Radioactivity – inverse square law, absorption, and rates presentation for Apr. 30, 2008 by Dr. Brian Davies, WIU Physics Dept.

Slides:



Advertisements
Similar presentations
Lecture 2, January 19 Conclusion of Mathematics Review with Examples Historical Timeline in Nuclear Medicine Radiation Safety Introduction Image of the.
Advertisements

NE Introduction to Nuclear Science Spring 2012
LOJ Feb 2004 Radioactivity 2 Ionizing Power and Penetrating Power.
My Chapter 29 Lecture.
NUCLEAR CHEMISTRY The Basics. The Nucleus The nucleus is composed of nucleons –protons –neutrons A nucleus is characterized by two numbers –atomic mass.
Nuclear Instability.
Chapter 30 Nuclear Physics
Charged Particle Radiation
Radioactivity – review of laboratory results For presentation on May 2, 2008 by Dr. Brian Davies, WIU Physics Dept.
Radiation – definitions of activity, dose, and dose rates presentation for May 2, 2008 by Dr. Brian Davies, WIU Physics Dept.
Nuclear Physics Selected Topics 2  Radioactivity.
Radioactivity – types of decays presentation for April 28, 2008 by Dr. Brian Davies, WIU Physics Dept.
Interactions with Matter
Radioactivity – decay rates and half life presentation for April 30, 2008 by Dr. Brian Davies, WIU Physics Dept.
Interaction of radiation with matter - 3
Quantum Physics and Nuclear Physics
Alpha Beta Gamma. Lesson Contents 1.Physical properties of ,  and  2.Penetrating power of ,  and  3.N v Z  graphs 4.Decay laws.
THE EXTERNAL HAZARD Radiation Protection.
Interaction of Gamma-Rays - General Considerations uncharged transfer of energy creation of fast electrons.
External Radiation Exposure Control
Radiation therapy is based on the exposure of malign tumor cells to significant but well localized doses of radiation to destroy the tumor cells. The.
Stopping Power The linear stopping power S for charged particles in a given absorber is simply defined as the differential energy loss for that particle.
NUCLEAR PHYSICS & RADIOACTIVITY PHYSICS - UNIT ONE.
Today’s Title: CW: Ionising radiation
Radiation: Particles and Energy.
Nuclear _____________of atom is changed Particles or energy is absorbed or emitted from nucleus Can involve one atom or multiple atoms New elements can.
Nuclear radiation. What do we mean by Radioactivity? Radioactive decay is the process in which an unstable atomic nucleus loses energy by emitting radiation.
NUCLEAR VS. CHEMICAL CHEMICAL reactions involve rearranging of atoms: e.g., H 2 +O 2  H 2 O No new atoms are created. Chemistry involves electrons only.
Unit 2: The Atom Nuclear Decay. Band Of Stability  Atoms that lie outside the band of stability are unstable  Atoms 1-20 n 0 /p + ratio must be 1:1.
Radioactivity!.
1 Nuclear Stability The larger the atom, the greater the proportion of the nucleus that must be neutrons. –The A/Z ratio is greater than 2 (or the N to.
Alpha Beta Gamma.
Radioactive Decay Alpha, Beta, and Gamma Decay. Radioactivity Emission of particles and energy from the nucleus of certain atoms This happens through.
Radiation Quality Chapter 4. X-ray Intensity Intensity: the amount of energy present per unit time per unit area perpendicular to the beam direction at.
Alpha and Beta Interactions
proton mass, m p = x kg = u neutron mass, m n = x kg = u electron mass, m e = x 10.
Interactions of radiation with Matter
ACADs (08-006) Covered Keywords Exposure, gamma ray constant, time, distance, shielding, shield placement, dose rate, sky shine, stay time, inverse square,
Nuclear Chemistry – Radioactive Decay Tuesday, October 13 th, 2015 Textbook pages 799 – 802, 807 – 808.
The production of X-Rays X-Rays are produced whenever charged particles are slowed down or stopped. X-rays are generated via interactions of the accelerated.
IB Assessment Statements Topic 13.2, Nuclear Physics Explain how the radii of nuclei may be estimated from charged particle scattering experiments.
Determining Radiation Intensity
Nuclear Physics and Radioactivity AP Physics Chapter 30.
GROUP 4 Firdiana Sanjaya ( ) Ana Alina ( )
Nuclear Decay. Radioactivity The emission of high-energy radiation or particles from the nucleus of a radioactive atom.
Interaction Ionizing Radiation with Matter BNEN Intro William D’haeseleer BNEN - Nuclear Energy Intro W. D'haeseleer
INTERACTIONS OF RADIATION WITH MATTER. twCshttp:// twCs
Energy Unit Learning Goal 3: Examine how changes in the nucleus of an atom result in emissions of radioactivity.
Nuclear Decay You will be learning: 1.What is alpha, beta, and gamma radiation. 2.Know the half-life of a radioactive material. 3.How to describe the process.
Interaction of x-ray photons (and gamma ray photons) with matter.
RTT 425 Radiation Therapy Physics Radiation Quality, Chapter 4 From Stanton and Stinson: Applied physics for Radiation Oncology.
Unstable Nuclei and Radioactive Decay Radioactivity – spontaneous emission of radiation Radiation – rays and particles emitted from a radioactive material.
Nuclear Chemistry The alpha particle (  ) The beta particle (  ) Gamma radiation (γ)
Absorption and ‘Spreading Out’ of ionising radiation. There are two mechanisms which cause the intensity of ionising radiation t decrease as distance from.
AQA A2 Physics A Nuclear Physics Section 9 Properties of Alpha, Beta and Gamma Radiation.
Electromagnetic Spectrum
Radioactivity – review of laboratory results
NUCLEAR DECAY.
Radioactive Decay Section 21.2.
Devil physics The baddest class on campus IB Physics
NUCLEAR DECAY.
Summary of alpha etc.
Interaction of Radiation with Matter
Logarithmic Functions
Log-log graph of the exponential exp(-x)
Radioactivity – decay rates and half life
Radioactivity GEOG/PHYS 182.
Radioactivity – inverse square law, absorption, and rates
Radioactivity – review of laboratory results
Presentation transcript:

