26.02.2013 Views

Program - Brookhaven National Laboratory

Program - Brookhaven National Laboratory

Program - Brookhaven National Laboratory

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

LE 5 5:00 PM<br />

Method of Best Representation for Averages in Data Evaluation<br />

M. Birch and B. Singh<br />

Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada<br />

A novel statistical approach to the averaging procedures in data evaluation is developed based on producing<br />

a mean probability density function to represent the data set. This Method of Best Representation (MBR)<br />

is shown to have desirable properties including being robust to outliers and agreement with the standard<br />

weighted average (weighting by the reciprocal of the square of the uncertainty in the measurement) in<br />

the case of non-discrepant data. Examples from isotopic half-life and gamma-ray intensity data will be<br />

discussed to illustrate the method.<br />

LE 6 5:15 PM<br />

New Model for ab initio Calculation of Atomic Radiations in Nuclear Decay<br />

A.E. Stuchbery, T. Kibédi, B.Q. Lee, K.A. Robertson,<br />

Department of Nuclear Physics, Research School of Physics and Engineering, The Australian <strong>National</strong><br />

University, Canberra, ACT 0200, Australia<br />

F.G. Kondev<br />

Argonne <strong>National</strong> <strong>Laboratory</strong>, Argonne, Illinois 60439, USA<br />

Unstable atomic nuclei release excess energy through various radioactive decay processes by emitting particles<br />

(e.g. neutron, alpha, beta) or electromagnetic radiation (gamma-ray photons). Most of the applications<br />

of nuclear isotopes make use of the interactions of their radiations passing through material, which depend<br />

on the type (photons, neutral or charged particles) and the transferred energy. The ionizing radiation<br />

produced by radioisotopes goes beyond the alpha, beta and gamma radiation from the nuclear decay. A<br />

cascade of Auger electrons is often emitted in the atomic relaxation process following a nuclear event.<br />

This radiation is particularly important for medical applications [1]. Since the early 70s, when the use of<br />

Auger electrons for cancer therapy was first suggested (see the review by Howell [2]), considerable advances<br />

have been made in understanding the radiobiological effect of low energy electrons. On the other hand,<br />

a comparison of the calculated Auger yields for selected radioisotopes [3] has identified significant differences<br />

between the various computational models. These differences stem from differences in the physical<br />

assumptions of the models as well as differences in the adopted atomic transition rates and energies. In<br />

this paper we review the current knowledge on Auger emission rates in nuclear decay and present a new<br />

ab initio model which evaluates the transition energies and rates from first principles using the GRASP2k<br />

[4] and RATIP [5] codes. A full Monte Carlo approach was adopted to treat the stochastic nature of the<br />

creation of the primary atomic vacancies after nuclear decay, as well as for the subsequent propagation of<br />

vacancies. Our first numerical results on selected medical radioisotopes will be presented.<br />

[1] A.L. Nichols, S.M. Qaim, R.C. Noy, Summary Report Technical Meeting on Intermediate-term Nuclear<br />

Data Needs for Medical Applications: Cross Sections and Decay Data, AEA Nuclear Data Section,<br />

INDC(NDS)-0596 (2011) [2] R.W. Howell, Journal of Radiation Biology, 84, 959 (2008) [3] B.Q. Lee, T.<br />

Kibédi, A.E. Stuchbery, K.A. Robertson, Computational and Mathematical Methods in Medicine (2012), in<br />

press, doi:10.1155/2012/651475 [4] P. Jönsson, X. He, C. Froese Fischer, I. P. Grant, Computer Physics<br />

Communications 177, 597 (2007) [5] S. Fritzsche, Computer Physics Communications 183, 1525 (2012)<br />

LE 7 5:30 PM<br />

182

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!