Laser pulse amplification through exchange of energy with an electron beam via nonlinear radiation pressure effects

1980 ◽  
Vol 51 (7) ◽  
pp. 3501-3505 ◽  
Author(s):  
R. Mavaddat ◽  
A. K. Ghatak
1997 ◽  
Vol 22 (11) ◽  
pp. 811 ◽  
Author(s):  
O. E. Martínez ◽  
C. M. González Inchauspe

1997 ◽  
Vol 58 (4) ◽  
pp. 613-621 ◽  
Author(s):  
JETENDRA PARASHAR ◽  
H. D. PANDEY ◽  
A. K. SHARMA ◽  
V. K. TRIPATHI

An intense short laser pulse or a millimetre wave propagating through a plasma channel may act as a wiggler for the generation of shorter wavelengths. When a relativistic electron beam is launched into the channel from the opposite direction, the laser radiation is Compton/Raman backscattered to produce coherent radiation at shorter wavelengths. The scheme, however, requires a superior beam quality with energy spread less than 1% in the Raman regime.


Laser Physics ◽  
2006 ◽  
Vol 16 (7) ◽  
pp. 1107-1110 ◽  
Author(s):  
H. Kotaki ◽  
A. Yamazaki ◽  
I. Daito ◽  
M. Kando ◽  
S. V. Bulanov ◽  
...  

2008 ◽  
Author(s):  
A. Heidmann ◽  
O. Arcizet ◽  
C. Molinelli ◽  
T. Briant ◽  
P.-F. Cohadon

2019 ◽  
Vol 61 (12) ◽  
pp. 124004 ◽  
Author(s):  
V Yu Bychenkov ◽  
M G Lobok ◽  
V F Kovalev ◽  
A V Brantov

1989 ◽  
Vol 113 ◽  
pp. 195-204
Author(s):  
I. Appenzeller

AbstractAs LBVs have luminosities close to their Eddington limits, their structure is profoundly influenced by radiation pressure. Radiation pressure effects probably cause the highly extended atmospheres and the extreme mass loss observed during the maximum states of the S Dor variables. An opacity-related instability of the radiative acceleration combined with a delayed thermal readjustement of the sub-atmospheric layers possibly explains the large-amplitude radius variations of these objects.


2010 ◽  
Vol 36 (1) ◽  
pp. 15-29 ◽  
Author(s):  
E. Yu. Echkina ◽  
I. N. Inovenkov ◽  
T. Zh. Esirkepov ◽  
F. Pegoraro ◽  
M. Borghesi ◽  
...  

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