Born-Oppenheimer approximation electron-nuclear separations

The idea of an effective potential function between the nuclei in a molecule can be formulated empirically (as we have done in Section 3.5 and Fig. 3.9), but it can be defined precisely and related to molecular parameters R, D and Dq only through quantum mechanics. The fundamental significance of the Born-Oppenheimer approximation is its separation of electronic and nuclear motions, which leads directly to the effective potential function. 

Note that the wave functions for the initial and final states and include both donor and acceptor. This equation is usually simplified by making the Born-Oppenheimer approximation for the separation of nuclear and electron wave functions, resulting in equation (12), in which V is the electronic matrix element describing the coupling between the electronic state of the reactants with those of the product, and FC is the Franck-Condon factor. 

Since the publication of the seminal paper by Born and Oppenheimer in 1927, the theoretical foundation of molecular science in the 20th century, and even to date, had been dominated by the so-called Born-Oppenheimer approximation, which dynamically separates electronic and nuclear motions under an assumption that electrons can follow the nuclear dynamics almost instantaneously. This idea led to the fixed nuclei approximation and the notion of electronic stationary-states that adjust themselves to any nuclear configurations in space. 

In currently available software, the Hamiltonian above is nearly never used. The problem can be simplified by separating the nuclear and electron motions. This is called the Born-Oppenheimer approximation. The Hamiltonian for a molecule with stationary nuclei is... 

The Born-Oppenheimer approximation is the first of several approximations used to simplify the solution of the Schradinger equation. It simplifies the general molecular problem by separating nuclear and electronic motions. This approximation is reasonable since the mass of a typical nucleus is thousands of times greater than that of an electron. The nuclei move very slowly with respect to the electrons, and the electrons react essentially instantaneously to changes in nuclear position. Thus, the electron distribution within a molecular system depends on the positions of the nuclei, and not on their velocities. Put another way, the nuclei look fixed to the electrons, and electronic motion can be described as occurring in a field of fixed nuclei. 

The concept of a potential energy surface has appeared in several chapters. Just to remind you, we make use of the Born-Oppenheimer approximation to separate the total (electron plus nuclear) wavefunction into a nuclear wavefunction and an electronic wavefunction. To calculate the electronic wavefunction, we regard the nuclei as being clamped in position. To calculate the nuclear wavefunction, we have to solve the relevant nuclear Schrddinger equation. The nuclei vibrate in the potential generated by the electrons. Don t confuse the nuclear Schrddinger equation (a quantum-mechanical treatment) with molecular mechanics (a classical treatment). 

Use of the Born-Oppenheimer approximation is implicit for any many-body problem involving electrons and nuclei as it allows us to separate electronic and nuclear coordinates in many-body wave function. Because of the large difference between electronic and ionic masses, the nuclei can be treated as an adiabatic background for instantaneous motion of electrons. So with this adiabatic approximation the many-body problem is reduced to the solution of the dynamics of the electrons in some frozen-in configuration of the nuclei. However, the total energy calculations are still impossible without making further simplifications and approximations. 

The separation of the electronic and nuclear motions depends on the large difference between the mass of an electron and the mass of a nucleus. As the nuclei are much heavier, by a factor of at least 1800, they move much more slowly. Thus, to a good approximation the movement of the elections in a polyatomic molecule can be assumed to take place in the environment of the nuclei that are fixed in a particular configuration. This argument is the physical basis of the Born-Oppenheimer approximation. 

Marcus uses the Born-Oppenheimer approximation to separate electronic and nuclear motions, the only exception being at S in the case of nonadiabatic reactions. Classical equilibrium statistical mechanics is used to calculate the probability of arriving at the activated complex only vibrational quantum effects are treated approximately. The result is... 

Separation of the wave functions describing the motion of nuclei and the wave function describing the electrons (Born-Oppenheimer approximation). This approximation is based on the fact that the nuclear particles are much heavier than the ele ctrons, and therefore much slower than the latter. In such a situation, the electronic wave function can be found at fixed positions of the nuclei. 

