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Chapter 29

Chapter 29. Nuclear Physics. Properties of Nuclei. All nuclei are composed of protons and neutrons (exception: ordinary hydrogen) The atomic number , Z, equals the number of protons in the nucleus The neutron number , N, is the number of neutrons in the nucleus

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Chapter 29

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  1. Chapter 29 Nuclear Physics

  2. Properties of Nuclei • All nuclei are composed of protons and neutrons (exception: ordinary hydrogen) • The atomic number, Z, equals the number of protons in the nucleus • The neutron number, N, is the number of neutrons in the nucleus • The mass number (not the same as the mass), A, is the number of nucleons in the nucleus: A = Z + N • Nucleon is a generic term used to refer to either a proton or a neutron

  3. Properties of Nuclei • Symbol: • X is the chemical symbol of the element • Example: • Mass number is 27; atomic number is 13; contains 13 protons and 14 = 27 – 13 neutrons • The Z may be omitted since the element can be used to determine Z • The nuclei of all atoms of a particular element must contain the same number of protons

  4. Properties of Nuclei • The nuclei may contain varying numbers of neutrons • Isotopes of an element have the same Z but differing N and A values. For example: • The proton has a single positive charge, +e (e = 1.602 177 33 x 10-19 C) • The electron has a single negative charge, -e • The neutron has no charge, which makes it difficult to detect

  5. Mass • It is convenient to express masses using unified mass units, u, based on definition that the mass of one atom of C-12 is exactly 12 u: 1 u = 1.660 559 x 10-27 kg • Mass can also be expressed in MeV/c2 (from E = m c2) 1 u = 931.494 MeV/c2

  6. The Size of the Nucleus • From scattering experiments, Rutherford found an expression for how close an alpha particle moving toward the nucleus can come before being turned around by the Coulomb force • The KE of the particle must be completely converted to PE • d gives an upper limit for the size of the nucleus (e.g., for gold, d = 3.2 x 10-14 m and for silver, d = 2 x 10-14 m)

  7. Enrico Fermi 1901 – 1954 The Size of the Nucleus • Such small lengths are often expressed in femtometers where 1 fm = 10-15 m Also called a fermi • Since the time of Rutherford, many other experiments have concluded that most nuclei are approximately spherical with the average radius of • ro = 1.2 x 10-15 m

  8. Density of Nuclei • The volume of the nucleus (assumed to be spherical) is directly proportional to the total number of nucleons • This suggests that all nuclei have nearly the same density • Nucleons combine to form a nucleus as though they were tightly packed spheres

  9. Nuclear Stability • There are very large repulsive electrostatic forces between protons • These forces should cause the nucleus to fly apart • The nuclei are stable because of the presence of another, short-range force, called the nuclear force • This is an attractive force that acts between all nuclear particles • The nuclear attractive force is stronger than the Coulomb repulsive force at the short ranges within the nucleus

  10. Nuclear Stability • Light nuclei are most stable if N = Z • Heavy nuclei are most stable when N > Z • As the number of protons increase, the Coulomb force increases and so more nucleons are needed to keep the nucleus stable • No nuclei are stable when Z > 83

  11. Chapter 29Problem 7 (a) Find the speed an alpha particle requires to come within 3.2 × 10−14 m of a gold nucleus. (b) Find the energy of the alpha particle in MeV.

  12. Binding Energy • The total energy of the bound system (the nucleus) is less than the combined energy of the separated nucleons • This difference in energy is called the binding energy of the nucleus • It can be thought of as the amount of energy you need to add to the nucleus to break it apart into separated protons and neutrons

  13. Binding Energy

  14. Binding Energy • Except for light nuclei, the binding energy is about 8 MeV per nucleon • The curve peaks in the vicinity of A = 60 • Nuclei with mass numbers greater than or less than 60 are not as strongly bound as those near the middle of the periodic table • The curve is slowly varying at A > 40, suggesting that the nuclear force saturates • A particular nucleon can interact with only a limited number of other nucleons

  15. Radioactivity • Radioactivity is the spontaneous emission of radiation • Radioactivity is the result of the decay (disintegration) of unstable nuclei • Three types of radiation can be emitted • 1) Alpha particles: 4He nuclei) • 2) Beta particles: either electrons or positrons (a positron is the antiparticle of the electron, similar to the electron except its charge is +e) • 3) Gamma rays: high energy photons

  16. Distinguishing Types of Radiation • A radioactive beam is directed into a region with a magnetic field • The gamma particles carry no charge and they are not deflected • The alpha particles are deflected upward • The beta particles (electrons) are deflected downward, whereas the positrons would be deflected upward

  17. Penetrating Ability of Particles • Alpha particles: barely penetrate a piece of paper • Beta particles: can penetrate a few mm of aluminum • Gamma rays: can penetrate several cm of lead

