively small laser facility, where no plasma mirror is equipped 14 , 15 . In such small laser facilities, the radiations from the laser matter interactions by shooting m thick solid targets would be a serious problem.…”
Section: Introductionmentioning
confidence: 99%