The purpose of most quantum chemical methods is to solve the time-independent Schrodinger equation. Given that the nuclei are much more heavier than the electrons, the nuclear and electronic motions can generally be treated separately (Born-Oppenheimer approximation). Within this approximation, one has to solve the electronic Schrodinger equation. Because of the presence of electron repulsion terms, this equation cannot be solved exactly for molecules with more than one electron. 

One branch of chemistry where the use of quantum mechanics is an absolute necessity is molecular spectroscopy. The topic is interaction between electromagnetic waves and molecular matter. The major assumption is that nuclear and electronic motion can effectively be separated according to the Born-Oppenheimer approximation, to be studied in more detail later on. The type of interaction depends on the wavelength, or frequency of the radiation which is commonly used to identify characteristic regions in the total spectrum, ranging from radio waves to 7-rays. 

Representing the molecular potential energy as an analytic function of the nuclear coordinates in this fashion implicitly invokes the Born-Oppenheimer approximation in separating the very fast electronic motions from the much slower ones of the nuclei. 

In the case of direct vibrational excitation, the vibrational transition probability is given by p, where are the intermediate and ground vibrational states, respectively, and is the vibrational transition moment. The electronic transition probability out of the intermediate state is < n < e ng e > n>, where are the excited and ground electronic states, respectively, and is the electronic dipole moment operator and vibrational state in the upper electronic state. Applying the Born-Oppenheimer approximation, where the nuclear electronic motion are separated, S can be presented as... 

This approximation of treating electronic and nuclear motions separately is the Born-Oppenheimer approximation. In the rest of this chapter, we consider the electronic Schrodinger equation. 

The Born-Oppenheimer approximation separates the molecular wave function into a product of electronic and nuclear wave functions ... 

The Born-Oppenheimer approximation permits the molecular Hamiltonian H to be separated into a component H, that depends only on the coordinates of the electrons relative to the nuclei, plus a component depending upon the nuclear coordinates. This in turn can be wriuen as a sum Hr + H, of terms for vibrational and rotational motion of ihe nuclei. 

In addition, we assume, for the systems of interest here, that the electronic motion is fast relative to the kinetic motion of the nuclei and that the total wave functions can be separated into a product form, with one term depending on the electronic motion and parametric in the nuclear coordinates and a second term describing the nuclear motion in terms of adiabatic potential hypersurfaces. This separation, based on the relative mass and velocity of an electron as compared with the nucleus mass and velocity, is known as the Born-Oppenheimer approximation. 

This is so because no coupling between electronic and nuclear motion is assumed within the Born-Oppenheimer approximation, which in the classical limit leads to separate conservation of the instantaneous heavy-particle motion. Denoting by EA(R,) and (/ ,) the instantaneous kinetic energy at the moment of transition in the upper- and lower potential curve,... 

Computational methods typically employ the Born-Oppenheimer approximation in most electronic structure programs to separate the nuclear and electronic parts of the Schrodinger equation that is still hard enough to solve approximately. There would be no potential energy (hyper)surface (PES) without the Born-Oppenheimer approximation -how difficult mechanistic organic chemistry would be without it ... 

In the Born-Oppenheimer approximation, in which the nuclear and electronic motions within the molecule are considered separately, the total... 

In molecular orbital (MO) theory, which is the most common implementation of QM used by chemists, electrons are distributed around the atomic nuclei until they reach a so-called self-consistent field (SCF), that is, until the attractive and repulsive forces between all the particles (electrons and nuclei) are in a steady state, and the energy is at a minimum. An SCF calculation yields the electronic wave function 4C (the electronic motion being separable from nuclear motion thanks to the Born-Oppenheimer approximation). This is the type of wave function usually referred to in the literature and in the rest of this chapter. 

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