Cross-section measurements of the space-star configuration in N-D breakup at 13.0 MeV

1995 ◽  
Author(s):  
H. R. Setze ◽  
C. R. Howell ◽  
R. T. Braun ◽  
D. E. Gonzalez Trotter ◽  
A. H. Hussein ◽  
...  
2003 ◽  
Vol 18 (02n06) ◽  
pp. 436-439 ◽  
Author(s):  
T. ISHIDA ◽  
T. YAGITA ◽  
S. OCHI ◽  
S. NOZOE ◽  
K. TSURUTA ◽  
...  

Systematic measurement of D(p,pp)n cross section has been made at an incident energy of 13MeV around the space star configuration. In spite of the anomaly found in nd breakup cross section, no anomaly has been found in pd breakup.


2009 ◽  
Vol 24 (11n13) ◽  
pp. 863-866
Author(s):  
T. SUETA ◽  
S. KUROITA ◽  
H. SHIMODA ◽  
Y. EGUCHI ◽  
K. YASHIMA ◽  
...  

We measured D (p, pp)n cross section at Ep = 9.5 MeV and 13 MeV at off-plane star configurations, including the space star where the star is perpendicular to the beam axis. The experimental results were compared with recent pd breakup calculations using screened Coulomb force, and disagreement was found to smoothly vary with an inclination angle of the off-plane star, α. Further systematic experiments are necessary to investigate the star anomaly.


2021 ◽  
Vol 104 (1) ◽  
Author(s):  
H. Witała ◽  
J. Golak ◽  
R. Skibiński ◽  
K. Topolnicki ◽  
E. Epelbaum ◽  
...  

2001 ◽  
Vol 684 (1-4) ◽  
pp. 583-585 ◽  
Author(s):  
Y. Tachikawa ◽  
T. Yagita ◽  
M. Kondo ◽  
S. Minami ◽  
T. Ishida ◽  
...  

Author(s):  
Andrzej Wilczek ◽  
Albert Szadziński ◽  
Kazimierz Bodek ◽  
Izabela Ciepał ◽  
Mohammad Eslami-Kalantari ◽  
...  

The~Space Star Anomaly in proton-deuteron breakup cross-section occurs at energies of about 10~MeV. Data for higher energies are sparse. Therefore, a~systematic scan over star configurations in the~range of intermediate energies between 50 and 100 MeV/nucleon is carried out on the~basis of data collected with the~large acceptance BINA detector. The~preliminary cross section results for forward star configurations at 80 MeV/nucleon slightly surpass the~theoretical calculations, but the~systematic uncertainties are still under study. Also, a~new variable describing rotation of star configurations is proposed.


2014 ◽  
Vol 55 (8-10) ◽  
pp. 725-728 ◽  
Author(s):  
K. Ohnaka ◽  
K. Sagara ◽  
Y. Maeda ◽  
K. Ishibashi ◽  
S. Kimura ◽  
...  

Author(s):  
T. ISHIDA ◽  
T. YAGITA ◽  
S. OCHI ◽  
S. NOZOE ◽  
K. TSURUTA ◽  
...  

1988 ◽  
Vol 102 ◽  
pp. 71-73
Author(s):  
E. Jannitti ◽  
P. Nicolosi ◽  
G. Tondello

AbstractThe photoabsorption spectra of the carbon ions have been obtained by using two laser-produced plasmas. The photoionization cross-section of the CV has been absolutely measured and the value at threshold, σ=(4.7±0.5) × 10−19cm2, as well as its behaviour at higher energies agrees quite well with the theoretical calculations.


Author(s):  
J. Langmore ◽  
M. Isaacson ◽  
J. Wall ◽  
A. V. Crewe

High resolution dark field microscopy is becoming an important tool for the investigation of unstained and specifically stained biological molecules. Of primary consideration to the microscopist is the interpretation of image Intensities and the effects of radiation damage to the specimen. Ignoring inelastic scattering, the image intensity is directly related to the collected elastic scattering cross section, σɳ, which is the product of the total elastic cross section, σ and the eficiency of the microscope system at imaging these electrons, η. The number of potentially bond damaging events resulting from the beam exposure required to reduce the effect of quantum noise in the image to a given level is proportional to 1/η. We wish to compare η in three dark field systems.


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