Näytä suppeat kuvailutiedot

dc.contributor.authorTolvanen, Alpi
dc.contributor.authorTiihonen, Juha
dc.contributor.authorRantala, Tapio T.
dc.date.accessioned2022-04-26T10:38:47Z
dc.date.available2022-04-26T10:38:47Z
dc.date.issued2022
dc.identifier.citationTolvanen, A., Tiihonen, J., & Rantala, T. T. (2022). Diamagnetic susceptibility from a nonadiabatic path-integral simulation of few-electron systems. <i>Physical Review A</i>, <i>105</i>(2), Article 022816. <a href="https://doi.org/10.1103/PhysRevA.105.022816" target="_blank">https://doi.org/10.1103/PhysRevA.105.022816</a>
dc.identifier.otherCONVID_118909674
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/80724
dc.description.abstractDiamagnetism is the response of dynamical compositions of charged particles, electrons, and nuclei, to an incident magnetic field. In this paper, we study how the finite temperature and finite nuclear masses affect the diamagnetic susceptibilities of selected small atoms and molecules, as limiting cases of dilute gas. We use nonrelativistic path-integral Monte Carlo simulation (PIMC), where both electrons and nuclei are treated on equal footing at finite temperatures in sampling exact Coulomb pair density matrices. The PIMC estimator of diamagnetic susceptibility has been briefly introduced in Ceperley [D. M. Ceperley, Rev. Mod. Phys. 67, 279 (1995)], but here we present a comprehensive derivation, discussion of practical effects, and proof-of-concept results for selected few-body Coulomb systems. Our results are in perfect agreement with high-accuracy literature references, where available, but also demonstrate additional thermal effects of the diamagnetic response of low-mass systems.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review A
dc.rightsIn Copyright
dc.titleDiamagnetic susceptibility from a nonadiabatic path-integral simulation of few-electron systems
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202204262398
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineNanoscience Centerfi
dc.contributor.oppiaineNanoscience Centeren
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9926
dc.relation.numberinseries2
dc.relation.volume105
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysomagneettikentät
dc.subject.ysomagnetismi
dc.subject.ysokvanttifysiikka
dc.subject.ysoMonte Carlo -menetelmät
dc.subject.ysosimulointi
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p19032
jyx.subject.urihttp://www.yso.fi/onto/yso/p7808
jyx.subject.urihttp://www.yso.fi/onto/yso/p5564
jyx.subject.urihttp://www.yso.fi/onto/yso/p6361
jyx.subject.urihttp://www.yso.fi/onto/yso/p4787
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevA.105.022816
jyx.fundinginformationThe authors wish to acknowledge CSC-IT Center for Science, Finland, for computational resources.
dc.type.okmA1


Aineistoon kuuluvat tiedostot

Thumbnail

Aineisto kuuluu seuraaviin kokoelmiin

Näytä suppeat kuvailutiedot

In Copyright
Ellei muuten mainita, aineiston lisenssi on In Copyright