Skip to Content
OpenStax Logo
University Physics Volume 3

10.3 Radioactive Decay

University Physics Volume 310.3 Radioactive Decay
Buy book
  1. Preface
  2. Unit 1. Optics
    1. 1 The Nature of Light
      1. Introduction
      2. 1.1 The Propagation of Light
      3. 1.2 The Law of Reflection
      4. 1.3 Refraction
      5. 1.4 Total Internal Reflection
      6. 1.5 Dispersion
      7. 1.6 Huygens’s Principle
      8. 1.7 Polarization
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    2. 2 Geometric Optics and Image Formation
      1. Introduction
      2. 2.1 Images Formed by Plane Mirrors
      3. 2.2 Spherical Mirrors
      4. 2.3 Images Formed by Refraction
      5. 2.4 Thin Lenses
      6. 2.5 The Eye
      7. 2.6 The Camera
      8. 2.7 The Simple Magnifier
      9. 2.8 Microscopes and Telescopes
      10. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
    3. 3 Interference
      1. Introduction
      2. 3.1 Young's Double-Slit Interference
      3. 3.2 Mathematics of Interference
      4. 3.3 Multiple-Slit Interference
      5. 3.4 Interference in Thin Films
      6. 3.5 The Michelson Interferometer
      7. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    4. 4 Diffraction
      1. Introduction
      2. 4.1 Single-Slit Diffraction
      3. 4.2 Intensity in Single-Slit Diffraction
      4. 4.3 Double-Slit Diffraction
      5. 4.4 Diffraction Gratings
      6. 4.5 Circular Apertures and Resolution
      7. 4.6 X-Ray Diffraction
      8. 4.7 Holography
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
  3. Unit 2. Modern Physics
    1. 5 Relativity
      1. Introduction
      2. 5.1 Invariance of Physical Laws
      3. 5.2 Relativity of Simultaneity
      4. 5.3 Time Dilation
      5. 5.4 Length Contraction
      6. 5.5 The Lorentz Transformation
      7. 5.6 Relativistic Velocity Transformation
      8. 5.7 Doppler Effect for Light
      9. 5.8 Relativistic Momentum
      10. 5.9 Relativistic Energy
      11. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
    2. 6 Photons and Matter Waves
      1. Introduction
      2. 6.1 Blackbody Radiation
      3. 6.2 Photoelectric Effect
      4. 6.3 The Compton Effect
      5. 6.4 Bohr’s Model of the Hydrogen Atom
      6. 6.5 De Broglie’s Matter Waves
      7. 6.6 Wave-Particle Duality
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
    3. 7 Quantum Mechanics
      1. Introduction
      2. 7.1 Wave Functions
      3. 7.2 The Heisenberg Uncertainty Principle
      4. 7.3 The Schrӧdinger Equation
      5. 7.4 The Quantum Particle in a Box
      6. 7.5 The Quantum Harmonic Oscillator
      7. 7.6 The Quantum Tunneling of Particles through Potential Barriers
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    4. 8 Atomic Structure
      1. Introduction
      2. 8.1 The Hydrogen Atom
      3. 8.2 Orbital Magnetic Dipole Moment of the Electron
      4. 8.3 Electron Spin
      5. 8.4 The Exclusion Principle and the Periodic Table
      6. 8.5 Atomic Spectra and X-rays
      7. 8.6 Lasers
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
    5. 9 Condensed Matter Physics
      1. Introduction
      2. 9.1 Types of Molecular Bonds
      3. 9.2 Molecular Spectra
      4. 9.3 Bonding in Crystalline Solids
      5. 9.4 Free Electron Model of Metals
      6. 9.5 Band Theory of Solids
      7. 9.6 Semiconductors and Doping
      8. 9.7 Semiconductor Devices
      9. 9.8 Superconductivity
      10. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    6. 10 Nuclear Physics
      1. Introduction
      2. 10.1 Properties of Nuclei
      3. 10.2 Nuclear Binding Energy
      4. 10.3 Radioactive Decay
      5. 10.4 Nuclear Reactions
      6. 10.5 Fission
      7. 10.6 Nuclear Fusion
      8. 10.7 Medical Applications and Biological Effects of Nuclear Radiation
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    7. 11 Particle Physics and Cosmology
      1. Introduction
      2. 11.1 Introduction to Particle Physics
      3. 11.2 Particle Conservation Laws
      4. 11.3 Quarks
      5. 11.4 Particle Accelerators and Detectors
      6. 11.5 The Standard Model
      7. 11.6 The Big Bang
      8. 11.7 Evolution of the Early Universe
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
  4. A | Units
  5. B | Conversion Factors
  6. C | Fundamental Constants
  7. D | Astronomical Data
  8. E | Mathematical Formulas
  9. F | Chemistry
  10. G | The Greek Alphabet
  11. Answer Key
    1. Chapter 1
    2. Chapter 2
    3. Chapter 3
    4. Chapter 4
    5. Chapter 5
    6. Chapter 6
    7. Chapter 7
    8. Chapter 8
    9. Chapter 9
    10. Chapter 10
    11. Chapter 11
  12. Index

