1 / 32

Nuclear Reactions

Nuclear Reactions. Natural Transmutation. 1 term on reactant side o riginal isotope (naturally radioactive) 2 terms on product side e mitted p article n ew Isotope. Happens all by itself (spontaneous) Not affected by anything in environment. Natural Transmutation.

rfortin
Download Presentation

Nuclear Reactions

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Nuclear Reactions

  2. Natural Transmutation 1 term on reactant side original isotope (naturally radioactive) 2 terms on product side emitted particle new Isotope Happens all by itself(spontaneous) Not affected by anything in environment

  3. Natural Transmutation 16N 0e + 16O 8 -1 7 2 terms on product side 1 term on reactant side

  4. Artificial Transmutation cause to happen: smash particles into one another 2 terms on reactant side original Isotope (non-radioactive) particle that hits it neutron, proton, or -particle product side: usually 2 terms

  5. Artificial Transmutation 27Al + 4He  30P + 1n 15 0 “bullet” - thing hits isotope 13 2 original isotope or target nucleus

  6. Artificial Transmutation 27Al + 4He 30P + 1n 2 15 0 13 1 2 8 7 2 35 0 33 0 17 all these equations have2 reactants! 14N + 4He 17O + 1H 75As + 4He 78Br + 1n 37Cl + 1n 38Cl 17

  7. Bombarding with protons or  protons & -particles have positive charge and mass do some damage when hit target nucleus must be accelerated to high speeds to overcome repulsive forces between nucleus & particle (both are +)

  8. What is an accelerator? vacuum chamber (usually long pipe) surrounded by vacuum pumps, magnets, radio-frequency cavities, high voltage instruments & electronic circuits inside pipe particles are accelerated to very high speeds then smashed into each other

  9. FissionReaction • splitting heavy nucleus into 2 lighter nuclei • requires critical mass of fissionable isotope • controlled: nuclear reactor • uncontrolled: bomb

  10. Fission reactant side: 2 terms 1 heavy isotope (examples: U-235 or Pu-239) bombarding particle – usually a neutron product side: at least 2 terms 2 medium-weight isotopes 1 or more neutrons huge amount energy released Fission = Division

  11. Fission 235U + 1n 91Kr + 142Ba + 31n + energy 56 0 36 92 235U + 1n 72Zn + 160Sm + 41n + energy 30 0 92 0 62 0 more than 200 different product isotopes identified from fission of U-235 small amount of mass is converted to energy according to E = mc2

  12. Fusion reactant side has 2 small nuclei: H + H; H + He; He + He product side: 1 nucleus (slightly larger; still small) and maybe a particle source of sun’s energy 2 nuclei unite 2H + 3H 4He + 1n + energy 0 2 1 1

  13. CERN • 27 kilometer ring • particles travel just below speed • of light • 10 hrs: particles make 400 • million revolutions of ring

  14. 4 miles in circumference! FermiLab

  15. Balancing Nuclear Equations

  16. Nuclear Equations - tasks • identify type (4 types): • natural transmutation • artificial transmutation • fission • fusion • balance to find unknown term

  17. Natural Transmutation – ID • 1 term on reactant side • starting isotope • 2 terms on product side • ending isotope & emitted particle • type of particle emitted characteristic of isotope – Table N

  18. Nuclear Equations • to balance: use conservation of both atomic number & mass number • mass number = left superscript • atomic number = left subscript

  19. Balancing Nuclear Equations 16N 0e + 16O -1 7 8 conservation of mass number:16 = 0 + 16 conservation of atomic number:7 = -1 + 8

  20. Writing Equations • write equation for decay of Thorium-232 • use Table N to find decay mode: α • write initial equation: 232Th 4He +X 90 2 figure out what element it turned into

  21. What’s under the hat? Little cats X, Y, & Z!

  22. Write an equation for the α decay of Th-232 232Th 4He + YX what’s X? 95 2 Z

  23. so Y = 228 232 = 4 + Y Y Z 2 232Th 4He + X 90 conservation of mass number: sum mass numbers on left side must = sum mass numbers on right side

  24. 2 90 Z 90 = 2 + Z so Z = 88 232Th 4He + 228X conservation of atomic number: sum of atomic numbers on left side must = sum of atomic numbers on right side

  25. 90 2 88 X = Ra use PT to find X: 232Th 4He + 228Ra 90 2 88 232Th 4He + 228X

  26. Radioactive Decay Series • sometimes 1 transmutation isn’t enough to achieve stability • some radioisotopes go through several changes before achieve stability (no longer radioactive)

  27. radioactive decay series: Th-232 transmuting to Pb-208

  28. β-14C 14N + 0e 6 7 -1 beta β+18F  18O + 0e 8 +1 positron 9

  29. How does the mass number or atomic number change in α,β or γ decay? • go to Table N: • find isotope that decays by α or βdecay • write equation • see how mass number (or atomic number) changes • 22688Ra 42 + X so X has to be 22286X • αdecay of Ra-226: • mass number decreases by 4 • atomic number decreases by 2

  30. So how do you know if an element is radioactive or not? the key is the proton to neutron ratio

More Related