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1 LA-UR- Approved for public release; distribution is unlimited. Title: Author(s): Submitted to: Los Alamos National Laboratory, an affirmative action/equal opportunity employer, is operated by the University of California for the U.S. Department of Energy under contract W-7405-ENG-36. By acceptance of this article, the publisher recognizes that the U.S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, or to allow others to do so, for U.S. Government purposes. Los Alamos National Laboratory requests that the publisher identify this article as work performed under the auspices of the U.S. Department of Energy. Los Alamos National Laboratory strongly supports academic freedom and a researcher s right to publish; as an institution, however, the Laboratory does not endorse the viewpoint of a publication or guarantee its technical correctness. Form 836 (8/00)
2 Medical Physics SDEF Sources By Tim Goorley, X-5 LA-UR
3 Abstract While it is important to accurately represent the appropriate geometry for Medical Physics simulations, it is just as important to accurately represent the radiation source. The following slides give several examples of photon and neutron sources encountered in Medical Physics applications. These examples show how to construct the SDEF card in MCNP to simulate various radiation sources.
4 SDEF Sources Co-60 Photon Source (Exercises 1-3) Epithermal Neutron Beam (Exercises 4-5)
5 Co-60 Photon Source Photon Energies: MeV, MeV Both energies equally probable Isotropic Exercise 1: Point Source at origin Exercise 2: Source Sphere (equally prob)
6 Solutions Simple input deck for Co-60 point or sphere source imp:p= imp:p=0 10 so 5.0 $ Sphere at origin, 5 cm radius c sdef erg=d1 cel=100 par=2 $ What would this line do? [Point origin] c sdef erg=d1 cel=100 par=2 rad=2.0 $ What would this line do? [Thin Shell Src] sdef erg=d1 cell=100 par=2 rad=d2 $ This is a homogeneous sphere source si1 L $ Discrete Co-60 Energies, in MeV sp1 D $ Equiprobable si2 H $ Radial Bin Distribution from 0.0 cm to 2.0 cm sp $ Power law sampling to 2 nd power, for spherical sources mode p $ Photon Source nps 50 m $ Water, note molecular formula is atom fraction print
7 Co-60 Seed Source Exercise 3: 2 hemispheres rad = 1.0 cm 1 cylinder rad = 1.0 cm, length = 1.0 cm Hint: Use Cell Acceptance
8 Solutions Exercise 3 SDEF ERG=D1 RAD=D2 CEL = 100 What would the following lines do? SDEF ERG=D1 CEL=100 SDEF ERG=D1 RAD=2.0
9 Exercise 3 Input Deck Simple input deck for Co-60 Seed source :-20:-30 imp:p= imp:p= imp:p=0 10 s s rcc so 5.0 c sdef erg=d1 cel=100 par=2 c sdef erg=d1 cel=100 par=2 rad=2.0 sdef erg=d1 cell=100 par=2 rad=d2 si1 L sp1 D si2 H sp mode p nps 50 m print $ What would this line do? $ What would this line do?
10 Exercise 3 Plotting These Vised Source plotting pictures show the difference between SP (left correct) and SP (right not homogeneous) Do you see a difference? Different colors for different energies
11 Neutron Beam Monoenergetic Epithermal N s 5.0 KeV Beam 5.0 cm radius Travels from x to +x [monodirectional] Starts at x= -5.0 Pass through a 1 cm rad ball of water at origin Exercise 4: Monodirectional beam
12 Neutron Beam Ex 4 soln Exercise 4 SDEF POS= VEC=1 0 0 $ What if no vec card? AXS=1 0 0 $ What if no axs card? DIR=1.0 $ What if no dir card? RAD=D3 ERG=0.005 PAR=1 SI3 H SP3-21 1
13 Exercise 4 Plotting These Vised Source plotting pictures show the difference between SP (left not correct) and SP (right correct) Do you see a difference?
14 Exercise 4 Input Deck This is a simple monodir neutron beam problem C Little geometry is needed imp:n= imp:n=1 $ What if imp:n=0? imp:n=0 10 so so 20.0 mode n p m sdef pos axs $ What happens if no axs? C If no axs, source becomes a spherical source vec $ What happens if no vec? C If no vec, no reference direction for particle direction dir 1.0 $ What happens if no dir? [isotropic source] erg=0.005 rad=d4 par 1 ext=0.0 $ A disk source is a degenerate cylinder source si4 H sp $ Power Law, power=1 for disk sources print nps 50
15 Exercise 5 Add beam divergence of 5 Think about difference between: Y A B 5 5 X Both are possible in MCNP (Do Both!)
16 Neutron Beam Ex 5 soln A Exercise 5 SDEF POS= VEC= AXS=1 0 0 DIR=1 PAR=1 RAD=D3 ERG=0.005 Exercise 5 SDEF POS= VEC= AXS= DIR=1 PAR=1 RAD=D3 ERG=0.005 The difference between these two is the cross section of the beam. The one on the right has a circular cross section, the one on the left has an elliptical cross section
17 Beam Cross Section AXS & VEC different AXS & VEC same Which did you intend?
18 Neutron Beam Ex 5 soln B Exercise 5 SDEF POS= VEC=1 0 0 AXS=1 0 0 DIR= $ = cos(5 deg*pi/180) PAR=1 RAD=D3 ERG=0.005
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FLUID COMPOSITION ANALYSIS BY MULTIPLE GAMMA-RAY BEAM AND MODALITY MEASUREMENTS Geir Anton Johansen 1,3 and Stein-Arild Tjugum 2,3 1 University of Bergen, Department of Physics and Technology Allégaten
............... [2] At the time of purchase of a Strontium-90 source, the activity is 3.7 10 6 Bq.
1 Strontium-90 decays with the emission of a β-particle to form Yttrium-90. The reaction is represented by the equation 90 38 The decay constant is 0.025 year 1. 90 39 0 1 Sr Y + e + 0.55 MeV. (a) Suggest,
