2018
DOI: 10.1016/j.nima.2017.09.046
|View full text |Cite
|
Sign up to set email alerts
|

OSCAR: A new modular device for the identification and correlation of low energy particles

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
9
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
7

Relationship

3
4

Authors

Journals

citations
Cited by 34 publications
(9 citation statements)
references
References 54 publications
0
9
0
Order By: Relevance
“…One can also observe in Fig. 2 a region containing events related to the channeling process [24]. The total counts related to the sum of spurious coincidence and channeling events represents a quite small fraction of about 2% of the elastic scattering yield.…”
Section: Methodsmentioning
confidence: 82%
“…One can also observe in Fig. 2 a region containing events related to the channeling process [24]. The total counts related to the sum of spurious coincidence and channeling events represents a quite small fraction of about 2% of the elastic scattering yield.…”
Section: Methodsmentioning
confidence: 82%
“…Such detectors are typically designed to have an optimized response to the detection of lighter particles and to have a high degree of versatility compared to the previous generation of large-acceptance detection systems. The higher stopping power of charged particles in CsI crystals enables a significantly larger dynamic energy range than that achieved with Si-Si modular telescopes (such as OSCAR [15]). However, the energy calibrations are more complicated as the light response of the CsI crystals is not linear and depends on the charge and mass of the charged particles as well as the length of the detector.…”
Section: Introductionmentioning
confidence: 99%
“…This diversification is needed to better investigate phenomena typical of different energy regimes: compound nucleus formation and decay [62], α-clustering [63], charged particle spectroscopy [64], isospin transport mechanisms [65][66][67] and neck emissions [68]. Various setups have been developed and used at LNS, LNL and GANIL: FAZIA [69,70], GARFIELD [71], OSCAR [72] and the ACTAR demonstrator [73]. PID makes use of detectors based on combinations of sensors into telescopes (see Sect.…”
Section: Nuclex: Nuclear Dynamics and Thermodynamics With Heavy Ionsmentioning
confidence: 99%