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Radioactivity inverse square law, absorption, and rates

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Suppose that S is the number of particles emitted by the source per unit time. ... The result is a range, a distance that only a small number of particles reach. ... – PowerPoint PPT presentation

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Title: Radioactivity inverse square law, absorption, and rates


1
Radioactivity inverse square law, absorption,
and rates
  • presentation for Apr. 30, 2008 by
  • Dr. Brian Davies, WIU Physics Dept.

2
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 4pr2
  • Therefore, the number per unit area per unit time
    depends on the radius.

3
Inverse square law

4
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 4pr2
  • Intensity is I S/A, the number of particles,
    per unit time, per unit area.
  • Then I S/4pr2
  • I decreases as the inverse square of the radius.

5
Intensity for r, 2r, 3r, etc.
  • If the intensity is I1 at a radius r1, then if we
    double the radius to 2r1, 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 r1 and r2, then we get a ratio of
    intensities that depends on the square of the
    radii
  • I2 / I1 (r1/r2)2
  • For example, if we compare radii of r and 3r, the
    intensities have a ratio of 1/9 (1/3)2

6
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.

I 1/r2
I(1) 1
o
I(2) 1/4
I(3) 1/9
o
o
r
7
Linear plot for 10000.r -2 over range 1 to 100.
not very useful !
8
Log-log plot for inverse square law.
  • If the intensity is a function of radius that is
    a power law rm (for example, inverse square is a
    power law, since I a.rm 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.rm) 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

9
log-log plot of I 10000 r -2
y log10(I)
I
4 3 2 1 0
r
0 1 2
log10(r) x
10
Analysis of I 10000 r -2
How does this equation produce a straight line
on the log-log plot? log(I)
log(10000.r-2) log(10000) log(r-2)
log(104) (-2).log(r) Now define y
log(I) and x log(r) and then y m.x
b with b log(104) 4 (the
intercept) m -2 is the slope
11
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.
12
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).

13
Exponential absorption of X-rays
  • I Io at detector, with no absorber

14
Exponential absorption of X-rays
  • With absorber in place, I Io exp(- m x)

15
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 Io exp(- m x) Io e - m x
  • where Io is the intensity without the absorber,
  • I is the intensity with the absorber, and
  • m is the linear absorption coefficient.
  • m depends on material density and X-ray energy.

16
Graph of the exponential exp(x)
  • exp(x)

exp(0) 1

x
17
Graph of the exponential exp(-x)

exp(0) 1
exp(-0.693) 0.5 ½
  • exp(-x)


exp(-1) 1/e 0.37
x
18
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(x½) Io exp(- m x ½) ½ Io
  • we solve to find the half-thickness x ½.
  • exp(- m x ½) ½ and m x ½ 0.693
  • so x ½ 0.693 / m

19
Calculation of half-thickness
  • To calculate x ½ (of lead, Pb) we need to know
    m.
  • As an example, for X-rays of energy 50 keV,
  • m 88 cm-1 and x ½ 0.693/m
    so
  • x ½ 0.693 / (88 cm-1) 0.0079 cm
  • But for hard X-rays with energy 433 keV,
  • m 2.2 cm-1 so
  • x ½ 0.693 / (2.2 cm-1) 0.31 cm

20
Graphs of linear attenuation coefficient m
  • The linear attenuation coefficient m can be
    obtained from tables, or from automated databases
    such as the NIST database
  • http//physics.nist.gov/PhysRefData/FFast/Text/c
    over.html

which produced this graph for lead (Pb)
21
Tables of linear attenuation coefficient m

Data for Z 82, E 2 - 433 keV E (keV ) µ
Total (cm-1) 2.0004844E00 1.3412E04
2.0104868E00 1.3272E04 2.0205393E00
1.3133E04 2.0306420E00 1.2996E04
4.479101E01 1.1677E02 4.788159E01
9.8248E01 5.118542E01 8.2776E01 5.471721E01
6.9836E01 5.849270E01 5.8933E01
3.544049E02 3.1633E00 3.788588E02
2.7826E00 4.050001E02 2.4588E00 4.329451E02
2.1827E00
The NIST database produces this table of m for
lead (Pb)
22
Half-thickness data from ORTEC-online. (link)
X
Gamma rays from Co-60
X
X
23
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 Io exp(- m x) we want to
    increase m or x. Then the exponential will be
    smaller, and I will be smaller for constant Io .
  • To increase the absorption coefficient m we need
    to increase the density of the shielding.
  • To increase the value of x we must use thicker
    shielding.

24
Shielding of charged particles (alpha and beta
particles)
  • The absorption of charged particles is quite
    different from the absorption of X-rays (or g).
  • 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.

25
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.
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