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Dive into the research topics where David C. Argento is active.

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Featured researches published by David C. Argento.


Physics in Medicine and Biology | 2015

Rapid MCNP simulation of DNA double strand break (DSB) relative biological effectiveness (RBE) for photons, neutrons, and light ions.

Robert D. Stewart; Seth Streitmatter; David C. Argento; Charles Kirkby; John T. Goorley; Greg Moffitt; Tatjana Jevremovic

To account for particle interactions in the extracellular (physical) environment, information from the cell-level Monte Carlo damage simulation (MCDS) for DNA double strand break (DSB) induction has been integrated into the general purpose Monte Carlo N-particle (MCNP) radiation transport code system. The effort to integrate these models is motivated by the need for a computationally efficient model to accurately predict particle relative biological effectiveness (RBE) in cell cultures and in vivo. To illustrate the approach and highlight the impact of the larger scale physical environment (e.g. establishing charged particle equilibrium), we examined the RBE for DSB induction (RBEDSB) of x-rays, (137)Cs γ-rays, neutrons and light ions relative to γ-rays from (60)Co in monolayer cell cultures at various depths in water. Under normoxic conditions, we found that (137)Cs γ-rays are about 1.7% more effective at creating DSB than γ-rays from (60)Co (RBEDSB  =  1.017) whereas 60-250 kV x-rays are 1.1 to 1.25 times more efficient at creating DSB than (60)Co. Under anoxic conditions, kV x-rays may have an RBEDSB up to 1.51 times as large as (60)Co γ-rays. Fission neutrons passing through monolayer cell cultures have an RBEDSB that ranges from 2.6 to 3.0 in normoxic cells, but may be as large as 9.93 for anoxic cells. For proton pencil beams, Monte Carlo simulations suggest an RBEDSB of about 1.2 at the tip of the Bragg peak and up to 1.6 a few mm beyond the Bragg peak. Bragg peak RBEDSB increases with decreasing oxygen concentration, which may create opportunities to apply proton dose painting to help address tumor hypoxia. Modeling of the particle RBE for DSB induction across multiple physical and biological scales has the potential to aid in the interpretation of laboratory experiments and provide useful information to advance the safety and effectiveness of hadron therapy in the treatment of cancer.


Physics in Medicine and Biology | 2018

Dosimetric characteristics of the University of Washington Clinical Neutron Therapy System

Gregory B Moffitt; Robert D. Stewart; John T. Goorley; David C. Argento; Tatjana Jevremovic; Robert Emery; Landon Wootton; Upendra Parvathaneni; George E. Laramore

The University of Washington (UW) Clinical Neutron Therapy System (CNTS), which generates high linear energy transfer fast neutrons through interactions of 50.5 MeV protons incident on a Be target, has depth-dose characteristics similar to 6 MV x-rays. In contrast to the fixed beam angles and primitive blocking used in early clinical trials of neutron therapy, the CNTS has a gantry with a full 360° of rotation, internal wedges, and a multi-leaf collimator (MLC). Since October of 1984, over 3178 patients have received conformal neutron therapy treatments using the UW CNTS. In this work, the physical and dosimetric characteristics of the CNTS are documented through comparisons of measurements and Monte Carlo simulations. A high resolution computed tomography scan of the model 17 ionization chamber (IC-17) has also been used to improve the accuracy of simulations of the absolute calibration geometry. The response of the IC-17 approximates well the kinetic energy released per unit mass (KERMA) in water for neutrons and photons for energies from a few tens of keV up to about 20 MeV. Above 20 MeV, the simulated model 17 ion chamber response is 20%-30% higher than the neutron KERMA in water. For CNTS neutrons, simulated on- and off-axis output factors in water match measured values within ~2%  ±  2% for rectangular and irregularly shaped field with equivalent square areas ranging in a side dimension from 2.8 cm to 30.7 cm. Wedge factors vary by less than 1.9% of the measured dose in water for clinically relevant field sizes. Simulated tissue maximum ratios in water match measured values within 3.3% at depths up to 20 cm. Although the absorbed dose for water and adipose tissue are within 2% at a depth of 1.7 cm, the absorbed dose in muscle and bone can be as much as 12 to 40% lower than the absorbed dose in water. The reported studies are significant from a historical perspective and as additional validation of a new tool for patient quality assurance and as an aid in ongoing efforts to clinically implement advanced treatment techniques, such as intensity modulated neutron therapy, at the UW.


