1 / 27

Nuclear Chemistry

Nuclear Chemistry. “Bravo” Test 1954 – 15,000 kilotons. Radioactivity and Nuclear Energy. Objective: To learn the types of radioactive decay Objective: To learn to write nuclear equations that describes radioactive decay

fineen
Download Presentation

Nuclear Chemistry

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 Chemistry “Bravo” Test 1954 – 15,000 kilotons

  2. Radioactivity and Nuclear Energy Objective: To learn the types of radioactive decay Objective: To learn to write nuclear equations that describes radioactive decay Objective: To learn how one element may be changed into another by particle bombardment

  3. What makes an atom radioactive? Radioactivity: the spontaneous decomposition of a nucleus to form another nucleus and produce one or more particles. -the neutrons act as glue holding the nucleus together -the heavier the atom, the more likely it is to be radioactive -if the number of protons in the nucleus exceeds 83, then the nuclide is radioactive

  4. Types of Radioactive Decay • alpha production (a, He): helium nucleus • beta production (b, e): • gamma ray production (g):

  5. Specifying Isotopes A X = the symbol of the element A = mass number (protons + neutrons) Z = the atomic number (number of protons) X Z

  6. Nuclear Symbols Mass number, A (p+ + no) Element symbol Atomic number, Z (number of p+)

  7. Key to Understanding Nuclear Reactions In nuclear reactions, both the atomic number Z and the mass number A must be conserved

  8. Balancing Nuclear Equations 222 226 = 4 + ____ 222 Rn 86 86 88 = 2 + ___ Atomic number 86 is radon, Rn

  9. Alpha Decay Alpha production (a): an alpha particle is a helium nucleus Alpha decay is limited to heavy, radioactive nuclei

  10. Alpha (α) Decay an alpha particle (helium nucleus) is produced P+N -4 4 P+N He + E2 E1 P 2 P-2

  11. Alpha Radiation Limited to VERY large nucleii.

  12. Example of Alpha Decay Radium 222 decays by α particle production to Radon 218 4 222 218 He + Rn Ra 88 2 86

  13. Beta Decay Beta production (b): A beta particle is an electron ejected from the nucleus Beta emission converts a neutron to a proton

  14. Beta (β) Decay P+N P+N 0 e + E2 E1 P -1 P+1 Beta emission converts a neutron to a proton

  15. Beta Radiation Converts a neutron into a proton.

  16. Example of Beta Decay Notice the mass of the beta particle is zero; it is so small that is must be neglected. 14 0 14 e N + C 6 -1 7

  17. Example of Beta Decay Thorium 234 decays by β particle production to Protactinium 234 (notice: no change in mass number A, and an increase of 1 in atomic number Z) 234 234 0 e Pa + Th 90 -1 91

  18. Gamma Ray Production Gamma ray production (g): Gamma rays are high energy photons produced in association with other forms of decay. Gamma rays are massless and do not, by themselves, change the nucleus

  19. Gamma Ray Production Gamma ray production (g): Gamma rays are high energy photons produced in association with other forms of decay. Gamma rays are massless and do not, by themselves, change the nucleus

  20. Positron Production Positron emission: Positrons are the anti-particle of the electron Positron emission converts a proton to a neutron

  21. Positron Production P+N P+N 0 e + E2 E1 P 1 P-1 Positron emission converts a proton to a neutron

  22. Electron Capture Electron capture: (inner-orbital electron is captured by the nucleus) Electron capture converts a proton to a neutron

  23. Types of Radiation

  24. NuclearStability Decay will occur in such a way as to return a nucleus to the band (line) of stability. The most stable nuclide is Iron-56 If Z > 83, the nuclide is radioactive

  25. A Decay Series A radioactive nucleus reaches a stable state by a series of steps Graphic – Wikimedia Commons User Tosaka

More Related