Atomic Quantum Mechanics - Hydrogen Atom (15.1-15.3) - PowerPoint PPT Presentation

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Atomic Quantum Mechanics - Hydrogen Atom (15.1-15.3)

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Atomic Quantum Mechanics - Hydrogen Atom (15.1-15.3) Assuming an atom doesn t move in space (translate), the SE is reduced to solving for the electrons only – PowerPoint PPT presentation

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Title: Atomic Quantum Mechanics - Hydrogen Atom (15.1-15.3)


1
Atomic Quantum Mechanics - Hydrogen Atom
(15.1-15.3)
  • Assuming an atom doesnt move in space
    (translate), the SE is reduced to solving for the
    electrons only
  • For single electron atoms and ions (e.g.,
    hydrogen), only the attraction of the electron to
    the nucleus is needed in the potential energy
    term
  • For many electron atoms and ions, repulsion
    between the electrons is needed in the PE
  • For the hydrogen atom, the solution to the SE is
    a set of atomic orbitals
  • The wavefunction involves three quantum numbers
    (n, l, ml) since three sets of boundary
    conditions are needed (1 for r, ?, and f)
  • The number of nodes in the wavefunction increases
    with increasing values of n and l
  • The energy of the hydrogen atom only depends on
    the principle quantum number n

2
Atomic QM Many Electron Atoms (15.6-15.7)
  • When more than one electron is present, Vee must
    be included in SE
  • Electrons are in constant motion, so potential
    energy is a constantly changing variable
    (electron correlation)
  • SE is no longer exactly solvable!
  • Solutions to many electron atom SE are very
    similar to hydrogen orbitals
  • The wavefunction for each electron is a
    hydrogen-like orbital (1s, 2s, 2p, etc.)
  • The energy associated with each electron now
    depends on n and l
    (orbital filling diagram)
  • Two electrons can have the same principle,
    angular, and magnetic quantum numbers
  • Electron configurations are used to show what the
    atomic wavefunction looks like
  • Electrons posses another quantum number
    associated with their spin
  • Electrons have another quantum number called the
    spin quantum number ( 1/2)
  • Pauli exclusion principle states no two electrons
    can have the same quantum numbers, so one
    electron in an orbital must be spin-up and the
    other spin-down

3
Hydrogen Wavefunctions
4
Radial Nodes in Hydrogen Orbitals
5
Angular Nodes in Hydrogen Orbitals
6
Probability Distribution Functions for Hydrogen
Orbitals
7
Orbital Filling Diagram
8
Atomic Orbital Overlap
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