Learning Objectives

By the end of this section, you will be able to:
  • Describe the decay of a radioactive substance in terms of its decay constant and half-life
  • Use the radioactive decay law to estimate the age of a substance
  • Explain the natural processes that allow the dating of living tissue using 14C14C

In 1896, Antoine Becquerel discovered that a uranium-rich rock emits invisible rays that can darken a photographic plate in an enclosed container. Scientists offer three arguments for the nuclear origin of these rays. First, the effects of the radiation do not vary with chemical state; that is, whether the emitting material is in the form of an element or compound. Second, the radiation does not vary with changes in temperature or pressure—both factors that in sufficient degree can affect electrons in an atom. Third, the very large energy of the invisible rays (up to hundreds of eV) is not consistent with atomic electron transitions (only a few eV). Today, this radiation is explained by the conversion of mass into energy deep within the nucleus of an atom. The spontaneous emission of radiation from nuclei is called nuclear radioactivity (Figure 10.8).

A yellow triangle with a black outline, enclosing a fan shaped structure is shown. The “fan” is black and has three blades.
Figure 10.8 The international ionizing radiation symbol is universally recognized as the warning symbol for nuclear radiation.

Radioactive Decay Law

When an individual nucleus transforms into another with the emission of radiation, the nucleus is said to decay. Radioactive decay occurs for all nuclei with Z>82,Z>82, and also for some unstable isotopes with Z<83.Z<83. The decay rate is proportional to the number of original (undecayed) nuclei N in a substance. The number of nuclei lost to decay, dNdN in time interval dt, is written

dNdt=λNdNdt=λN
(10.7)

where λλ is called the decay constant. (The minus sign indicates the number of original nuclei decreases over time.) In other words, the more nuclei available to decay, the more that do decay (in time dt). This equation can be rewritten as

dNN=λdt.dNN=λdt.
(10.8)

Integrating both sides of the equation, and defining N0N0 to be the number of nuclei at t=0t=0, we obtain

N0NdNN=0tλdt.N0NdNN=0tλdt.
(10.9)

This gives us

lnNN0=λt.lnNN0=λt.
(10.10)

Taking the left and right sides of the equation as a power of e, we have the radioactive decay law.

Radioactive Decay Law

The total number N of radioactive nuclei remaining after time t is

N=N0eλtN=N0eλt
(10.11)

where λλ is the decay constant for the particular nucleus.

The total number of nuclei drops very rapidly at first, and then more slowly (Figure 10.9).

A graph of N versus t is shown. It is labeled N equal to N subscript 0 e to the power minus lambda t. The value of N is maximum, N subscript 0, at t =0 and it reduces with time till it reaches 0. At t = T subscript half, N = N subscript 0 by 2 and at t = 2T subscript half, N = N subscript 0 by 4.
Figure 10.9 A plot of the radioactive decay law demonstrates that the number of nuclei remaining in a decay sample drops dramatically during the first moments of decay.

The half-life (T1/2)(T1/2) of a radioactive substance is defined as the time for half of the original nuclei to decay (or the time at which half of the original nuclei remain). The half-lives of unstable isotopes are shown in the chart of nuclides in Figure 10.4. The number of radioactive nuclei remaining after an integer (n) number of half-lives is therefore

N=N02nN=N02n
(10.12)

If the decay constant (λλ) is large, the half-life is small, and vice versa. To determine the relationship between these quantities, note that when t=T1/2t=T1/2, then N=N0/2N=N0/2. Thus, Equation 10.10 can be rewritten as

N02=N0eλT1/2.N02=N0eλT1/2.
(10.13)

Dividing both sides by N0N0 and taking the natural logarithm yields

ln12=lneλT1/2ln12=lneλT1/2
(10.14)

which reduces to

λ=0.693T1/2.λ=0.693T1/2.
(10.15)

Thus, if we know the half-life T1/2 of a radioactive substance, we can find its decay constant. The lifetime TT of a radioactive substance is defined as the average amount of time that a nucleus exists before decaying. The lifetime of a substance is just the reciprocal of the decay constant, written as

T=1λ.T=1λ.
(10.16)

The activity A is defined as the magnitude of the decay rate, or

A=dNdt=λN=λN0eλt.A=dNdt=λN=λN0eλt.
(10.17)

The infinitesimal change dN in the time interval dt is negative because the number of parent (undecayed) particles is decreasing, so the activity (A) is positive. Defining the initial activity as A0=λN0A0=λN0, we have

A=A0eλt.A=A0eλt.
(10.18)

Thus, the activity A of a radioactive substance decreases exponentially with time (Figure 10.10).

