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The particle density in extensive air showers fluctuates at the ground level. These fluctuations, at the scale of the scintillator detector size (several meters), lead to the diversity of the individual detector responses. Therefore, small…

Astrophysics · Physics 2008-11-26 V. A. Kuzmin , G. I. Rubtsov

An intense 146 MeV/c pion beam was stopped inside a scintillating fiber detector made out of 12 planes with 16 pixels each, where every pixel consists out of 8 times 8 scintillating fibers of 500 mkm diameter dense packed. The detector was…

Instrumentation and Detectors · Physics 2009-10-31 J. Baehr , R. Nahnhauer , S. Nerreter , R. Shanidze

The DArk Matter Particle Explorer (DAMPE) is one of the four satellites within Strategic Pioneer Research Program in Space Science of the Chinese Academy of Science (CAS). DAMPE can detect electrons, photons and ions in a wide energy range…

Instrumentation and Methods for Astrophysics · Physics 2017-01-23 Rui Qiao , Wen-Xi Peng , Dong-Ya Guo , Hao Zhao , Huan-Yu Wang

High light collection efficiency is an important requirement in any application of scintillation detectors. The purpose of this study is to investigate the possibility for improving this parameter in cryogenic scintillation bolometers,…

Instrumentation and Detectors · Physics 2014-02-11 F. A. Danevich , R. V. Kobychev , V. V. Kobychev , H. Kraus , V. B. Mikhailik , V. M. Mokina

The DArk Matter Particle Explorer (DAMPE) is a satellite-borne detector for high-energy cosmic rays and $\gamma$-rays. To fully understand the detector performance and obtain reliable physical results, extensive simulations of the detector…

Plastic scintillator detectors have been extensively used in particle physics experiments for decades. A large-scale detector is typically arranged as an array of staggered long bars which provide a fast trigger signal and/or particle…

The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic rays with primary energies above 1.6 x 10^(18) eV. This measurement is based upon four years of observation by the surface detector…

High Energy Astrophysical Phenomena · Physics 2013-04-12 T. Abu-Zayyad , R. Aida , M. Allen , R. Anderson , R. Azuma , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , R. Cady , B. G. Cheon , J. Chiba , M. Chikawa , E. J. Cho , W. R. Cho , H. Fujii , T. Fujii , T. Fukuda , M. Fukushima , W. Hanlon , K. Hayashi , Y. Hayashi , N. Hayashida , K. Hibino , K. Hiyama , K. Honda , T. Iguchi , D. Ikeda , K. Ikuta , N. Inoue , T. Ishii , R. Ishimori , D. Ivanov , S. Iwamoto , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , T. Kanbe , K. Kasahara , H. Kawai , S. Kawakami , S. Kawana , E. Kido , H. B. Kim , H. K. Kim , J. H. Kim , J. H. Kim , K. Kitamoto , S. Kitamura , Y. Kitamura , K. Kobayashi , Y. Kobayashi , Y. Kondo , K. Kuramoto , V. Kuzmin , Y. J. Kwon , J. Lan , S. I. Lim , S. Machida , K. Martens , T. Matsuda , T. Matsuura , T. Matsuyama , J. N. Matthews , M. Minamino , K. Miyata , Y. Murano , I. Myers , K. Nagasawa , S. Nagataki , T. Nakamura , S. W. Nam , T. Nonaka , S. Ogio , M. Ohnishi , H. Ohoka , K. Oki , D. Oku , T. Okuda , A. Oshima , S. Ozawa , I. H. Park , M. S. Pshirkov , D. C. Rodriguez , S. Y. Roh , G. Rubtsov , D. Ryu , H. Sagawa , N. Sakurai , A. L. Sampson , L. M. Scott , P. D. Shah , F. Shibata , T. Shibata , H. Shimodaira , B. K. Shin , J. I. Shin , T. Shirahama , J. D. Smith , P. Sokolsky , B. T. Stokes , S. R. Stratton , T. A. Stroman , S. Suzuki , Y. Takahashi , M. Takeda , A. Taketa , M. Takita , Y. Tameda , H. Tanaka , K. Tanaka , M. Tanaka , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , Y. Tsunesada , K. Tsutsumi , Y. Tsuyuguchi , Y. Uchihori , S. Udo , H. Ukai , G. Vasiloff , Y. Wada , T. Wong , M. Wood , Y. Yamakawa , R. Yamane , H. Yamaoka , K. Yamazaki , J. Yang , Y. Yoneda , S. Yoshida , H. Yoshii , X. Zhou , R. Zollinger , Z. Zundel

