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Using 12C beams of 200 AMeV kinetic energy the production of secondary fragments from nuclear reactions in a thick water absorber (12.78 cm) was investigated. Fast neutrons and energetic charged particles (p-, d-, t-, a-particles) emitted in the forward hemisphere were identified by a BaF2/plastic-scintillation detector telescope. Neutron energy spectra were recorded at various angles using time-of-flight techniques. The neutron emission is forward peaked and the energy spectrum shows a broad maximum about half the energy per nucleon of the primary 12C ions. The total yield of fast neutrons emitted into the forward hemisphere integrated over the energy range of 25 to 500 MeV was found to be 0.43 +/- 0.1 per primary ion. The dose contribution of fast neutrons in patient treatments with carbon ions is estimated to be less than 1% of the total treatment dose.
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http://dx.doi.org/10.1016/s0167-8140(04)80023-9 | DOI Listing |
Space Sci Rev
September 2025
Johns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
A Gamma-Ray and Neutron Spectrometer (GRNS) instrument has been developed as part of the science payload for NASA's Discovery Program Psyche mission to the M-class asteroid (16) Psyche. The GRNS instrument is designed to measure the elemental composition of Psyche with the goal to understand the origin of this mysterious, potentially metal-rich planetary body. The GRNS will measure the near-surface abundances for the elements Ni, Fe, Si, K, S, Al, and Ca, as well as the spatial distribution of Psyche's metal-to-silicate fraction (or metal fraction).
View Article and Find Full Text PDFLife Sci Space Res (Amst)
August 2025
Juntendo University, Tokyo 113-0034, Japan.
In deep space environments such as the Moon and Mars, secondary radiation generated by interactions between galactic cosmic rays and spacecraft walls or planetary surfaces presents a significant challenge. In particular, the effects of neutron radiation remain insufficiently understood. This study investigates the impact of neutron radiation on pharmaceuticals, specifically the general anesthetic propofol (2,6-Diisopropylphenol).
View Article and Find Full Text PDFSensors (Basel)
July 2025
Dipartimento di Ingegneria Industriale, Università degli Studi di Trento, 38123 Trento, Italy.
In recent years, 3D pixel sensors have been a topic of increasing interest within the High Energy Physics community. Due to their inherent radiation hardness, demonstrated up to a fluence of 3×1016 1 MeV equivalent neutrons per square centimeter, 3D pixel sensors have been used to equip the innermost tracking layers of the ATLAS and CMS detector upgrades at the High-Luminosity Large Hadron Collider. Additionally, the next generation of vertex detectors calls for precise measurement of charged particle timing at the pixel level.
View Article and Find Full Text PDFDiscov Nano
July 2025
Department of Physics, University of Surrey, Guildford, GU2 7XH, UK.
To be used as efficient alpha particle scintillator in the fields of nuclear security, nuclear nonproliferation and high-energy physics, scintillator screens must have high light output and fast decay properties. While there has been a great deal of progress in scintillation efficiency, achieving fast decay time properties are still a challenge. In this work, the near band edge (NBE) UV luminescence and alpha particle induced scintillation properties of vertically aligned densely packed ZnO nanorods (NRs) doped with Al, Ga, and In have been thoroughly investigated.
View Article and Find Full Text PDFAppl Radiat Isot
November 2025
Giresun University, Central Research Laboratory Application and Research Center, 28100 Giresun, Türkiye.
Composite materials comprising titanium diboride (TiB), unsaturated polyester resin, and pyrite (FeS) at varying weight percentages were fabricated and evaluated for their interaction with neutron and gamma radiation. This study adopts a comprehensive methodology, combining theoretical calculations, experimental measurements, and Monte Carlo simulations using PHITS and MCNP6. A strong correlation was observed among experimental results, WinXCOM data, and simulation outputs, with discrepancies remaining within approximately 5 %.
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