Darwin and mass-velocity relativistic corrections in the non-Born-Oppenheimer calculations of pure vibrational states of H2

dc.contributor.authorKeĀødziera, Dariusz
dc.contributor.authorStanke, Monika
dc.contributor.authorBubin, Sergiy
dc.contributor.authorBarysz, Maria
dc.contributor.authorAdamowicz, Ludwik
dc.date.accessioned2016-01-29T06:29:15Z
dc.date.available2016-01-29T06:29:15Z
dc.date.issued2006
dc.description.abstractThe Darwin and mass-velocity relativistic corrections have been calculated for all pure vibrational states of the H2 using the perturbation theory and very accurate variational wave functions obtained without assuming the Born-Oppenheimer BO approximation. Expansions in terms of explicitly correlated Gaussians with premultipliers in the form of even powers of the internuclear distance were used for the wave functions. With the inclusion of the two relativistic corrections to the non-BO energies the transition energies for the highest states agree more with the experimental resultsru_RU
dc.identifier.citationKeĀødziera Dariusz, Stanke Monika, Bubin Sergiy, Barysz Maria, Adamowicz Ludwik; 2006; Darwin and mass-velocity relativistic corrections in the non-Born-Oppenheimer calculations of pure vibrational states of H2; THE JOURNAL OF CHEMICAL PHYSICSru_RU
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/1095
dc.language.isoenru_RU
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectResearch Subject Categories::NATURAL SCIENCES::Physicsru_RU
dc.subjectBorn-Oppenheimer approximationru_RU
dc.titleDarwin and mass-velocity relativistic corrections in the non-Born-Oppenheimer calculations of pure vibrational states of H2ru_RU
dc.typeArticleru_RU

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