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Research at the University of Kentucky Accelerator Laboratory

Producción científica: Conference articlerevisión exhaustiva

1 Cita (Scopus)

Resumen

The Department of Physics and Astronomy at the University of Kentucky operates a 7-MV CN Van de Graaff accelerator that produces primary beams of protons, deuterons, and helium ions. An in-terminal pulsing and bunching system operates at 1.875 MHz and is capable of providing 1 ns beam bunches at an average current of several microamperes. Nearly all ongoing research programs involve secondary pulsed neutrons produced with gas cells containing deuterium or tritium, as well as with a variety of solid targets. Most experiments are performed at a target station positioned over a deep pit, so as to reduce the background created by backscattered neutrons. Recent experiments will be described; these include: measurements of n-p scattering total cross sections from En = 90 to 1800 keV to determine the n-p effective range parameter; the response of the plastic scintillator BC-418 below 1 MeV to low-energy recoil protons; n-p radiative capture cross sections important for our understanding of nucleosynthesis approximately 2 minutes after the occurrence of the Big Bang; γ-ray spectroscopy following inelastic neutron scattering to study nuclear structure relevant to double-β decay and to understand the role of phonon-coupled excitations in weakly deformed nuclei; and measurements of neutron elastic and inelastic scattering cross sections for nuclei that are important for energy production and for our global understanding of the interaction of neutrons with matter.

Idioma originalEnglish
Páginas (desde-hasta)440-447
Número de páginas8
PublicaciónPhysics Procedia
Volumen90
DOI
EstadoPublished - 2017
EventoConference on the Application of Accelerators in Research and Industry, CAARI 2016 - Fort Worth, United States
Duración: oct 30 2016nov 4 2016

Nota bibliográfica

Publisher Copyright:
© 2017 The Authors.

Financiación

This work was supported in part by grants from Department of Energy NNSA/SSAA Grant DE-NA0003348, the National Science Foundation under Grant No. PHY-1606890, and the Department of Energy NNSA/SSAA Grant DE-NA0002931. The authors would like to thank UK accelerator engineer Harvey Baber, MIT collaborators June Matthews and Brian Daub, U. S. Naval Academy collaborator Jeffrey Vanhoy, University of Kentucky graduate students Zachariah Miller, Jason McGinnis, Scott Miller, and Hongwei Yang, postdocs Erin Peters, Sharmistha Mukhopadhyay, and Anthony Ramirez, and UKAL director Steven W. Yates. This work was supported in part by grants from Department of Energy NNSA/SSAA Grant DE-NA0003348, the National Science Foundation under Grant No. PHY-1606890, and the Department of Energy NNSA/SSAA Grant DENA0002931.

FinanciadoresNúmero del financiador
Department of Energy NNSA/SSAADE-NA0003348
National Science Foundation Arctic Social Science ProgramDE-NA0002931, PHY-1606890
National Science Foundation Arctic Social Science Program

    ASJC Scopus subject areas

    • General Physics and Astronomy

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