The performance of many-body perturbation theory for calculating ground-state properties is investigated. We present fully numerical results for the electron gas in three and two dimensions in the framework of the GW approximation. The overall agreement with very accurate Monte Carlo data is excellent, even for those ranges of densities for which the GW approach is often supposed to be unsuitable. The latter seems to be due to the fulfillment of general conservation rules. These results open further prospects for accurate calculations of ground-state properties circumventing the limitations of standard density-functional theory
Atomic hydrogen provides a unique test case for computational electronic structure methods, since it...
We solve the Dyson equation for atoms and diatomic molecules within the GW approximation, in order t...
In order to increase the predictive pmver of electronic structure calculations on atomic and condens...
The performance of many-body perturbation theory for calculating ground-state properties is investig...
We present GW many-body results for ground-state properties of two simple but very distinct families...
With the aim of identifying universal trends, we compare fully self-consistent electronic spectra an...
We propose a new method for calculating total energies of systems of interacting electrons, which re...
GW calculations with a fully self-consistent Green’s function G and screened interaction W—based on ...
There is increasing interest in many-body perturbation theory as a practical tool for the calculatio...
Motivated by the recently developed renormalized second-order perturbation theory for ground-state e...
In electronic structure methods based on the correction of approximate density-functional theory (DF...
The ground state of the homogeneous electron gas is a cornerstone in quantum physics and chemistry. ...
The variational and diffusion quantum Monte Carlo methods are used to calculate the correlation ener...
We perform GW calculations on atoms and diatomic molecules at different levels of self-consistency a...
International audienceThe accuracy of the many-body perturbation theory GW formalism to calculate el...
Atomic hydrogen provides a unique test case for computational electronic structure methods, since it...
We solve the Dyson equation for atoms and diatomic molecules within the GW approximation, in order t...
In order to increase the predictive pmver of electronic structure calculations on atomic and condens...
The performance of many-body perturbation theory for calculating ground-state properties is investig...
We present GW many-body results for ground-state properties of two simple but very distinct families...
With the aim of identifying universal trends, we compare fully self-consistent electronic spectra an...
We propose a new method for calculating total energies of systems of interacting electrons, which re...
GW calculations with a fully self-consistent Green’s function G and screened interaction W—based on ...
There is increasing interest in many-body perturbation theory as a practical tool for the calculatio...
Motivated by the recently developed renormalized second-order perturbation theory for ground-state e...
In electronic structure methods based on the correction of approximate density-functional theory (DF...
The ground state of the homogeneous electron gas is a cornerstone in quantum physics and chemistry. ...
The variational and diffusion quantum Monte Carlo methods are used to calculate the correlation ener...
We perform GW calculations on atoms and diatomic molecules at different levels of self-consistency a...
International audienceThe accuracy of the many-body perturbation theory GW formalism to calculate el...
Atomic hydrogen provides a unique test case for computational electronic structure methods, since it...
We solve the Dyson equation for atoms and diatomic molecules within the GW approximation, in order t...
In order to increase the predictive pmver of electronic structure calculations on atomic and condens...