Monte Carlo Radiation Transport Kenny Wood

Similar documents
Monte Carlo Radiation Transport Kenny Wood

MCRT L10: Scattering and clarification of astronomy/medical terminology

Enrico Fermi and the FERMIAC. Mechanical device that plots 2D random walks of slow and fast neutrons in fissile material

Monte Carlo Sampling

MCRT L8: Neutron Transport

Monte Carlo Radiation Transfer I

Reflection Nebulae: can reflections from grains diagnose albedo?

Chemistry 500: Chemistry in Modern Living. Topic 5: The Fires of Nuclear Fission. Atomic Structure, Nuclear Fission and Fusion, and Nuclear.

Radiation Friend or Foe? Saturday Physics for Everyone 7 Oct 2017 Kevin Pitts

Unit 6 Nuclear Radiation Parent Guide. What is radioactivity and why are things radioactive?

Science 30 Unit C Review Outline GCCHS. Negatively charged Positively charged Coulomb Conductor Electric potential difference

Stars AS4023: Stellar Atmospheres (13) Stellar Structure & Interiors (11)

Monte Carlo Methods:

MCRT: L4 A Monte Carlo Scattering Code

Name Date Class NUCLEAR RADIATION. alpha particle beta particle gamma ray

APPENDIX A RADIATION OVERVIEW

MCRT L9: Neutron Transport

Emphasis on what happens to emitted particle (if no nuclear reaction and MEDIUM (i.e., atomic effects)

Lecture 1 Bioradiation

THE GALAXY. Spitzer Space Telescope Images & Spectra: 3µm - 170µm

Astronomy 1 Fall Reminder: When/where does your observing session meet? [See from your TA.]

Physics Courses. Courses. Physics Courses 1

Spectral energy distribution fitting with MagPhys package

Master of Science Astrophysics

Atomic & Nuclear Physics

Masters in Astrophysics

College Physics B - PHY2054C

Name Period. CRHS Academic Chemistry Unit 3 - Atomic Structure & Nuclear Chemistry. Homework. Due Date Assignment On-Time (100) Late (70)

Radiation Basics. Mary Lou Dunzik-Gougar, PhD Idaho State University/Idaho National Laboratory. ANS Teachers Workshop Anaheim, CA November 2014

1. Work ( ) = Force ( ) X distance ( ). 2. Force is measured in newtons and measures how hard something is or.

Chapter 21

CHAPTER 1 RADIATION AND RADIOACTIVITY

Atomic Structure & Nuclear Chemistry Unit 3 Notes

Core Questions Physics unit 4 - Atomic Structure

Waves & Radiation exam questions

PHYSICS A2 UNIT 2 SECTION 1: RADIOACTIVITY & NUCLEAR ENERGY

INAYA MEDICAL COLLEGE (IMC) RAD LECTURE 1 RADIATION PHYSICS DR. MOHAMMED MOSTAFA EMAM

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017

Radiation Awareness Training. Stephen Price Office of Research Safety

Lecture Outlines Chapter 32. Physics, 3 rd Edition James S. Walker

INAYA MEDICAL COLLEGE (IMC) RAD LECTURE 1 RADIATION PHYSICS DR. MOHAMMED MOSTAFA EMAM

Nuclear Chemistry Unit

Physics 3204 UNIT 3 Test Matter Energy Interface

Nuclear Spectroscopy: Radioactivity and Half Life

Radioactivity pp Topic 9: Nuclear Physics Ch. 10. Radioactivity. Radioactivity

Chapter 10 The Interstellar Medium

Isotopes. An isotope is an atom of the same element (same number of protons) that varies in the number of neutrons.

Isotopes. An isotope is an atoms of the same element (same number of protons) that vary in the number of neutrons.

Lecture PowerPoint. Chapter 31 Physics: Principles with Applications, 6 th edition Giancoli

11/10/2014. Chapter 1: Introduction to Medical Imaging. Projection (Transmission) vs. Emission Imaging. Emission Imaging

22.54 Neutron Interactions and Applications (Spring 2004) Chapter 1 (2/3/04) Overview -- Interactions, Distributions, Cross Sections, Applications

The basic structure of an atom is a positively charged nucleus composed of both protons and neutrons surrounded by negatively charged electrons.