Physics in Medicine and Biology | 2016

MCNP6 model of the University of Washington clinical neutron therapy system (CNTS).

G Moffitt; Robert D. Stewart; John T. Goorley; David C. Argento; Tatjana Jevremovic

A MCNP6 dosimetry model is presented for the Clinical Neutron Therapy System (CNTS) at the University of Washington. In the CNTS, fast neutrons are generated by a 50.5 MeV proton beam incident on a 10.5 mm thick Be target. The production, scattering and absorption of neutrons, photons, and other particles are explicitly tracked throughout the key components of the CNTS, including the target, primary collimator, flattening filter, monitor unit ionization chamber, and multi-leaf collimator. Simulations of the open field tissue maximum ratio (TMR), percentage depth dose profiles, and lateral dose profiles in a 40 cm × 40 cm × 40 cm water phantom are in good agreement with ionization chamber measurements. For a nominal 10 × 10 field, the measured and calculated TMR values for depths of 1.5 cm, 5 cm, 10 cm, and 20 cm (compared to the dose at 1.7 cm) are within 0.22%, 2.23%, 4.30%, and 6.27%, respectively. For the three field sizes studied, 2.8 cm × 2.8 cm, 10.4 cm × 10.3 cm, and 28.8 cm × 28.8 cm, a gamma test comparing the measured and simulated percent depth dose curves have pass rates of 96.4%, 100.0%, and 78.6% (depth from 1.5 to 15 cm), respectively, using a 3% or 3 mm agreement criterion. At a representative depth of 10 cm, simulated lateral dose profiles have in-field (⩾ 10% of central axis dose) pass rates of 89.7% (2.8 cm × 2.8 cm), 89.6% (10.4 cm × 10.3 cm), and 100.0% (28.8 cm × 28.8 cm) using a 3% and 3 mm criterion. The MCNP6 model of the CNTS meets the minimum requirements for use as a quality assurance tool for treatment planning and provides useful insights and information to aid in the advancement of fast neutron therapy.


Quaternary Geochronology | 2016

The CRONUS-Earth Project: A synthesis

Fred M. Phillips; David C. Argento; Greg Balco; Marc W. Caffee; J. Clem; Tibor J. Dunai; Robert C. Finkel; Brent M. Goehring; John C. Gosse; Adam M. Hudson; A. J. Timothy Jull; Meredith A. Kelly; Mark D. Kurz; Devendra Lal; Nathaniel A. Lifton; Shasta M. Marrero; Kunihiko Nishiizumi; Robert C. Reedy; Joerg M. Schaefer; John O. Stone; Terry W. Swanson; Marek Zreda


Nuclear Instruments & Methods in Physics Research Section B-beam Interactions With Materials and Atoms | 2013

Modeling the earth’s cosmic radiation

David C. Argento; Robert C. Reedy; John O. Stone


Nuclear Instruments & Methods in Physics Research Section B-beam Interactions With Materials and Atoms | 2013

Ultra-sensitive measurements of 36Cl and 236U at the Australian National University

L.K. Fifield; S.G. Tims; John O. Stone; David C. Argento; M. De Cesare


Nuclear Instruments & Methods in Physics Research Section B-beam Interactions With Materials and Atoms | 2010

Chlorine-36 in seawater

David C. Argento; John O. Stone; L. Keith Fifield; S.G. Tims


Quaternary Geochronology | 2015

Physics-based modeling of cosmogenic nuclides part II – Key aspects of in-situ cosmogenic nuclide production

David C. Argento; John O. Stone; Robert C. Reedy; Keran O'Brien


Quaternary Geochronology | 2015

Physics-based modeling of cosmogenic nuclides part I – Radiation transport methods and new insights

David C. Argento; John O. Stone; Robert C. Reedy; Keran O'Brien


Quaternary Geochronology | 2016

Where now? Reflections on future directions for cosmogenic nuclide research from the CRONUS Projects

Fred M. Phillips; David C. Argento; Didier Bourlès; Marc W. Caffee; Tibor J. Dunai; Brent M. Goehring; John C. Gosse; Adam M. Hudson; A. J. Timothy Jull; Meredith A. Kelly; Nathaniel A. Lifton; Shasta M. Marrero; Kuni Nishiizumi; Robert C. Reedy; John O. Stone

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John O. Stone

University of Washington

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Robert C. Reedy

Planetary Science Institute

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John T. Goorley

Los Alamos National Laboratory

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S.G. Tims

Australian National University

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Fred M. Phillips

New Mexico Institute of Mining and Technology

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