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Chem3D Users Manual - CambridgeSoft

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the same wave function and a constant. The wave<br />

function is called an eigenfunction, and the constant, an<br />

eigenvalue.<br />

nuclear energy by an electronic Hamiltonian, which<br />

can be solved at any set of nuclear coordinates. The<br />

electronic version of the Schrödinger equation is:<br />

Administrator<br />

• Exact solutions to the Schrödinger equation<br />

are possible only for the simplest 1 electron-1<br />

nucleus system. These solutions, however,<br />

yield the basis for all of quantum mechanics.<br />

• The solutions describe a set of allowable states<br />

for an electron. The observable quantity for<br />

these states is described as a probability<br />

function. This function is the square of the<br />

wave function, and when properly normalized,<br />

describes the probability of finding an electron<br />

in that state.<br />

∫Ψ 2 ()r r d = 1<br />

where r = radius (x, y, and z)<br />

H elec<br />

Ψ elec<br />

=E elec<br />

Ψ elec<br />

Another approximation assumes that electrons act<br />

independently of one another, or, more accurately,<br />

that each electron is influenced by an average field<br />

created by all other electrons and nuclei. Each<br />

electron in its own orbital is unimpeded by its<br />

neighbors.<br />

The electronic Hamiltonian is thus simplified by<br />

representing it as a sum of 1-electron Hamiltonians,<br />

and the wave equation becomes solvable for<br />

individual electrons in a molecule once a functional<br />

form of the wave function can be derived.<br />

• There are many solutions to this probability<br />

function. These solutions are called atomic<br />

orbitals, and their energies, orbital energies.<br />

• For a molecule with many electrons and nuclei<br />

the aim is to be able to describe molecular<br />

orbitals and energies in as analogous a fashion<br />

to the original Schrödinger equation as<br />

possible.<br />

Approximations to the Hamiltonian<br />

The first approximation made is known as the<br />

Born-Oppenheimer approximation, which allows<br />

separate treatment of the electronic and nuclear<br />

energies. Due to the large mass difference between<br />

an electron and a nucleus, a nucleus moves so much<br />

more slowly than an electron that it can be regarded<br />

as motionless relative to the electron. In effect, this<br />

approximation considers electrons to be moving<br />

with respect to a fixed nucleus. This allows the<br />

electronic energy to be described separately from<br />

H elec<br />

=<br />

∑<br />

H eff ψ =εψ<br />

H i<br />

eff<br />

For a molecular system, a matrix of these 1-electron<br />

Hamiltonians is constructed to describe the<br />

1-electron interactions between a single electron<br />

and the core nucleus. The following represents the<br />

matrix for two atomic orbitals, φ µ and φ ν .<br />

H uv ∫ =φ H eff µ v<br />

φdτ<br />

i<br />

However, in molecular systems, this Hamiltonian<br />

does not account for the interaction between<br />

electrons with 2 or more different interaction<br />

centers or the interaction of two electrons. Thus,<br />

the Hamiltonian is further modified. This<br />

modification renames the Hamiltonian operator to<br />

the Fock operator.<br />

Fψ=Eψ<br />

The Fock operator is composed of a set of 1-<br />

electron Hamiltonians that describe the 1-electron,<br />

1 center interactions and is supplemented by terms<br />

144•Computation Concepts<br />

<strong>CambridgeSoft</strong><br />

Quantum Mechanics Theory in Brief

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