Radioactivity – inverse square law, absorption, and rates presentation for Apr. 30, 2008 by Dr. Brian Davies, WIU Physics Dept.

Inverse square law for radiation Particles and photons emitted by radioactive nuclei continue moving until they are absorbed by some material. The particles (or photons) that leave the sample will continue to move out in a radial direction. The number that pass through an imaginary sphere of radius r in some interval of time is the same for different radii, but the area of the sphere depends on the radius. A = 4  r 2 Therefore, the number per unit area per unit time depends on the radius.

Inverse square law

Relation between source activity and intensity at various radii Suppose that S is the number of particles emitted by the source per unit time. This S might be due to an activity which is written as S decays per second. (in Bq) At a distance r, the particles pass through a sphere of radius r and area A = 4  r 2 Intensity is I = S/A, the number of particles, per unit time, per unit area. Then I = S/4  r 2 I decreases as the inverse square of the radius.

Intensity for r, 2r, 3r, etc. If the intensity is I 1 at a radius r 1, then if we double the radius to 2r 1, the intensity will be ¼ as much, because the area is now 2x2 = 4 times as much. More generally, if we compare the intensity at radii r 1 and r 2, then we get a ratio of intensities that depends on the square of the radii: I 2 / I 1 = (r 1 /r 2 ) 2 For example, if we compare radii of r and 3r, the intensities have a ratio of 1/9 = (1/3) 2

Linear plot for inverse square law. We can plot I vs. r on a linear graph, but this is not always useful if the range is too large. r I = 1/r 2 I (1) = 1 I (2) = 1/4 I (3) = 1/9 o o o

Linear plot for r -2 over range 1 to 100. not very useful !

