scholarly journals Development of scintillation detectors with SiPM readout for the NICA project

2020 ◽  
Vol 50 ◽  
pp. 2060008
Author(s):  
V. I. Yurevich ◽  
S. A. Sedykh ◽  
S. V. Sergeev ◽  
D. N. Bogoslovski ◽  
V. Yu. Rogov ◽  
...  

Scintillation detectors with SiPM readout are developed for trigger systems and neutron time-of-flight measurements in the framework of the NICA project at JINR. Some detectors are operated in a strong magnetic field of the BM@N and MPD setups. New projects of detectors with picosecond time resolution for trigger of nucleus–nucleus collisions in collider experiment and neutron time-of-flight measurements are discussed.

2001 ◽  
Vol 72 (1) ◽  
pp. 859-862
Author(s):  
D. G. Hicks ◽  
C. K. Li ◽  
F. H. Séguin ◽  
J. A. Frenje ◽  
R. D. Petrasso ◽  
...  

2020 ◽  
Vol 239 ◽  
pp. 17007
Author(s):  
F. Gunsing ◽  
F. Belloni ◽  
E. Berthoumieux ◽  
M. Diakaki ◽  
E. Dupont ◽  
...  

MicroMegas detectors are versatile gaseous detectors which are used for ionizing particle detection. A MicroMegas detector consists of two adjacent gas-filled volumes. One volume acts as a drift region with an electric field operating in the ionization chamber regime, the second volume is the amplification region acting as a parallel-plate avalanche counter. The use of the microbulk technique allows the production of thin, radiation resistant, and low-mass detector with a highly variable gain. Such MicroMegas detectors have been developed and used in combination with neutron time-of-flight measurements for in-beam neutron-flux monitoring, fission and light-charged particle reaction cross section measurements, and for neutron-beam imaging. An overview of MicroMegas detectors for neutron detection and neutron reaction cross section measurements and related results and developments will be presented.


2019 ◽  
Vol 90 (7) ◽  
pp. 073505 ◽  
Author(s):  
E. Ruskov ◽  
V. Yu. Glebov ◽  
T. W. Darling ◽  
F. J. Wessel ◽  
F. Conti ◽  
...  

1997 ◽  
Vol 163 ◽  
pp. 391-395
Author(s):  
Jeremy Bailey

AbstractAM Herculis Binaries (or Polars) are a subclass of the Cataclysmic Variables in which the accreting white dwarf has a strong magnetic field giving rise to highly polarized cyclotron radiation from the shock heated accretion region. A number of AM Herculis binaries are now known in which the white dwarf is eclipsed by the companion star. High time resolution observations of these eclipses allow a particularly detailed study of the process of accretion onto the magnetic white dwarf. Results on a number of systems will be presented and used to derive information on the accretion structure as well as on the fundamental properties of the binaries.


2010 ◽  
Vol 81 (10) ◽  
pp. 10D319 ◽  
Author(s):  
R. A. Lerche ◽  
V. Yu. Glebov ◽  
M. J. Moran ◽  
J. M. McNaney ◽  
J. D. Kilkenny ◽  
...  

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