J. Folkerts

ORCID: 0000-0002-9807-9209
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About
Contact & Profiles
Research Areas
  • Neutrino Physics Research
  • Radiation Detection and Scintillator Technologies
  • Dark Matter and Cosmic Phenomena
  • Particle Detector Development and Performance
  • Astrophysics and Cosmic Phenomena
  • Nuclear Physics and Applications
  • Medical Imaging Techniques and Applications

Wichita State University
2022-2024

10.1016/j.nima.2025.170597 article EN Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 2025-05-01

10.1016/j.nima.2023.168064 article EN publisher-specific-oa Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 2023-01-21

10.1016/j.nima.2024.170116 article EN Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 2024-11-01

Abstract Low energy anti-neutrinos detected from reactors or other sources have typically used the conversion of an anti-neutrino on Hydrogen, producing a positron and free neutron. This neutron is subsequently captured secondary element with large capture cross-section such as gadolinium cadmium. With most captures gadolinium, it possible to get two three delayed gamma signals known occur. Modern experiments can make measurements timing order 25 ns. Fast electronics like these allow for...

10.1088/1748-0221/19/06/p06037 article EN Journal of Instrumentation 2024-06-01

10.1016/j.nima.2024.170121 article EN Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 2024-12-09

The concept of putting a neutrino detector in close orbit the sun has been unexplored until very recently. primary scientific return is to vastly enhance our understanding solar interior, which major NASA goal. Preliminary calculations show that such spacecraft, if properly shielded, can operate space environments while taking data from interactions. These interactions be distinguished random background rates electromagnetic emissions, galactic charged cosmic-rays, and gamma-rays by using...

10.48550/arxiv.2206.00703 preprint EN cc-by arXiv (Cornell University) 2022-01-01
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