Derivator
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Hi,
in the derivation of the Born-Oppenheimer-Approximation you have the Hamiltonoperator H=T_n + H_e, where T_n is the kinetic energy of the nuclei and H_e the electronic Hamiltonian.
The Schroedinger equation to solve is:
H \Psi = E \Psi
Now, what people do, is the following ansatz:
\Psi = \sum_k \Psi^n_k \Psi^e_k
where the \Psi^e_k are soultions of the electronic problem:
H_e \Psi^e_k = E_e \Psi^e_k
and \Psi^n_k is a coefficient that depends on the nucleonic coordinates.My question:
Using the ansatz:
\Psi = \sum_k \Psi^n_k \Psi^e_k
how can you tell, that you don't loose some possible solutions of H \Psi = E \Psi?
in the derivation of the Born-Oppenheimer-Approximation you have the Hamiltonoperator H=T_n + H_e, where T_n is the kinetic energy of the nuclei and H_e the electronic Hamiltonian.
The Schroedinger equation to solve is:
H \Psi = E \Psi
Now, what people do, is the following ansatz:
\Psi = \sum_k \Psi^n_k \Psi^e_k
where the \Psi^e_k are soultions of the electronic problem:
H_e \Psi^e_k = E_e \Psi^e_k
and \Psi^n_k is a coefficient that depends on the nucleonic coordinates.My question:
Using the ansatz:
\Psi = \sum_k \Psi^n_k \Psi^e_k
how can you tell, that you don't loose some possible solutions of H \Psi = E \Psi?