  18. The Decay Constant • The number of particles that decay in a given time is proportional to the total number of particles in a radioactive sample ΔN = - λ N Δt • λ: the decay constant; determines the rate at which the material will decay • The decay rate or activity, R, of a sample is defined as the number of decays per second

  19. Decay Curve • The decay curve follows the equation N = No e- λt • Another useful parameter is the half-life defined as the time it takes for half of any given number of radioactive nuclei to decay

  20. Decay Curve

  21. Antoine Henri Becquerel 1852 – 1908 Maria Skłodowska-Curie 1867 – 1934 Units • The unit of activity, R, is the Curie, Ci: 1 Ci = 3.7 x 1010 decays/second • The most commonly used units of activity are the mCi and the µCi • The SI unit of activity is the Becquerel, Bq: 1 Bq = 1 decay/second (therefore, 1 Ci = 3.7 x 1010 Bq)

  22. Chapter 29Problem 24 A building has become accidentally contaminated with radioactivity. The longest-lived material in the building is strontium-90. (The atomic mass of is 89.907 7.) If the building initially contained 5.0 kg of this substance, and the safe level is less than 10.0 counts/min, how long will the building be unsafe?

  23. Decay – General Rules • When one element changes into another element, the process is called spontaneous decay or transmutation • The sum of the mass numbers, A, must be the same on both sides of the equation • The sum of the atomic numbers, Z, must be the same on both sides of the equation • Conservation of mass-energy and conservation of momentum must hold

  24. Alpha Decay • When a nucleus emits an alpha particle it loses two protons and two neutrons (N decreases by 2; Z decreases by 2; A decreases by 4) • Symbolically • X: parent nucleus; Y: daughter nucleus • Example: decay of 226 Ra (half life is 1600 years) • Excess mass is converted into kinetic energy • Momentum of the two particles is equal and opposite

  25. Beta Decay • During beta decay, the daughter nucleus has the same number of nucleons as the parent, but the atomic number is changed by one • Symbolically: • The emission of the electron is from the nucleus, which contains protons and neutrons • The process occurs when a neutron is transformed into a proton and an electron • The energy must be conserved: the energy released in the decay process should almost all go to kinetic energy of the electron (KEmax)

  26. Beta Decay • Experiments showed that few electrons had this amount of kinetic energy • To account for this “missing” energy, Pauli proposed the existence of another particle, which Fermi later named the neutrino • Properties of the neutrino: • Zero electrical charge • Mass much smaller than the electron, probably not zero • Spin of ½ • Very weak interaction with matter

  27. Beta Decay • Symbolically •  is the symbol for the neutrino; is the symbol for the antineutrino • Therefore, in beta decay, the following pairs of particles are emitted: either an electron and an antineutrino or a positron and a neutrino

  28. Gamma Decay • Gamma rays are given off when an excited nucleus “falls” to a lower energy state (similar to the process of electron “jumps” to lower energy states and giving off photons) • The gamma ray photons are very high in energy relative to light • The excited nuclear states result from “jumps” made by a proton or neutron • The excited nuclear states may be the result of violent collision or more likely of an alpha or beta emission

  29. Gamma Decay • Example of a decay sequence • The first decay is a beta emission • The second step is a gamma emission • The C* indicates the Carbon nucleus is in an excited state • Gamma emission doesn’t change either A or Z

  30. Natural Radioactivity • There are unstable nuclei found in nature, which give rise to natural radioactivity • Nuclei produced in the laboratory through nuclear reactions exhibit artificial radioactivity • Three series of natural radioactivity exist (see table 29.2): 1) Uranium 2) Actinium 3) Thorium (processes through a series of alpha and beta decays and ends with a stable isotope of lead, 208Pb)

  31. Nuclear Reactions • Structure of nuclei can be changed by bombarding them with energetic particles • These changes are called nuclear reactions • As with nuclear decays, the atomic numbers and mass numbers must balance on both sides of the equation • E.g., alpha particle colliding with nitrogen: • Balancing the equation allows for the identification of X, so the reaction is

  32. Chapter 29Problem 39 Identify the unknown particles X and X’ in the following nuclear reactions:

  33. Answers to Even Numbered Problems Chapter 28: Problem 4 ρn/ρa = 8.6 × 1013

  34. Answers to Even Numbered Problems • Chapter 28: • Problem 8 • 1.9 × 10-15 m • 7.4 × 10-15 m

  35. Answers to Even Numbered Problems • Chapter 28: • Problem 10 • 1.11 MeV/nucleon • 7.07 MeV/nucleon • (c) 8.79 MeV/nucleon • (d) 7.57 MeV/nucleon

  36. Answers to Even Numbered Problems • Chapter 28: • Problem 18 • 8.06 d • (b) It is probably 13153I

  37. Answers to Even Numbered Problems Chapter 28: Problem 20 2.29 g

  38. Answers to Even Numbered Problems Chapter 28: Problem 38 42He, 42He

  39. Answers to Even Numbered Problems • Chapter 28: • Problem 42 • 105B • –2.79 MeV

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