Log-log plot for inverse square law. If the intensity is a function of radius that is a power law r m (for example, inverse square is a power law, since I = a. r m where m = -2), then, we can plot I vs. r on a log-log graph. Applying the logarithm to both sides of the equation: and using log(ab) = log(a) + log(b) log ( I ) = log(a. r m ) = log(a) + m. log(r) and if y = log( I ), x = log(r), and log(a) = b, we have the eq. of a straight line y = m. x + b

log-log plot of I = r y = log 10 ( I ) I r log 10 (r) = x 0 1 2

Analysis of I = r -2 How does this equation produce a straight line on the log-log plot? log( I ) = log( r -2 ) = log(10000) + log(r -2 ) = log(10 4 ) + (-2). log(r) Now define y = log(I) and x = log(r) and then y = m. x + b with b = log(10 4 ) = 4 (the intercept) m = -2 is the slope

We study this in laboratory # 10. We use laboratory equipment to study the distance dependence of the radiation from a small source. This is examined experimentally using log-log graph paper. We also examine the use of shielding materials, which requires semi-log paper to plot the absorption of gamma rays.

Absorption of X-rays and gamma rays X-rays and gamma rays can be very penetrating. Scattering of photons is not very important. It is more probable for the photon to be absorbed by an atom in the photoelectric effect. The photon is absorbed with some probability as it passes through a layer of material. This results in an exponential decrease in the intensity of the radiation (in addition to the inverse square law for distance dependence).

Exponential absorption of X-rays I = I o at detector, with no absorber

Exponential absorption of X-rays With absorber in place, I = I o exp(-  x)

Exponential absorption of X-rays The exponential decrease in the intensity of the radiation due to an absorber of thickness x has this form: I = I o exp(-  x) = I o e -  x where I o is the intensity without the absorber, I is the intensity with the absorber, and  is the linear absorption coefficient.  depends on material density and X-ray energy.

Graph of the exponential exp(x) exp(x) x exp(0) = 1 +

Graph of the exponential exp(-x) exp(-x) x + exp(-1) = 1/e = 0.37 exp(-0.693) = 0.5 = ½ + exp(0) = 1 +

Half-thickness for absorption of X-rays For a particular thickness x ½ the intensity is decreased to ½ of its original magnitude. So if I (x ½ ) = I o exp(-  x ½ ) = ½ I o we solve to find the half-thickness x ½. exp(-  x ½ ) = ½ and  x ½ = so x ½ = / 

Calculation of half-thickness To calculate x ½ (of lead, Pb) we need to know . As an example, for X-rays of energy 50 keV,  = 88 cm -1 and x ½ = 0.693/  so x ½ = / (88 cm -1 ) = cm But for hard X-rays with energy 433 keV,  = 2.2 cm -1 so x ½ = / (2.2 cm -1 ) = 0.31 cm

Graphs of linear attenuation coefficient  The linear attenuation coefficient  can be obtained from tables, or from automated databases such as the NIST database: which produced this graph for lead (Pb):

Tables of linear attenuation coefficient  The NIST database produces this table of  for lead (Pb): Data for Z = 82, E = keV E (keV )µ Total (cm -1 ) E E E E E E E E+04 … E E E E E E E E E E+01 … E E E E E E E E+00

Half-thickness data from ORTEC-online. (link)(link) X X Gamma rays from Co-60 X

Shielding of X-rays and gamma rays To reduce the intensity of radiation from a source, we can use an absorber in the path of the radiation. This is called shielding. To minimize I = I o exp(-  x) we want to increase  or x. Then the exponential will be smaller, and I will be smaller for constant I o. To increase the absorption coefficient  we need to increase the density of the shielding. To increase the value of x we must use thicker shielding.

Shielding of charged particles (alpha and beta particles) The absorption of charged particles is quite different from the absorption of X-rays (or  ). Charged particles lose kinetic energy continuously, instead of being absorbed in one single event like photons, and they also can scatter (change direction). The result is a range, a distance that only a small number of particles reach. Beyond the range, there is zero intensity.

Range of alpha and beta particles The range of alpha particles is a few centimeters in air and much less in solids. Alphas may be completely absorbed by a single sheet of paper or by your skin Beta particles can travel a few meters in air or a few millimeters in organic materials, depending on their kinetic energy. One cm of polymer will usually stop beta particles. However, they can easily pass through skin or gloves.