Figure a shows a graph of A versus t. It starts at point A subscript 0 and reduces with time. The rate of reduction decreases slowly till A is very close to 0, making a curved plot on the graph. The plot is labeled A = A subscript 0 e to the power minus lambda t. Figure b shows a graph of ln A versus t. It starts at ln A subscript 0 and slopes downwards in a straight line. The slope of the line is labeled minus lambda t.
Figure 10.10 (a) A plot of the activity as a function of time (b) If we measure the activity at different times, we can plot ln A versus t, and obtain a straight line.

Example 10.4

Decay Constant and Activity of Strontium-90 The half-life of strontium-90, 3890Sr3890Sr, is 28.8 y. Find (a) its decay constant and (b) the initial activity of 1.00 g of the material.

Strategy We can find the decay constant directly from Equation 10.15. To determine the activity, we first need to find the number of nuclei present.

Solution

  1. The decay constant is found to be
    λ=0.693T1/2=(0.693T1/2)(1yr3.16×107s)=7.61×10−10s1.λ=0.693T1/2=(0.693T1/2)(1yr3.16×107s)=7.61×10−10s1.
  2. The atomic mass of 3890Sr3890Sr is 89.91 g. Using Avogadro’s number NA=6.022×1023NA=6.022×1023 atoms/mol, we find the initial number of nuclei in 1.00 g of the material:
    N0=1.00g89.91g(NA)=6.70×1021nuclei.N0=1.00g89.91g(NA)=6.70×1021nuclei.

    From this, we find that the activity A0A0 at t=0t=0 for 1.00 g of strontium-90 is
    A0=λN0=(7.61×10−10s−1)(6.70×1021nuclei)=5.10×1012decays/s.A0=λN0=(7.61×10−10s−1)(6.70×1021nuclei)=5.10×1012decays/s.

Expressing λλ in terms of the half-life of the substance, we get

A=A0e(0.693/T1/2)T1/2=A0e−0.693=A0/2.A=A0e(0.693/T1/2)T1/2=A0e−0.693=A0/2.
(10.19)

Therefore, the activity is halved after one half-life. We can determine the decay constant λλ by measuring the activity as a function of time. Taking the natural logarithm of the left and right sides of Equation 10.17, we get

lnA=λt+lnA0.lnA=λt+lnA0.
(10.20)

This equation follows the linear form y=mx+by=mx+b. If we plot ln A versus t, we expect a straight line with slope λλ and y-intercept lnA0lnA0 (Figure 10.10(b)). Activity A is expressed in units of becquerels (Bq), where one 1Bq=1decay per second1Bq=1decay per second. This quantity can also be expressed in decays per minute or decays per year. One of the most common units for activity is the curie (Ci), defined to be the activity of 1 g of 226Ra226Ra. The relationship between the Bq and Ci is

1Ci=3.70×1010Bq.1Ci=3.70×1010Bq.

Example 10.5

What is 14C14C Activity in Living Tissue? Approximately 20%20% of the human body by mass is carbon. Calculate the activity due to 14C14C in 1.00 kg of carbon found in a living organism. Express the activity in units of Bq and Ci.

Strategy The activity of 14C14C is determined using the equation A0=λN0A0=λN0, where λ is the decay constant and N0N0 is the number of radioactive nuclei. The number of 14C14C nuclei in a 1.00-kg sample is determined in two steps. First, we determine the number of 12C12C nuclei using the concept of a mole. Second, we multiply this value by 1.3×10−121.3×10−12 (the known abundance of 14C14C in a carbon sample from a living organism) to determine the number of 14C14C nuclei in a living organism. The decay constant is determined from the known half-life of 14C14C (available from Figure 10.4).

Solution One mole of carbon has a mass of 12.0 g, since it is nearly pure 12C12C. Thus, the number of carbon nuclei in a kilogram is

N(12C)=6.02×1023mol−112.0g/mol×(1000g)=5.02×1025.N(12C)=6.02×1023mol−112.0g/mol×(1000g)=5.02×1025.

The number of 14C14C nuclei in 1 kg of carbon is therefore

N(14C)=(5.02×1025)(1.3×10−12)=6.52×1013.N(14C)=(5.02×1025)(1.3×10−12)=6.52×1013.

