Cusp type electrostatic analyzer for measurements of medium energy charged particles

2006 ◽  
Vol 77 (12) ◽  
pp. 123303 ◽  
Author(s):  
S. Kasahara ◽  
K. Asamura ◽  
Y. Saito ◽  
T. Takashima ◽  
M. Hirahara ◽  
...  
Author(s):  
Paula Rangel Pestana Allegro ◽  
Márcia de Almeida Rizzutto ◽  
Nemitala Added ◽  
Vitor Ângelo Paulino de Aguiar ◽  
Dennis Lozano Toufen ◽  
...  

This study presents an alternative method to determine isotope ratios using a medium energy accelerator and simultaneously measuring the charged particles and gamma-rays produced in a nuclear reaction.


2020 ◽  
Vol 91 (1) ◽  
pp. 013303
Author(s):  
C. A. Maldonado ◽  
Z. Eyler ◽  
B. Pierce ◽  
L. Matson ◽  
P. Neal ◽  
...  

Proceedings ◽  
2019 ◽  
Vol 10 (1) ◽  
pp. 43
Author(s):  
Samrangy Sadhu

The azimuthal correlations between heavy-flavour hadrons or heavy-flavour decay electrons with charged particles in Pb-Pb collisions give insight on the modification of charm-jet properties in nucleus-nucleus collisions and the mechanisms through which heavy quarks in-medium energy-loss takes place. Studies in pp collisions, besides constituting the necessary baseline for nucleus-nucleus measurements, are important for testing expectations from pQCD-inspired Monte Carlo generators. In ALICE heavy-flavour hadrons are studied via their fully reconstructed hadronic decays (D mesons and Λ c baryon), via semileptonic decays of charmed baryons ( Λ c , Ξ c ) and via leptons coming from heavy-flavour hadron decays. In particular in the central barrel, η < | 0 . 8 | , the electrons from heavy-flavour hadron decays are investigated. This proceeding will include the study of azimuthal correlations of D mesons with charged particles in pp collisions and heavy-flavour decay electrons with charged particles in pp and Pb-Pb collisions at different energies available at the LHC. The Experimental results will also be compared with the expectations from POWHEG and PYTHIA event generators.


Author(s):  
Ian J.D. MacGregor ◽  
Stephen N. Dancer ◽  
John R.M. Annand ◽  
Peter A. Wallace ◽  
James D. Kellie ◽  
...  

1972 ◽  
Vol 15 (12) ◽  
pp. 1797-1800
Author(s):  
K. S. Golovanivskii ◽  
A. D. Guseinova ◽  
V. D. Dugar-Zhabon ◽  
A. I. Lushchik

1984 ◽  
Vol 75 ◽  
pp. 203-209
Author(s):  
Joseph A. Burns

ABSTRACTLying in Jupiter's equatorial plane is a diaphanous ring having little substructure within its three components (main band, faint disk, and halo). Micron-sized grains account for much of the visible ring, but particles of centimeter sizes and larger must also be present to absorb charged particles. Since dynamical evolution times and survival life times are quite short (≲102-3yr) for small grains, the Jovian ring is being continually replenished; probably most of the visible ring is generated by micrometeoroids colliding into unseen parent bodies that reside in the main band.


Author(s):  
Kin Lam

The energy of moving ions in solid is dependent on the electronic density as well as the atomic structural properties of the target material. These factors contribute to the observable effects in polycrystalline material using the scanning ion microscope. Here we outline a method to investigate the dependence of low velocity proton stopping on interatomic distances and orientations.The interaction of charged particles with atoms in the frame work of the Fermi gas model was proposed by Lindhard. For a system of atoms, the electronic Lindhard stopping power can be generalized to the formwhere the stopping power function is defined as


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