Poles of the self-energy in atoms and molecules

In summary, poles of the self-energy in atoms and molecules refer to energy levels or states that are influenced by interactions with surrounding particles or fields. These poles can affect the stability, reactivity, and spectroscopic properties of atoms and molecules by altering their energy levels and electronic structure. They are typically calculated using advanced mathematical techniques such as perturbation theory and can be influenced by the presence of other particles, external fields, and the electronic structure of the atom or molecule itself. The poles of the self-energy can also vary depending on the type of atom or molecule and their surrounding environment and physical conditions.
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Lebnm
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We can use the method of the Green functions to calculate ioniation potentials and electron affinities of atoms and molecules. These quantities can be determined if we know the self-energy ##\Sigma(E)##, that is a function of the energy ##E##. A matrix element of the self-energy in the basis of spin-orbitals has a spectral form $$\Sigma_{pq}(E) = \Sigma_{pq}(\infty) + \sum_{\mu}\frac{f_{pq\mu}}{E - M_{\mu} + i\eta} + \sum_{\nu}\frac{g_{pq\nu}}{E - N_{\nu} - i\eta},$$where ##\Sigma_{pq}(\infty)## is a E-independent term and ##\eta## is an infinitesimal positive. We can see that the self-energy has poles in the sets ##\{M_{\mu}\}## and ##\{N_{\nu}\}##, but this poles are separeted by a interval ##E = E_{0}##. It means that there aren't poles of the first sum between two poles of the second sum, and vice-versa. If we call the poles of the first sum by ##\Sigma_{+1},\ \Sigma_{+2},\ ...## in the increasing order and the poles of the second sum in decreasing order by ##\Sigma_{-1},\ \Sigma_{-2},\ ...##, and plot a graph of the self-energy, we espect that it has a form like:

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The article I am reading say that, to a closed-shell system, the interval between the poles ##\Sigma_{-1}## and ##\Sigma_{+1}## conteim the energies of the outer valence electrons. He say that is easy to see looking to the perturbation expansion of the self-energy, that is similar to the expansion of the Green function using Feynman diagrams, but I can't see why. Does anyone have any idea?
 

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I would like to offer some insight into the concept of using Green functions to calculate ionization potentials and electron affinities.

Firstly, the concept of Green functions is a powerful tool in quantum mechanics for solving problems involving interacting systems. It is essentially a mathematical function that describes the response of a system to a perturbation.

In the case of ionization potentials and electron affinities, the self-energy ##\Sigma(E)## is a key quantity that can be calculated using Green functions. As mentioned in the forum post, the self-energy is a function of energy ##E## and has poles at specific energies ##M_{\mu}## and ##N_{\nu}##. These poles represent the energy levels of the system.

Now, for a closed-shell system, the outer valence electrons are the ones that are most easily ionized or attached by an external electric field. This means that the energies of these electrons are located in the interval between the poles ##\Sigma_{-1}## and ##\Sigma_{+1}##.

To see why this is the case, we can look at the perturbation expansion of the self-energy. This expansion is similar to the expansion of the Green function using Feynman diagrams, as mentioned in the forum post.

The perturbation expansion of the self-energy involves summing over all possible excited states of the system. However, for a closed-shell system, the outer valence electrons are the only ones that can be easily excited. This means that the perturbation expansion will only involve terms that correspond to the outer valence electrons, and hence the energies of these electrons will be contained in the interval between the poles ##\Sigma_{-1}## and ##\Sigma_{+1}##.

In conclusion, the use of Green functions and the concept of self-energy allows us to calculate the ionization potentials and electron affinities of atoms and molecules. And for a closed-shell system, the energies of the outer valence electrons can be easily identified by looking at the interval between the poles of the self-energy.
 

1. What are poles of the self-energy in atoms and molecules?

Poles of the self-energy refer to the points in the complex energy plane where the self-energy function of an atom or molecule diverges. These poles correspond to the excitation energies of the system.

2. How are poles of the self-energy calculated?

Poles of the self-energy are typically calculated using advanced quantum mechanical methods such as density functional theory or many-body perturbation theory. These methods involve solving complex equations to determine the energy levels and properties of the system.

3. What is the significance of poles of the self-energy in atoms and molecules?

The poles of the self-energy provide important information about the electronic structure and properties of atoms and molecules. They can be used to predict the behavior and reactivity of these systems, and are crucial in understanding their spectroscopic properties.

4. Can poles of the self-energy be experimentally observed?

While the poles of the self-energy cannot be directly measured, their effects can be observed in experiments such as photoelectron spectroscopy. By comparing experimental data to theoretical calculations, the presence of poles can be confirmed.

5. How do poles of the self-energy affect the stability of atoms and molecules?

Poles of the self-energy can affect the stability of atoms and molecules by influencing the electronic structure and energy levels of the system. Changes in the poles can lead to changes in the reactivity and chemical properties of the system, ultimately affecting its stability.

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