Coulomb potentials and Taylor expansions in time-dependent density-functional theory
hal.structure.identifier | ||
dc.contributor.author | Fournais, Søren | |
hal.structure.identifier | ||
dc.contributor.author | Lampart, Jonas
HAL ID: 174062 ORCID: 0000-0002-6980-3800 | |
hal.structure.identifier | ||
dc.contributor.author | Lewin, Mathieu
HAL ID: 1466 ORCID: 0000-0002-1755-0207 | |
hal.structure.identifier | ||
dc.contributor.author | Sørensen, Thomas Østergaard | |
dc.date.accessioned | 2017-03-15T15:19:38Z | |
dc.date.available | 2017-03-15T15:19:38Z | |
dc.date.issued | 2016 | |
dc.identifier.issn | 2469-9934 | |
dc.identifier.uri | https://basepub.dauphine.fr/handle/123456789/16367 | |
dc.language.iso | en | en |
dc.subject | TDDFT | en |
dc.subject.ddc | 520 | en |
dc.title | Coulomb potentials and Taylor expansions in time-dependent density-functional theory | en |
dc.type | Article accepté pour publication ou publié | |
dc.description.abstracten | We investigate when Taylor expansions can be used to prove the Runge-Gross theorem, which is at the foundation of time-dependent density-functional theory (TDDFT). We start with a general analysis of the conditions for the Runge-Gross argument, especially the time differentiability of the density. The latter should be questioned in the presence of singular (e.g., Coulomb) potentials. Then we show that a singular potential in a one-body operator considerably decreases the class of time-dependent external potentials to which the original argument can be applied. A two-body singularity has an even stronger impact and an external potential is essentially incompatible with it. For the Coulomb interaction and all reasonable initial many-body states, the Taylor expansion only exists to a finite order, except for constant external potentials. Therefore, high-order Taylor expansions are not the right tool to study atoms and molecules in TDDFT. | en |
dc.relation.isversionofjnlname | Physical Review A | |
dc.relation.isversionofjnlvol | 93 | en |
dc.relation.isversionofjnlissue | 6 | en |
dc.relation.isversionofjnldate | 2016 | |
dc.relation.isversionofjnlpages | n°062510 | en |
dc.relation.isversionofdoi | 10.1103/PhysRevA.93.062510 | en |
dc.identifier.urlsite | https://arxiv.org/abs/1603.02219v2 | en |
dc.relation.isversionofjnlpublisher | American Physical Society | en |
dc.subject.ddclabel | Sciences connexes (physique, astrophysique) | en |
dc.relation.forthcoming | non | en |
dc.relation.forthcomingprint | non | en |
dc.description.ssrncandidate | non | en |
dc.description.halcandidate | non | en |
dc.description.readership | recherche | en |
dc.description.audience | International | en |
dc.relation.Isversionofjnlpeerreviewed | non | en |
dc.relation.Isversionofjnlpeerreviewed | non | en |
dc.date.updated | 2017-03-09T13:52:36Z | |
hal.author.function | aut | |
hal.author.function | aut | |
hal.author.function | aut | |
hal.author.function | aut |
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