Observation of Monoenergetic Relativistic Electron Beams from Intense Laser - Plasma Interactions

Author(s):  
S.P.D. Mangles ◽  
C.D. Murphy ◽  
Z. Najmudin ◽  
A.G.R. Thomas ◽  
B.R. Walton ◽  
...  
2003 ◽  
Vol 10 (9) ◽  
pp. 3712-3716 ◽  
Author(s):  
H. Habara ◽  
R. Kodama ◽  
Y. Sentoku ◽  
N. Izumi ◽  
Y. Kitagawa ◽  
...  

2017 ◽  
Vol 19 (6) ◽  
pp. 063014 ◽  
Author(s):  
F Dollar ◽  
C Zulick ◽  
A Raymond ◽  
V Chvykov ◽  
L Willingale ◽  
...  

2007 ◽  
Vol 9 (11) ◽  
pp. 402-402 ◽  
Author(s):  
S Kar ◽  
M Borghesi ◽  
C A Cecchetti ◽  
L Romagnani ◽  
F Ceccherini ◽  
...  

Atoms ◽  
2018 ◽  
Vol 6 (3) ◽  
pp. 45 ◽  
Author(s):  
Elisabeth Dalimier ◽  
Tatiana A. Pikuz ◽  
Paulo Angelo

Intra-Stark spectroscopy (ISS) is the spectroscopy within the quasi-static Stark profile of a spectral line. The present paper reviews the X-ray ISS-based studies recently advanced for the diagnostics of the relativistic laser–plasma interactions. By improving experiments performed on the Vulcan Petawatt (PW) laser facility at the Rutherford Appleton Laboratory (RAL), the simultaneous production of the Langmuir waves and of the ion acoustic turbulence at the surface of the relativistic critical density gave the first probe by ISS of the parametric decay instability (PDI) predicted by PIC simulations. The reliable reproducibility of the experimental signatures of PDI—i.e., the Langmuir-wave-induced dips—allowed measurements of the fields of the Langmuir and ion acoustic waves. The parallel theoretical study based on a rigorous condition of the dynamic resonance depending on the relative values of the ion acoustic and the Langmuir fields could explain the disappearance of the Langmuir dips as the Langmuir wave field increases. The ISS used for the diagnostic of the PDI process in relativistic laser–plasma interactions has reinforced the reliability of the spectral line shape while allowing for all broadening mechanisms. The results can be used for a better understanding of intense laser–plasma interactions and for laboratory modelling of physical processes in astrophysical objects.


2015 ◽  
Vol 81 (6) ◽  
Author(s):  
Antonio Giulietti ◽  
Danilo Giulietti

Creation of plasmas by intense laser pulses and consequent laser–plasma interactions involve highly non-linear processes. In particular, a variation of the refractive index induced by the laser action turns into a self-phase modulation (SPM) of the laser field. This effect, already observed with nanosecond laser pulses, achieves striking evidence with ultra-short pulses whose intensity can produce index changes in a time as short as a single optical cycle. In this condition, spectral modifications of the laser pulse produced by SPM may strongly modify the laser–plasma interaction. At the same time, the spectral analysis of the transmitted and scattered laser radiation gives valuable information on a variety of processes occurring in the plasma. In this paper we simply consider a few results, which can be attributed to SPM, with the aim of comparing nanosecond and sub-picosecond laser interaction regimes at moderate laser intensities.


2012 ◽  
Vol 21 (12) ◽  
pp. 1250102 ◽  
Author(s):  
SACHIE KIMURA ◽  
ALDO BONASERA

We discuss scaling laws of fusion yields generated by laser-plasma interactions. The yields are found to scale as a function of the laser power. The origin of the scaling law in the laser driven fusion yield is derived in terms of hydrodynamic scaling. We point out that the scaling properties can be attributed to the laser power dependence of three terms: the reaction rate, the density of the plasma and the projected range of the plasma particle in the target medium. The resulting scaling relations have a predictive power that enables estimating the fusion yield for a nuclear reaction which has not been investigated by means of the laser accelerated ion beams.


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