18bishop ec (1)

Upload: anand-muruganantham

Post on 25-Feb-2018

223 views

Category:

Documents


0 download

TRANSCRIPT

  • 7/25/2019 18Bishop EC (1)

    1/25

    Chapter 18

    Nuclear Chemistry

  • 7/25/2019 18Bishop EC (1)

    2/25

    Chapter

    Map

  • 7/25/2019 18Bishop EC (1)

    3/25

    Nuclides

    Nuclide = a particular type ofnucleus, characterized by a

    specific atomic number and

    nucleon number

    Nucleon numberormass number

    = the number of nucleons(protons and neutrons) in the

    nucleus of a nuclide.

  • 7/25/2019 18Bishop EC (1)

    4/25

    Nuclide Symbolism

  • 7/25/2019 18Bishop EC (1)

    5/25

    Nuclear Stability Electrostatic force = the force that

    causes opposite electrical chargesto attract each other.

    Strong force = the force betweennucleons (protons and neutrons).

    Neutrons increase the attractionfrom the strong force without

    increasing electrostatic repulsion

    between nucleons.

  • 7/25/2019 18Bishop EC (1)

    6/25

    Band ofStability

  • 7/25/2019 18Bishop EC (1)

    7/25

    Alpha Emission

  • 7/25/2019 18Bishop EC (1)

    8/25

    Beta Emission

  • 7/25/2019 18Bishop EC (1)

    9/25

    Positron Emission

  • 7/25/2019 18Bishop EC (1)

    10/25

    Electron Capture

  • 7/25/2019 18Bishop EC (1)

    11/25

    Gamma Emission

  • 7/25/2019 18Bishop EC (1)

    12/25

    Nuclear Reactions Nuclear reactions involve changes

    in the nucleus, whereas chemicalreactions involve the loss, gain,and sharing of electrons.

    Different isotopes of the sameelement may undergo very

    different nuclear reactions, eventhough an elements isotopes allshare the same chemical

    characteristics.

  • 7/25/2019 18Bishop EC (1)

    13/25

    Nuclear Reactions(cont.)

    Unlike chemical reactions, the ratesof nuclear reactions are unaffected

    by temperature, pressure, and the

    presence of other atoms to which

    the radioactive atom may be

    bonded. Nuclear reactions, in general, give

    off much more energy thanchemical reactions

  • 7/25/2019 18Bishop EC (1)

    14/25

    Nuclear

    Equations

  • 7/25/2019 18Bishop EC (1)

    15/25

    General Nuclear Equations

  • 7/25/2019 18Bishop EC (1)

    16/25

    Half-life = the time it takes for

    one-half of a sample to disappear.

  • 7/25/2019 18Bishop EC (1)

    17/25

    Radioactive Decay Series

  • 7/25/2019 18Bishop EC (1)

    18/25

    Radiation Effect onBody

    Radioactive emissions ionize atoms andmolecules. This also leads to freeradicals (particles with unpairedelectrons).

    H2O H2O+ + e

    H2O+ + H2O H3O

    + + OH

    H2O + e

    H

    + OH

    These reactive particles react withimportant substances in the body,leading to immediate damage anddelayed problems, such as cancer.

  • 7/25/2019 18Bishop EC (1)

    19/25

    Uses for RadioactiveNuclides

    Cancer radiation treatment

    Computer imaging techniques

    Radiocarbon dating

    Smoke detectors

    Food irradiation

    Radioactive tracers

  • 7/25/2019 18Bishop EC (1)

    20/25

    Nuclear Energy Binding energy = the amount of energy

    released when a nucleus is formed. Binding energy per nucleon generally

    increases from small atoms to atoms with

    a mass number around 56. Thus fusingsmall atoms to form medium-sized atoms(nuclear fusion) releases energy.

    Binding energy per nucleon generallydecreases from atoms with a massnumber around 56 to larger atoms. Thussplitting large atoms to form medium-

    sized atoms (nuclear fission) alsoreleases energy.

  • 7/25/2019 18Bishop EC (1)

    21/25

    Binding

    Energy

    per Nucleon

  • 7/25/2019 18Bishop EC (1)

    22/25

    Nuclear Fission

    Ch i

  • 7/25/2019 18Bishop EC (1)

    23/25

    Chain

    Reaction

  • 7/25/2019 18Bishop EC (1)

    24/25

    Nuclear Reactor

  • 7/25/2019 18Bishop EC (1)

    25/25

    Nuclear Fusion Powers the Sun