Lecture PowerPoints. Chapter 31 Physics: Principles with Applications, 7th edition Giancoli

Name: COMBINED SCIENCE Topics 4, 5 & 6 LEARNING OUTCOMES. Maintain a record of your progress Use the booklet to guide revision

Radiation Safety. PIXE PAN 2008 Ed Stech University of Notre Dame

Nuclear Chemistry AP Chemistry Lecture Outline

SYLLABUS. COURSE DESCRIPTION (Course information, basic description, general information, teaching overview, required equipment and preparation, etc.

Isotopes Atoms of an element (same # p+) that differ in their number of neutrons

Radiation Safety Talk. UC Santa Cruz Physics 133 Winter 2018

Radioactivity. L 38 Modern Physics [4] Hazards of radiation. Nuclear Reactions and E = mc 2 Einstein: a little mass goes a long way

((Radiation )) أيهمدغيم. Ionizing RadiationNon-ionizing radiation. This is the last sheet for Dr. Madi s lectures & its number is ((22)).

4.4.1 Atoms and isotopes The structure of an atom Mass number, atomic number and isotopes. Content

Summary of changes (certificate to new GCSE)

UNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY

Laser Beam Interactions with Solids In absorbing materials photons deposit energy hc λ. h λ. p =

Radiation Safety Training Session 1: Radiation Protection Fundamentals and Biological Effects

City University of Hong Kong

A Short Course on Geant4 Simulation Toolkit. Introduction.

RADIATION AND NUCLEAR SCIENCE 10 EARTH SCIENCE ENERGY

Dust radiative transfer modelling. Maarten Baes

Particles involved proton neutron electron positron gamma ray 1

Recap I Lecture 41 Matthias Liepe, 2012

Properties of the nucleus. 9.1 Nuclear Physics. Isotopes. Stable Nuclei. Size of the nucleus. Size of the nucleus

A World of Dust. Bare-Eye Nebula: Orion. Interstellar Medium

(Triple Science) Physics Paper 1

Wallace Hall Academy Physics Department. Radiation. Pupil Notes Name:

CRaTER Science Requirements

The Atomic Nucleus & Radioactive Decay. Major Constituents of an Atom 4/28/2016. Student Learning Outcomes. Analyze radioactive decay and its results

Basics of Monte Carlo Simulation

Physics and Chemistry of the Interstellar Medium

Lecture5PracticeQuiz.txt

Nuclear Science Merit Badge Workbook

Astronomy II (ASTR-1020) Homework 2

Properties of the nucleus. 8.2 Nuclear Physics. Isotopes. Stable Nuclei. Size of the nucleus. Size of the nucleus

12/1/17 OUTLINE KEY POINTS ELEMENTS WITH UNSTABLE NUCLEI Radioisotopes and Nuclear Reactions 16.2 Biological Effects of Nuclear Radiation

Industrial Hygiene: Assessment and Control of the Occupational Environment

Reminders! Observing Projects: Both due Monday. They will NOT be accepted late!!!

Unit 12: Nuclear Chemistry

21/11/ /11/2017 Atomic Structure AQA Physics topic 4

The diagram below shows a radioactive isotope going through several half-lives as it decays.

Nobel prizes in nuclear and reactor physics. Szabolcs Czifrus Institute of Nuclear Techniques BME

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

L-35 Modern Physics-3 Nuclear Physics 29:006 FINAL EXAM. Structure of the nucleus. The atom and the nucleus. Nuclear Terminology

Delayed neutrons in nuclear fission chain reaction

Unit 3: Chemistry in Society Nuclear Chemistry Summary Notes

Astronomy 104: Second Exam

Final Exam. Evaluations. From last time: Alpha radiation. Beta decay. Decay sequence of 238 U

Nuclear Reactions and E = mc 2. L 38 Modern Physics [4] Hazards of radiation. Radiation sickness. Biological effects of nuclear radiation

Name Date Class NUCLEAR CHEMISTRY

Year 11 Physics booklet Topic 1 Atomic structure and radioactivity Name:

Transcription:

MCRT: L0 Some background, what previous courses students should look over, gentle introduction/recap of probabilities Get an idea of computer programming experience of the class Overview of course structure and assessment

Monte Carlo Radiation Transport Kenny Wood kw25@st-andrews.ac.uk A practical approach to the numerical simulation of radiation transport Develop programs for the random walks of photons and neutrons using Monte Carlo techniques Will refer to previous courses on optics, radiation, neutrons, atomic physics, biological tissue structure, some hydrodynamics Guest lectures in week 3 from Prof Steve Jacques (Oregon) on Monte Carlo radiation transfer in biological tissue and medical physics

