Nuclear Chemistry AP Chemistry Lecture Outline

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Nuclear Chemistry AP Chemistry Lecture Outline Name: involve changes with electrons. involve changes in atomic nuclei. Spontaneously-changing nuclei emit and are said to be. Radioactivity nucleons: mass number: isotopes: atoms having the same number of p +, but different numbers of n 0 -- radioactive ones are called nuclide: a nucleus with a specified number of p + and n 0 -- radioactive ones are called these are unstable and emit radiation atomic number: Radioactive Decay For nuclear equations, mass (top) and charge (bottom) must balance. alpha ( ) decay: beta ( ) decay: -particle (i.e., a He nucleus): massive, slow-moving; stopped by skin -particle (i.e., a fast-moving electron): little mass; stops ~1 cm into body In -decay, the effect is that a n 0 is converted into a p +, ejecting an e from the nucleus. 1

NOTE: There are no e in the nucleus. The ejected e is formed when energy released from the nucleus congeals into mass, via E = mc 2. gamma radiation: -- can penetrate to internal organs -- gamma ray: emitted when nucleons rearrange into a more stable configuration -- gamma radiation often accompanies other nuclear decays positron decay: electron capture: nucleus captures orbiting e positron: identical to an e, but (+) The effect of positron decay and electron capture is to turn a p + into a n 0. Nuclear Stability Nucleons are held together by the. ~1.5 n 0 : 1 p + # of n 0 Band (or Belt) of Stability ~1 n 0 : 1 p + 0 83 Z (i.e., # of p + ) At Z > 83, none are stable (i.e., all are radioactive) 2

Nuclei that have too many and stabilize by are above belt are below belt have Z > 83 Examples: A radioactive series is the sequence a radionuclide goes through to become stable. e.g., -- there are three basic series, ending with Also, nuclei having magic numbers of p + or n 0 tend to be more stable than those that don t. p + : n 0 : The shell model of the nucleus, which says that the nucleons reside in shells, has been proposed to explain these observations. This theory is similar to how e reside in shells. Finally, nuclides with an even number of p + AND an even number of n 0 tend to be stable. 3

Nuclear Transmutations These are induced by a bombarding particle, and are typically written in the following order: target bombarding product ejected nucleus particle nucleus particle This reaction is abbreviated EX. Write the shorthand for 27 13 Al 1 0 n 24 11 Na 4 2 He EX. Write the equation for 16 8 O (p, ) 13 7 N Particle accelerators are used to accelerate charged particles (e.g., ). We cannot accelerate neutrons, but we can use n 0 -emitters to produce artificial isotopes. Often, -emission follows n 0 absorption. For example: First then and then Rates of Radioactive Decay Each radioisotope has a unique rate of decay, its half-life, t 1/2, which is the time required for half of a sample of a radioisotope to decay into something stable. An isotope s half-life is: (1) independent of T, P, and its state of chemical combination (2) useful in radioactive dating. 4

Radioactive decay is a first-order kinetic process. Recall the first-order rate law: By setting N t = ½ N o and integrating, we get EX. F-18 has a half-life of 110 minutes. What % is present after 300 minutes? EX. Molybdenum-99 has a half-life of 67.0 hours. How much of a 1.000 mg sample of Mo-99 is left after 16.0 days? Detection of Radioactivity photographic film (film badges): cheap, ballpark qualitative Geiger counter: ionization of gas produces measurable electric current scintillation counter: radiation causes phosphors to glow; flashes counted electronically radiotracer: radioisotopes that are monitored during chemical reactions -- all isotopes of an element behave the same, chemically 5

Energy Changes in Nuclear Reactions Energy and mass are two sides of the same coin. When a system loses/gains energy, it loses/gains mass. In chemical reactions, this mass change is nearly undetectable, so we speak of mass as being conserved, when it really isn t. The amount of mass-and-energy-together, however, IS conserved. Mass changes in nuclear reactions are much larger. Nuclear Binding Energy mass of nucleus mass of individual nucleons in nucleus rest masses: n 0 = 1.00866 amu = 1.67493 x 10 24 g p + = 1.00728 amu = 1.67262 x 10 24 g mass defect = EX. A plutonium-232 nucleus has mass 3.85285 x 10 22 g. Calculate its mass defect, in g. Use mass defect, E = mc 2, and # of nucleons to calculate binding energy per nucleon (BE/n). -- large BE/n means great nuclear stability -- BE/n is largest for Fe-56, meaning that (1) larger nuclei decay OR can undergo fission (2) smaller nuclei can undergo fusion 6

EX. Calculate the binding energy per nucleon of N-14, which has a nuclear mass of SOLN: 13.999234 amu. mass defect = convert to kg X kg = Nuclear Fission Fission requires Important fissionable nuclei: chain reaction: one nuclear reaction leads to one or more others critical mass: the mass of fissionable material required to maintain a chain reaction at a constant rate supercritical mass: the mass above which the chain reaction accelerates Nuclear Reactors -- fuel is -- control rods of B or Cd -- moderator: -- water is heated to steam, which spins electrical-generating turbines Main benefits: (1) (2) (3) breeder reactors: reactors that generate new fissionable material at a greater rate than the original fuel is consumed -- non-fissionable U-238 is transmuted into fissionable Pu-239 Main problem: 7

Nuclear Fusion -- also called thermonuclear reactions -- products are generally NOT radioactive -- requires high temperatures -- the tokamak uses magnetic fields to contain and heat the reaction Biological Effects of Radiation nonionizing radiation: bumps e to higher energy levels or heats molecules; ionizing radition: knocks e out of molecules; -- e.g., -- sequence of action in living tissue (1) (2) -- the tissues most damaged by radiation are the ones with cells that rapidly reproduce: -- low doses over a long time can induce cancer, which is Units for Radiation Doses 1 bequerel (Bq) = 1 disintegration/sec 1 gray (Gy) = absorbing 1 J/kg of tissue 1 Curie (Ci) = 3.7 x 10 10 disintegrations/sec 1 rad = absorbing 1 x 10 2 J/kg of tissue Since the various types of radiation damage tissue with various degrees of efficiency, each type has its own relative biological effectiveness (RBE). Radon -- an -emitter from the decay of radium in rocks and soil -- very dense, seeps into basements, and is readily inhaled -- estimated to be responsible for of U.S. lung cancer deaths 8