{"title":"NoO和YbO的性质。","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":"{\"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}","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
摘要
基于闭合壳层构型Yb2+(4f14)O2-(2p6)和No2+(5f14)O2-(2p6)计算了YbO和NoO基态在Brueckner double (BD(T))能级和耦合簇CCSD(T)能级的键解离能(BDEs)和光谱参数。YbO的BD(T) BDE (3.93 eV)和振动频率(686.3 cm-1)与实验结果一致;BD(T)键距为1.8492 Å,比实验长约0.04 Å。对于NoO,计算的bde为3.07 eV (BD(T))和3.08 eV (CCSD(T)),预计可以达到±3 kcal/mol(±0.13 eV)。在SA-CASSCF/SO-CASPT2/aQ-DK水平上计算了YbO和NoO的f13s1构型的自旋轨道(Ω)态势能曲线(PECs)。考虑到f13s1和f14配置的PECs是在这个级别上计算的,因为基态预计包含这两种配置。由于SA-CASSCF对f13s1配置的偏差,导致f14配置不能与f13s1配置同时得到正确的描述。基于自然键轨道的自然居群分析表明,YbO和NoO具有很强的离子性,YbO中的5d轨道比NoO中的6d轨道更重要。
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.