Now we can find the activity A by using the equation A=0.693Nt1/2.A=0.693Nt1/2. Entering known values gives us

A=0.693(6.52×1013)5730y=7.89×109y1A=0.693(6.52×1013)5730y=7.89×109y1

or 7.89×1097.89×109 decays per year. To convert this to the unit Bq, we simply convert years to seconds. Thus,

A=(7.89×109y1)1.00y3.16×107s=250Bq,A=(7.89×109y1)1.00y3.16×107s=250Bq,

or 250 decays per second. To express A in curies, we use the definition of a curie,

A=250Bq3.7×1010Bq/Ci=6.76×10−9Ci.A=250Bq3.7×1010Bq/Ci=6.76×10−9Ci.

Thus,

A=6.76nCi.A=6.76nCi.

Significance Approximately 20%20% of the human body by weight is carbon. Hundreds of 14C14C decays take place in the human body every second. Carbon-14 and other naturally occurring radioactive substances in the body compose a person’s background exposure to nuclear radiation. As we will see later in this chapter, this activity level is well below the maximum recommended dosages.

Radioactive Dating

Radioactive dating is a technique that uses naturally occurring radioactivity to determine the age of a material, such as a rock or an ancient artifact. The basic approach is to estimate the original number of nuclei in a material and the present number of nuclei in the material (after decay), and then use the known value of the decay constant λλ and Equation 10.10 to calculate the total time of the decay, t.

An important method of radioactive dating is carbon-14 dating. Carbon-14 nuclei are produced when high-energy solar radiation strikes 14N14N nuclei in the upper atmosphere and subsequently decay with a half-life of 5730 years. Radioactive carbon has the same chemistry as stable carbon, so it combines with the ecosphere and eventually becomes part of every living organism. Carbon-14 has an abundance of 1.3 parts per trillion of normal carbon. Therefore, if you know the number of carbon nuclei in an object, you multiply that number by 1.3×10−121.3×10−12 to find the number of 14C14C nuclei in that object. When an organism dies, carbon exchange with the environment ceases, and 14C14C is not replenished as it decays.

By comparing the abundance of 14C14C in an artifact, such as mummy wrappings, with the normal abundance in living tissue, it is possible to determine the mummy’s age (or the time since the person’s death). Carbon-14 dating can be used for biological tissues as old as 50,000 years, but is generally most accurate for younger samples, since the abundance of 14C14C nuclei in them is greater. Very old biological materials contain no 14C14C at all. The validity of carbon dating can be checked by other means, such as by historical knowledge or by tree-ring counting.

Example 10.6

An Ancient Burial Cave In an ancient burial cave, your team of archaeologists discovers ancient wood furniture. Only 80%80% of the original 14C14C remains in the wood. How old is the furniture?

Strategy The problem statement implies that N/N0=0.80.N/N0=0.80. Therefore, the equation N=N0eλtN=N0eλt can be used to find the product, λtλt. We know the half-life of 14C14C is 5730 y, so we also know the decay constant, and therefore the total decay time t.

Solution Solving the equation N=N0eλtN=N0eλt for N/N0N/N0 gives us

NN0=eλt.NN0=eλt.

Thus,

0.80=eλt.0.80=eλt.

Taking the natural logarithm of both sides of the equation yields

ln0.80=λt,ln0.80=λt,

so that

−0.223=λt.−0.223=λt.

Rearranging the equation to isolate t gives us

t=0.223λ,t=0.223λ,

where

λ=0.693t1/2=0.6935730y.λ=0.693t1/2=0.6935730y.

Combining this information yields

t=0.223(0.6935730y)=1844y.t=0.223(0.6935730y)=1844y.

Significance The furniture is almost 2000 years old—an impressive discovery. The typical uncertainty on carbon-14 dating is about 5%5%, so the furniture is anywhere between 1750 and 1950 years old. This date range must be confirmed by other evidence, such as historical records.

Check Your Understanding 10.3

A radioactive nuclide has a high decay rate. What does this mean for its half-life and activity?

Interactive

Visit the Radioactive Dating Game to learn about the types of radiometric dating and try your hand at dating some ancient objects.

Citation/Attribution

Want to cite, share, or modify this book? This book is Creative Commons Attribution License 4.0 and you must attribute OpenStax.

Attribution information
  • If you are redistributing all or part of this book in a print format, then you must include on every physical page the following attribution:
    Access for free at https://openstax.org/books/university-physics-volume-3/pages/1-introduction
  • If you are redistributing all or part of this book in a digital format, then you must include on every digital page view the following attribution:
    Access for free at https://openstax.org/books/university-physics-volume-3/pages/1-introduction
Citation information

© Sep 29, 2016 OpenStax. Textbook content produced by OpenStax is licensed under a Creative Commons Attribution License 4.0 license. The OpenStax name, OpenStax logo, OpenStax book covers, OpenStax CNX name, and OpenStax CNX logo are not subject to the Creative Commons license and may not be reproduced without the prior and express written consent of Rice University.