Backward Compton scattering of laser light against high-energy electrons: the LADON photon beam at Frascati

1980 ◽  
Vol 59 (2) ◽  
pp. 247-256 ◽  
Author(s):  
L. Federici ◽  
G. Giordano ◽  
G. Matone ◽  
G. Pasquariello ◽  
P. G. Picozza ◽  
...  
2018 ◽  
Vol 8 (9) ◽  
pp. 1565 ◽  
Author(s):  
Tadzio Levato ◽  
Stefano Bonora ◽  
Gabriele Grittani ◽  
Carlo Lazzarini ◽  
Muhammad Nawaz ◽  
...  

Laser wake field acceleration (LWFA) is an efficient method to accelerate electron beams to high energy. This is a benefit in research infrastructures where a multidisciplinary environment can benefit from the different secondary sources enabled, having the opportunity to extend the range of applications that is accessible and to develop new ideas for fundamental studies. The ELI Beamline project is oriented to deliver such beams to the scientific community both for applied and fundamental research. The driver laser is a Ti:Sa diode-pumped system , running at a maximum performance of 10 Hz, 30 J, and 30 fs. The possibilities to setup experiments using different focal lengths parabolas, as well as the possibility to counter-propagate a second laser beam intrinsically synchronized, are considered in the electron acceleration program. Here, we review the laser-driven electron acceleration experimental platform under implementation at ELI Beamlines, the HELL (High-energy Electrons by Laser Light) experimental platform .


1973 ◽  
Vol 7 (5) ◽  
pp. 1568-1572 ◽  
Author(s):  
H. F. Wellenstein ◽  
R. A. Bonham

1970 ◽  
Vol 37 ◽  
pp. 247-249
Author(s):  
Krishna M. V. Apparao

The electromagnetic spectrum of the Crab Nebula has been determined experimentally in the radio, optical, and X-ray regions [1], in which it follows a power law of the type S(v) = Av−α, where S(v) is the power (in watts/m2 sec Hz), A and α are constants, and v is the frequency in Hz. Recent measurements [2–5], however, show a deviation from a power law in the microwave region (see Figure 1). In this paper, we investigate the origin of this deviation and calculate the γ-Ray spectrum due to this increase in the microwave photons via the Compton scattering from high-energy electrons.


2010 ◽  
Vol 104 (24) ◽  
Author(s):  
J.-P. Bocquet ◽  
D. Moricciani ◽  
V. Bellini ◽  
M. Beretta ◽  
L. Casano ◽  
...  

2005 ◽  
Vol 20 (02n03) ◽  
pp. 503-513 ◽  
Author(s):  
◽  
D. MORICCIANI ◽  
O. BARTALINI ◽  
V. BELLINI ◽  
J. P. BOCQUET ◽  
...  

A polarised and tagged [Formula: see text] ray beam is produced at GRAAL by the Compton scattering of laser light on the high energy electron of the ESRF storage ring. We present results on the beam polarisation asymmetries and cross sections in the photoproduction of mesons on hydrogen and deuterium target in the energy region 500-1500 MeV. These very precise results cover the angular range 30°-150°, providing stringent constraints to theoretical models.


2004 ◽  
Vol 19 (30) ◽  
pp. 5097-5186 ◽  
Author(s):  
B. BADELEK ◽  
C. BLÖCHINGER ◽  
J. BLÜMLEIN ◽  
E. BOOS ◽  
R. BRINKMANN ◽  
...  

High energy photon colliders (γγ,γe) are based on e-e-linear colliders where high energy photons are produced using Compton scattering of laser light on high energy electrons just before the interaction point. This paper is a part of the Technical Design Report of the linear collider TESLA.1Physics program, possible parameters and some technical aspects of the photon collider at TESLA are discussed.


Author(s):  
D. REBREYEND ◽  
J.-P. Bocquet ◽  
D. Moricciani ◽  
V. Bellini ◽  
M. Beretta ◽  
...  

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