Astrophysics Interpreting data via 3D radiation transfer modeling Heating of dust and gas, thermal pressure, radiation pressure Radiation-magneto-hydrodynamics

Dusty Ultra Compact H II Regions ONE 3D model can explain ALL UCHII SEDs!! Indebetouw, Whitney, Johnson, & Wood (2006)

Hierarchical Density Structure Fractal generating algorithm reproduces observed structure and fractal dimension, D, of clouds in interstellar medium 2D: P ~ A D/2 ; Circle: D =1 ISM clouds: D ~ 1.3 Radiation transfer in clouds Elmegreen (1997)

Monte Carlo scattered light Simulations of fractal clouds NGC 7023 Reflection Nebula 3D density: viewing angle effects Mathis, Whitney, & Wood (2002)

Atmospheric Physics Clouds important for photon transport and temperature structure of atmosphere

Medical Physics Light activated treatments such as photodynamic therapy: how deep does the radiation penetrate into skin and tissue? Imaging using x-ray, ultraviolet, optical, infrared, & polarised light Optical tweezers, photo-acoustic imaging, nuclear medicine, etc, etc Monte Carlo simulations of computed topography (CT) x-ray imaging doses Rensselaer Polytechnic Institute

Nuclear Physics & Neutron Transport Compute controlled criticality assemblies & geometries for nuclear fission reactors Nuclear safety radioactive shielding calculations Uncontrolled reactions critical masses for bombs Chain reaction in 235 U Chicago Pile 1, December 1942 World s first artificial nuclear reactor

Course Structure Lectures on MCRT techniques and outline of FORTRAN programs Computer lab sessions for what you ll need in FORTRAN and to develop a code for photon random walks in a uniform density sphere Tutorial-style problems to do in groups No final exam, 100% continuous assessment: 40% for two homework sheets of written problems and short programs & subroutines 40% for one large project 20% for one short project

Remind yourself of Refractive index, Snell s Law, Fresnel reflection & refraction (PH1011 Waves & Optics) Polarization (PH3007 Electromagnetism & PH4035 Principles of Optics) Ionization potentials, atomic term diagrams PH4037 (Physics of Atoms) Equations of hydrodynamics, pressure & forces (PH4031 Fluids) Probability theory: probability distribution function (PDF) and cumulative distribution function (CDF) Numerical integration, Simpsons rule, quadrature

Intensity, luminosity, flux, radiation pressure (many astronomy courses) Biological tissue optics, skin structure, light-tissue interactions (PH5016 Biophotonics) Neutron cross sections: scattering, absorption, fission Fission products, slow/fast & prompt/delayed neutrons Chain reactions, critical mass, moderators PH4022 or PH4040 (Nuclear & Particle Physics)

Programming in FORTRAN77 You ll need: text editor; FORTRAN compiler (gfortran); graphics package for plotting lines, contours, 3D visualisation By Monday create file called hello.f Compile it: gfortran hello.f Run the executable:./a.out program hello implicit none Note six spaces before text starts on each line! print *, Hello stop end

Buffon s needles Georges-Louis Leclerc Comte de Buffon 1707-1788 What is the probability that a needle will cross a line?

θ l x s Needles of length l Line separation s x = distance from needle centre to closest line Needle touches/crosses line if x l 2 sinθ Probability density function: function of a variable that gives probability for variable to take a given value Exponential distribution: p(x) = e -x, for x in range 0 to infinity Uniform distribution: p(x) = 1/L, for x in range 0 to L Normalised over all x: p(x) dx =1 0

Probability x lies in range a < x < b is ratio of areas under the curve b p(x) dx a P = p(x) dx 0 x is distributed uniformly between (0, s/2), θ in range (0, π/2) p(x) = 2/s, p(θ) = 2/π Variables x and θ independent, so joint probability is p(x, θ) = 4/(s π)

Probability of a needle touching a line (l < s) is P = π / 2 0 0 l / 2 sinθ 4 dx dθ = 2l sπ sπ Drop lots of needles. Probability of needle crossing line is P = Number of needles crossing lines Total number of needles dropped Can estimate π : π = 2 l sp