Real-time Kadanoff-Baym approach to nuclear response functions
Linear density response functions are calculated for symmetric nuclear matter of normal density by time-evolving two-time Green's functions in real time. Of particular interest is the effect of correlations. The system is therefore initially time-evolved with a collision term calculated in a di...
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Language | English |
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Abstract | Linear density response functions are calculated for symmetric nuclear matter of normal density by time-evolving two-time Green's functions in real time. Of particular interest is the effect of correlations. The system is therefore initially time-evolved with a collision term calculated in a direct Born approximation as well as with full (RPA) ring-summation until fully correlated. An external time-dependent potential is then applied. The ensuing density fluctuations are recorded to calculate the density response. This method was previously used by Kwong and Bonitz for studying plasma oscillations in a correlated electron gas. The energy-weighted sum-rule for the response function is guaranteed by using conserving self-energy insertions as the method then generates the full vertex-functions. These can alternatively be calculated by solving a Bethe -Salpeter equation as done in some previous works. The (first order) mean field is derived from a momentum-dependent (non-local) interaction while \(2^{nd}\) order self-energies are calculated using a particle-hole two-body effective (or 'residual') interaction given by a gaussian \it local \rm potential. We present numerical results for the response function \(S(\omega,q_0)\) for \(q_0=0.2,0.4\) and \(0.8 {\rm fm}^{-1}\). Comparison is made with the nucleons being un-correlated i.e. with only the first order mean field included, the 'HF+RPA' approximation. We briefly discuss the relation of our work with the Landau quasi-particle theory as applied to nuclear systems by Sj\"oberg and followers using methods developped by Babu and Brown, with special emphasis on the 'induced' interaction. |
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AbstractList | Linear density response functions are calculated for symmetric nuclear matter
of normal density by time-evolving two-time Green's functions in real time. Of
particular interest is the effect of correlations. The system is therefore
initially time-evolved with a collision term calculated in a direct Born
approximation as well as with full (RPA) ring-summation until fully correlated.
An external time-dependent potential is then applied. The ensuing density
fluctuations are recorded to calculate the density response. This method was
previously used by Kwong and Bonitz for studying plasma oscillations in a
correlated electron gas. The energy-weighted sum-rule for the response function
is guaranteed by using conserving self-energy insertions as the method then
generates the full vertex-functions. These can alternatively be calculated by
solving a Bethe -Salpeter equation as done in some previous works. The (first
order) mean field is derived from a momentum-dependent (non-local) interaction
while $2^{nd}$ order self-energies are calculated using a particle-hole
two-body effective (or 'residual') interaction given by a gaussian \it local
\rm potential. We present numerical results for the response function
$S(\omega,q_0)$ for $q_0=0.2,0.4$ and $0.8 {\rm fm}^{-1}$. Comparison is made
with the nucleons being un-correlated i.e. with only the first order mean field
included, the 'HF+RPA' approximation. We briefly discuss the relation of our
work with the Landau quasi-particle theory as applied to nuclear systems by
Sj\"oberg and followers using methods developped by Babu and Brown, with
special emphasis on the 'induced' interaction. Linear density response functions are calculated for symmetric nuclear matter of normal density by time-evolving two-time Green's functions in real time. Of particular interest is the effect of correlations. The system is therefore initially time-evolved with a collision term calculated in a direct Born approximation as well as with full (RPA) ring-summation until fully correlated. An external time-dependent potential is then applied. The ensuing density fluctuations are recorded to calculate the density response. This method was previously used by Kwong and Bonitz for studying plasma oscillations in a correlated electron gas. The energy-weighted sum-rule for the response function is guaranteed by using conserving self-energy insertions as the method then generates the full vertex-functions. These can alternatively be calculated by solving a Bethe -Salpeter equation as done in some previous works. The (first order) mean field is derived from a momentum-dependent (non-local) interaction while \(2^{nd}\) order self-energies are calculated using a particle-hole two-body effective (or 'residual') interaction given by a gaussian \it local \rm potential. We present numerical results for the response function \(S(\omega,q_0)\) for \(q_0=0.2,0.4\) and \(0.8 {\rm fm}^{-1}\). Comparison is made with the nucleons being un-correlated i.e. with only the first order mean field included, the 'HF+RPA' approximation. We briefly discuss the relation of our work with the Landau quasi-particle theory as applied to nuclear systems by Sj\"oberg and followers using methods developped by Babu and Brown, with special emphasis on the 'induced' interaction. |
Author | Kwong, N H Köhler, H S |
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BackLink | https://doi.org/10.48550/arXiv.1601.05463$$DView paper in arXiv https://doi.org/10.1088/1742-6596/696/1/012011$$DView published paper (Access to full text may be restricted) |
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Snippet | Linear density response functions are calculated for symmetric nuclear matter of normal density by time-evolving two-time Green's functions in real time. Of... Linear density response functions are calculated for symmetric nuclear matter of normal density by time-evolving two-time Green's functions in real time. Of... |
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SubjectTerms | Approximation Bethe-Salpeter equation Born approximation Collision dynamics Correlation Density Electron gas Green's functions Mathematical analysis Nuclear matter Nucleons Particle theory Physics - Nuclear Theory Plasma oscillations Real time Response functions Time dependence Variations |
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Title | Real-time Kadanoff-Baym approach to nuclear response functions |
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