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dc.contributor.authorVítek, Aleš
dc.contributor.authorŠarmanová, Martina
dc.contributor.authorKalus, René
dc.date.accessioned2022-05-04T09:11:40Z
dc.date.available2022-05-04T09:11:40Z
dc.date.issued2021
dc.identifier.citationTheoretical Chemistry Accounts. 2021, vol. 140, issue 6, art. no. 54.cs
dc.identifier.issn1432-881X
dc.identifier.issn1432-2234
dc.identifier.urihttp://hdl.handle.net/10084/146109
dc.description.abstractParallel-tempering Monte Carlo calculations have been performed for the Hg8 cluster in an isothermal-isobaric ensemble. Temperature and pressure dependent cluster residual heat capacity and Pearson correlation coefficient for cluster energy and volume have been calculated over a broad range of cluster temperatures and external pressures using a 2D multiple histogram method. Calculated data have subsequently been used in investigations of structural changes in Hg8 induced by increased pressure and temperature. A global picture of these changes is provided in the form of a cluster temperature-pressure phase diagram.cs
dc.language.isoencs
dc.publisherSpringer Naturecs
dc.relation.ispartofseriesTheoretical Chemistry Accountscs
dc.relation.urihttps://doi.org/10.1007/s00214-021-02739-8cs
dc.rightsCopyright © 2021, The Author(s), under exclusive licence to Springer-Verlag GmbH Germany, part of Springer Naturecs
dc.subjectmercury clusterscs
dc.subjectstructurecs
dc.subjectstructural changescs
dc.subjectMonte Carlo simulationscs
dc.titleIsothermal-isobaric thermodynamics of small HgN clusters. A case study on Hg8cs
dc.typearticlecs
dc.identifier.doi10.1007/s00214-021-02739-8
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.volume140cs
dc.description.issue6cs
dc.description.firstpageart. no. 54cs
dc.identifier.wos000694963600001


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