{"title":"Properties of NoO and YbO.","authors":"João G F Romeu, Sarah Sprouse, David A Dixon","doi":"10.1021/acs.jpca.4c07245","DOIUrl":null,"url":null,"abstract":"<p><p>Bond dissociation energies (BDEs) and spectroscopic parameters for the ground states of YbO and NoO were calculated at the Brueckner doubles (BD(T)) level and for NoO at the coupled cluster CCSD(T) level based on the closed-shell configurations Yb<sup>2+</sup>(4f<sup>14</sup>)O<sup>2-</sup>(2p<sup>6</sup>) and No<sup>2+</sup>(5f<sup>14</sup>)O<sup>2-</sup>(2p<sup>6</sup>). For YbO, the BD(T) BDE (3.93 eV) and vibrational frequency (686.3 cm<sup>-1</sup>) are consistent with the experiment; the BD(T) bond distance was 1.8492 Å, about 0.04 Å longer than the experiment. For NoO, the calculated BDEs are 3.07 eV (BD(T)) and 3.08 eV (CCSD(T)) and are expected to be good to ±3 kcal/mol (±0.13 eV). Potential energy curves (PECs) for the spin-orbit (Ω) states associated with the f<sup>13</sup>s<sup>1</sup> configurations of YbO and NoO were calculated at the SA-CASSCF/SO-CASPT2/aQ-DK level. PECs considering both the f<sup>13</sup>s<sup>1</sup> and f<sup>14</sup> configurations were calculated at this level, as the ground states are expected to contain both configurations. Due to a bias in the SA-CASSCF to the f<sup>13</sup>s<sup>1</sup> configurations, the f<sup>14</sup> configurations could not be properly described simultaneously with the f<sup>13</sup>s<sup>1</sup> ones. The natural population analysis based on the natural bond orbitals shows that YbO and NoO are quite ionic, with 5d orbitals being more important in YbO than the 6d orbitals in NoO.</p>","PeriodicalId":59,"journal":{"name":"The Journal of Physical Chemistry A","volume":" ","pages":"162-173"},"PeriodicalIF":2.7000,"publicationDate":"2025-01-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Journal of Physical Chemistry A","FirstCategoryId":"1","ListUrlMain":"https://doi.org/10.1021/acs.jpca.4c07245","RegionNum":2,"RegionCategory":"化学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2024/12/27 0:00:00","PubModel":"Epub","JCR":"Q3","JCRName":"CHEMISTRY, PHYSICAL","Score":null,"Total":0}
引用次数: 0
Abstract
Bond dissociation energies (BDEs) and spectroscopic parameters for the ground states of YbO and NoO were calculated at the Brueckner doubles (BD(T)) level and for NoO at the coupled cluster CCSD(T) level based on the closed-shell configurations Yb2+(4f14)O2-(2p6) and No2+(5f14)O2-(2p6). For YbO, the BD(T) BDE (3.93 eV) and vibrational frequency (686.3 cm-1) are consistent with the experiment; the BD(T) bond distance was 1.8492 Å, about 0.04 Å longer than the experiment. For NoO, the calculated BDEs are 3.07 eV (BD(T)) and 3.08 eV (CCSD(T)) and are expected to be good to ±3 kcal/mol (±0.13 eV). Potential energy curves (PECs) for the spin-orbit (Ω) states associated with the f13s1 configurations of YbO and NoO were calculated at the SA-CASSCF/SO-CASPT2/aQ-DK level. PECs considering both the f13s1 and f14 configurations were calculated at this level, as the ground states are expected to contain both configurations. Due to a bias in the SA-CASSCF to the f13s1 configurations, the f14 configurations could not be properly described simultaneously with the f13s1 ones. The natural population analysis based on the natural bond orbitals shows that YbO and NoO are quite ionic, with 5d orbitals being more important in YbO than the 6d orbitals in NoO.
期刊介绍:
The Journal of Physical Chemistry A is devoted to reporting new and original experimental and theoretical basic research of interest to physical chemists, biophysical chemists, and chemical physicists.