scholarly journals Compton scattering fromC12using tagged photons in the energy range 65–115 MeV

2014 ◽  
Vol 89 (3) ◽  
Author(s):  
L. S. Myers ◽  
K. Shoniyozov ◽  
M. F. Preston ◽  
M. D. Anderson ◽  
J. R. M. Annand ◽  
...  
Keyword(s):  
Energy Range ◽  
Compton Scattering ◽  
Tagged Photons

scholarly journals CROSS SECTION ASYMMETRY OF THE 12C(γ,p0)11B AND 12C(γ,p1)11B REACTIONS AT PHOTON ENERGIES 40...55MeV

2019 ◽  
pp. 26-37
Author(s):  
D.D. Burdeinyi ◽  
J. Brudvik ◽  
V.B. Ganenko ◽  
K. Hansen ◽  
K. Fissum ◽  
...  
Keyword(s):  
Reaction Mechanism ◽  
Energy Range ◽  
Cross Section ◽  
Relative Contribution ◽  
Linearly Polarized ◽  
The Asymmetry ◽  
The Cross ◽  
Tagged Photons

The asymmetry of the cross section of the 12C(γ,p0)11B and 12C(γ,p1)11B reactions has been measured in the energy range 40...55MeV using linearly polarized tagged photons of the MAX-lab facility. The asymmetry of the process 12C(⃗γ,p0)11B is Σ ≈ 0.85, that implies one-particle reaction mechanism. The asymmetry of the reaction 12C(⃗γ,p1)11B is smaller, Σ ≈ 0.6...0.7, that may be due to the stronger relative contribution of the 2h−1p mechanism to the dominant one-particle reaction mechanism.

Rayleigh and Compton scattering analysis for PMMA in the mammography energy range

2009 ◽  
pp. 234-237 ◽  
Author(s):  
Yoshiki Yamaguchi ◽  
Souichiro Kawaguchi ◽  
Hidetaka Arimura ◽  
Junji Morishita ◽  
Masafumi Ohki ◽  
...  
Keyword(s):  
Energy Range ◽  
Compton Scattering

Experimental study of the photoemission of protons off12C using tagged photons in the energy range 200?385 MeV

1980 ◽  
Vol 298 (2) ◽  
pp. 103-111 ◽  
Author(s):  
J. Arends ◽  
J. Eyink ◽  
H. Hartmann ◽  
A. Hegerath ◽  
B. Mecking ◽  
...  
Keyword(s):  
Experimental Study ◽  
Energy Range ◽  
Tagged Photons

Fissilities of 238U and 237Np nuclei measured with tagged photons in the energy range 60–240 MeV

1992 ◽  
Vol 539 (2) ◽  
pp. 263-275 ◽  
Author(s):  
A.S. Iljinov ◽  
D.I. Ivanov ◽  
M.V. Mebel ◽  
V.G. Nedorezov ◽  
A.S. Sudov ◽  
...  
Keyword(s):  
Energy Range ◽  
Tagged Photons

PRELIMINARY RESULTS ON η′ PHOTOPRODUCTION AT GRAAL

2010 ◽  
Vol 19 (05n06) ◽  
pp. 1177-1182
Author(s):  
M. MANGANARO ◽  
V. BELLINI ◽  
J. P. BOCQUET ◽  
L. CASANO ◽  
A. D'ANGELO ◽  
...  
Keyword(s):  
Energy Range ◽  
Beam Asymmetry ◽  
Preliminary Results ◽  
Tagged Photons

The γp → η′p reaction was studied near the threshold, in the 1.44 GeV > Eγ < 1.55 GeV energy range with the tagged photons of the former GRAAL experiment. The two neutral decays γγ(Γi/Γ = 2.10 ± 0.12%) and π0π0η(Γi/Γ = 20.7 ± 1.2%) were analized and preliminary results of the beam asymmetry were extracted together with the invariant masses.

Differential cross sections of proton Compton scattering in the energy range between 450 and 950 MeV

1978 ◽  
Vol 141 (4) ◽  
pp. 364-378 ◽  
Author(s):  
K. Toshioka ◽  
M. Chiba ◽  
S. Kato ◽  
K. Sugano ◽  
K. Ukai ◽  
...  
Keyword(s):  
Energy Range ◽  
Compton Scattering ◽  
Cross Sections ◽  
Differential Cross ◽  
Differential Cross Sections

scholarly journals Compton scattering for spectroscopic detection of ultra-fast, high flux, broad energy range X-rays

2013 ◽  
Vol 84 (11) ◽  
pp. 113302 ◽  
Author(s):  
S. Cipiccia ◽  
S. M. Wiggins ◽  
D. Maneuski ◽  
E. Brunetti ◽  
G. Vieux ◽  
...  
Keyword(s):  
Energy Range ◽  
Compton Scattering ◽  
High Flux ◽  
X Rays ◽  
Broad Energy Range ◽  
Broad Energy

scholarly journals X-RAY TRANSMISSION AND REFLECTION THROUGH A COMPTON-THICK MEDIUM VIA MONTE-CARLO SIMULATIONS

2014 ◽  
Vol 54 (3) ◽  
pp. 177-182 ◽  
Author(s):  
Wiebke Eikmann ◽  
Jörn Wilms ◽  
Randall K. Smith ◽  
Julia C. Lee
Keyword(s):  
Monte Carlo ◽  
Energy Range ◽  
Compton Scattering ◽  
Primary Source ◽  
High Energy ◽  
X Ray ◽  
Absorption Models ◽  
High Column ◽  
Transmission And Reflection ◽  
Thick Medium

The spectral shape of an X-ray source strongly depends on the amount and distribution of the surrounding material. The spectrum of a primary source which is located in an optically thin medium with respect to Compton scattering is mainly modified by photo absorption in the lower energy range and is almost unaltered above ~ 10 keV. This picture changes when the source is obscured by gas exceeding hydrogen column densities of ~ 10<sup>24</sup> cm<sup>−2</sup>. At this degree of absorption it is likely that photons are scattered at least twice before leaving the medium. The multiple scatterings lead to a lack of photons in the high energy range of the resulting spectrum as well as to an accumulation of photons at moderate energies forming the so-called Compton-bump. The shape of the fluorescent lines also changes since scattered line photons form several Compton-shoulders which are very prominent especially for Compton-thick sources. Using a Monte Carlo method, we demonstrate the importance of Compton scattering for high column densities. For that purpose, we compare our results with existing absorption models that do not consider Compton scattering. These calculations will be implemented in a prospective version of the <em>tbabs</em> absorption model including an analytic evaluation of the strength of the fluorescent lines.

Experimental study of Compton scattering on protons by polarized photons in the energy range Egamma=0.5-1.0 GeV

1993 ◽  
Vol 19 (9) ◽  
pp. L139-L142 ◽  
Author(s):  
F V Adamian ◽  
A Yu Buniatian ◽  
G S Frangulian ◽  
P I Galumian ◽  
V H Grabsky ◽  
...  
Keyword(s):  
Experimental Study ◽  
Energy Range ◽  
Compton Scattering ◽  
Polarized Photons
Sign in / Sign up

Export Citation Format

Share Document