Gregory Bizarri

Dr. Gregory Bizarri


Research Focus & Metrics

Academic Career Length

24Years (2003-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 June 2005 in Journal of Luminescence
Verified
Journal Article
Closed access
GBGregory Bizarri
Gregory Bizarri
BMB. Moine
B. Moine

13 October 2011 in IEEE Transactions on Nuclear Science
Verified
Journal Article
Closed access
SPStephen A. Payne
Stephen A. Payne
WMWilliam W. Moses
William W. Moses
SSSteven Sheets
Steven Sheets
LALarry Ahle
Larry Ahle
NCNerine J. Cherepy
Nerine J. Cherepy
WCWoon-Seng Choong
Woon-Seng Choong
We report measurements of electron response of scintillators, including data on 29 halides, oxides, organics, and fluorides. We model the data based on combining the theories of: Onsager, to account for formation of excitons and excited activators; Birks, to allow for exciton-exciton annihilation; Bethe-Bloch, to relate electron stopping to its energy; and Landau, to describe how fluctuations in the linear energy deposited (dE/dx) lead to nonproportionality's contribution to resolution. In general there is satisfactory agreement with experiment, in terms of fitting the electron response data and reproducing the literature values of resolution. We find that the electron response curve shapes are more affected by the host lattice than by the activator or its concentration.

15 February 2009 in Journal of Applied Physics
Verified
Journal Article
Closed access
PDF file
GBGregory Bizarri
Gregory Bizarri
WMW. W. Moses
W. W. Moses
JSJ. Singh
J. Singh
AVA. N. Vasil’ev
A. N. Vasil’ev
RWR. T. Williams
R. T. Williams
Analytical expressions for the local light yield as a function of the local deposited energy (−dE/dx) and total scintillation yield integrated over the track of an electron of initial energy E are derived from radiative and/or nonradiative rates of first through third order in density of electronic excitations. The model is formulated in terms of rate constants, some of which can be determined independently from time-resolved spectroscopy and others estimated from measured light yield efficiency as a constraint assumed to apply in each kinetic order. The rates and parameters are used in the theory to calculate scintillation yield versus primary electron energy for comparison to published experimental results on four scintillators. Influence of the track radius on the yield is also discussed. Results are found to be qualitatively consistent with the observed scintillation light yield. The theory can be applied to any scintillator if the rates of the radiative and nonradiative processes are known.

5 March 2012 in IEEE Transactions on Nuclear Science
Verified
Journal Article
Closed access
WMW. W. Moses
W. W. Moses
GBGregory Bizarri
Gregory Bizarri
RWR. T. Williams
R. T. Williams
SPS. A. Payne
S. A. Payne
AVAndrey Vasil'ev
Andrey Vasil'ev
WCW.-S. Choong
W.-S. Choong
Recent years have seen significant advances in both theoretically understanding and mathematically modeling the underlying causes of scintillator non-proportionality. The core cause is that the interaction of radiation with matter invariably leads to a non-uniform ionization density in the scintillator, coupled with the fact that the light yield depends on the ionization density. The mechanisms that lead to the luminescence dependence on ionization density are incompletely understood, but several important features have been identified, notably Auger-like processes (where two carriers of excitation interact with each other, causing one to de-excite non-radiatively), the inability of excitation carriers to recombine (caused either by trapping or physical separation), and the carrier mobility. This paper reviews the present understanding of the fundamental origins of scintillator non-proportionality, specifically the various theories that have been used to explain non-proportionality.

1 December 2009 in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Journal Article
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EBE.D. Bourret-Courchesne
E.D. Bourret-Courchesne
GBGregory Bizarri
Gregory Bizarri
RBR. Borade
R. Borade
ZYZ. Yan
Z. Yan
SHS.M. Hanrahan
S.M. Hanrahan
SDS.E. Derenzo
S.E. Derenzo

14 May 2007 in Physical Review B
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Journal Article
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GBGregory Bizarri
Gregory Bizarri
PDP. Dorenbos
P. Dorenbos
The scintillation yield and decay time of LaBr3 doped with 0.2%, 0.5%, and 5% cerium were studied between 80K and 600K. LaBr3:5%Ce3+ on a photomultiplier tube shows at 300K a very high scintillation yield of 22800 photoelectrons per MeV (64000 photons per MeV) with a decay time of 16ns. At 600K the yield decreases by ≃15%. The scintillation yield of LaBr3:0.2%Ce3+ is 19800 photoelectrons per MeV (56000 photons per MeV) at 300K with a decrease by ≃50% at 600K and a main scintillation decay time around 30ns. The appearance of slow components in the Ce emission indicates a relatively slow energy transfer from the host crystal to Ce. The presence or absence of slow components depends on both concentration and temperature. The results are analyzed and interpreted with a model that comprises prompt charge carrier trapping by Ce and delayed excitation of Ce by means of thermally activated transport of self-trapped exciton defects. The results of the study provide detailed information on the scintillation mechanism. Besides presenting experimental data, the different energy transfer processes are quantified.