The Strontium Iodide Radiation Instrument (SIRI) is a single detector, gamma-ray spectrometer designed to space-qualify the new scintillation detector material europium-doped strontium iodide (SrI2:Eu) and new silicon photomultiplier (SiPM)…

Instrumentation and Methods for Astrophysics · Physics 2019-07-29 Lee J. Mitchell , Bernard F. Phlips , J. Eric Grove , Theodore Finne , Mary Johnson-Rambert , W. Neil Johnson

We report progress on applying technologies developed for LHC-era experiments to cosmic ray detection, using scintillating tiles with embedded wavelength-shifting fibers and avalanche photodiode readouts as parts of a robust, inexpensive…

Polarization measurements in the X-ray and gamma-ray energy range can provide crucial information on massive compact objects such as black holes and neutron stars. The Polarized Gamma-ray Observer (PoGO) is a new balloon-borne instrument…

Observations of pulsar scintillation are among the few astrophysical probes of very small-scale ($\lesssim$ au) phenomena in the interstellar medium (ISM). In particular, characterization of scintillation arcs, including their curvature and…

High Energy Astrophysical Phenomena · Physics 2023-11-28 S. K. Ocker , J. M. Cordes , S. Chatterjee , D. R. Stinebring , T. Dolch , V. Pelgrims , J. W. McKee , C. Giannakopoulos , D. J. Reardon

The GERDA experiment searches for the neutrinoless double beta ($0\nu\beta\beta$) decay in $^{76}$Ge in order to probe whether the neutrino is a Majorana particle and to shed light on the neutrino mass ordering. For investigating such a…

Instrumentation and Detectors · Physics 2019-11-11 Nuno Barros , Alexander R. Domula , Björn Lehnert , Birgit Zatschler , Kai Zuber

Cosmic Ray Neutron Sensing (CRNS) is a powerful technique that allows non-invasive monitoring of soil moisture on length scales well matched for agricultural applications. One factor limiting the use of the technique within industrial…

Instrumentation and Detectors · Physics 2021-12-15 J. P. Stowell , S. J. Fargher , C. A. Steer , L. F. Thompson

We used the GEANT4 Monte Carlo MC Toolkit to simulate carbon ion beams incident on water, tissue, and bone, taking into account nuclear fragmentation reactions. Upon increasing the energy of the primary beam, the position of the Bragg-Peak…

Medical Physics · Physics 2021-02-26 M. Kh. Hamad

We report on our studies of applying novel detector technologies developed for LHC-era experiments to cosmic ray detection. In particular, we are investigating usage of scintillating tiles with embedded wavelength-shifting fibers and…

High Energy Physics - Experiment · Physics 2007-05-23 L. A. Anchordoqui , J. Cook , M. Gabour , N. Kirsch , J. MacLeod , T. P. McCauley , Y. Musienko , T. C. Paul , S. Reucroft , J. D. Swain , R. Terry

LHAASO is expected to be the most sensitive project to face the open problems in Galactic cosmic ray physics through a combined study of photon- and charged particle-induced extensive air showers in the energy range 10$^{11}$ - 10$^{17}$…

High Energy Astrophysical Phenomena · Physics 2019-08-13 G. Di Sciascio

The Gamma RAy Polarimeter Experiment (GRAPE), a balloon borne Compton polarimeter for 50-500 keV gamma rays, was successfully flown for the second time in 2014. GRAPE consists of 24 collimated polarimeter modules. Each module is made up of…

Instrumentation and Methods for Astrophysics · Physics 2020-12-25 Sambid K. Wasti

Future HEP experiments at the energy and intensity frontiers present stringent challenges to inorganic scintillators in radiation tolerance, ultrafast time response and cost. This paper reports recent progress in radiation hard, ultrafast,…

Instrumentation and Detectors · Physics 2022-03-15 Chen Hu , Liyuan Zhang , Ren-Yuan Zhu

We have investigated scintillation light distribution in BaF$_{2}$ and pure CsI crystals with dimensions 3x3x20 cm$^{3}$ using the Geant4 toolkit. The diffuse wrapping material is selected as coating for the crystals. The simulated cosmic…

Instrumentation and Detectors · Physics 2016-04-05 Zafar Usubov