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      Dehydrogenation of Ammonia Borane Impacts Valence and Core Electrons: A Photoemission Spectroscopic Study

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      ACS Omega
      American Chemical Society

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          Abstract

          Ammonia borane (H 3BNH 3) is a promising material for hydrogen storage and release. Dehydrogenation of ammonia borane produces small boron–nitrogen hydrides such as aminoborane (H 2BNH 2) and iminoborane (HBNH). The present study investigates ammonia borane and its two dehydrogenated products for the first time using calculated photoemission spectra of the valence and core electrons. It is found that a significant decrease in the dipole moment was observed associated with the dehydration from 5.397 D in H 3BNH 3, to 1.942 D in H 2BNH 2, and to 0.083 D in HBNH. Such reduction in the dipole moment impacts properties such as hydrogen bonding, dihydrogen bonding, and their spectra. Dehydrogenation of H 3BNH 3 impacts both the valence and core electronic structure of the boron–nitrogen hydrides. The calculated valence vertical ionization energy (VIE) spectra of the boron–nitrogen hydrides show that valence orbitals dominated by 2p-electrons of B and N atoms exhibit large changes, whereas orbitals dominated by s-electrons, such as (3a 14a 15a 1/3σ4σ5σ) remain less affected. The first ionization energy slightly increases from 10.57 eV for H 3BNH 3 to 11.29 eV for both unsaturated H 2BNH 2 and HBNH. In core space, the oxidative dehydrogenation of H 3BNH 3 affects the core electron binding energy (CEBE) of borane and nitrogen oppositely. The B1s binding energies increase from 194.01 eV in H 3BNH 3 to 196.93 eV in HBNH, up by 2.92 eV, whereas the N1s binding energies decrease from 408.20 eV in H 3BNH 3 to 404.88 eV in HBNH, dropped by 3.32 eV.

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          Atoms, molecules, solids, and surfaces: Applications of the generalized gradient approximation for exchange and correlation

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            Accurate and simple density functional for the electronic exchange energy: Generalized gradient approximation

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              Optimized Slater-type basis sets for the elements 1-118.

              Seven different types of Slater type basis sets for the elements H (Z = 1) up to E118 (Z = 118), ranging from a double zeta valence quality up to a quadruple zeta valence quality, are tested in their performance in neutral atomic and diatomic oxide calculations. The exponents of the Slater type functions are optimized for the use in (scalar relativistic) zeroth-order regular approximated (ZORA) equations. Atomic tests reveal that, on average, the absolute basis set error of 0.03 kcal/mol in the density functional calculation of the valence spinor energies of the neutral atoms with the largest all electron basis set of quadruple zeta quality is lower than the average absolute difference of 0.16 kcal/mol in these valence spinor energies if one compares the results of ZORA equation with those of the fully relativistic Dirac equation. This average absolute basis set error increases to about 1 kcal/mol for the all electron basis sets of triple zeta valence quality, and to approximately 4 kcal/mol for the all electron basis sets of double zeta quality. The molecular tests reveal that, on average, the calculated atomization energies of 118 neutral diatomic oxides MO, where the nuclear charge Z of M ranges from Z = 1-118, with the all electron basis sets of triple zeta quality with two polarization functions added are within 1-2 kcal/mol of the benchmark results with the much larger all electron basis sets, which are of quadruple zeta valence quality with four polarization functions added. The accuracy is reduced to about 4-5 kcal/mol if only one polarization function is used in the triple zeta basis sets, and further reduced to approximately 20 kcal/mol if the all electron basis sets of double zeta quality are used. The inclusion of g-type STOs to the large benchmark basis sets had an effect of less than 1 kcal/mol in the calculation of the atomization energies of the group 2 and group 14 diatomic oxides. The basis sets that are optimized for calculations using the frozen core approximation (frozen core basis sets) have a restricted basis set in the core region compared to the all electron basis sets. On average, the use of these frozen core basis sets give atomic basis set errors that are approximately twice as large as the corresponding all electron basis set errors and molecular atomization energies that are close to the corresponding all electron results. Only if spin-orbit coupling is included in the frozen core calculations larger errors are found, especially for the heavier elements, due to the additional approximation that is made that the basis functions are orthogonalized on scalar relativistic core orbitals. Copyright 2003 Wiley Periodicals, Inc.
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                Author and article information

                Journal
                ACS Omega
                ACS Omega
                ao
                acsodf
                ACS Omega
                American Chemical Society
                2470-1343
                29 September 2022
                11 October 2022
                : 7
                : 40
                : 35924-35932
                Affiliations
                []Department of Chemistry, University of British Columbia , 2036 Main Mall, Vancouver, British Columbia V6T 1Z1, Canada
                []Department of Chemistry and Biotechnology, School of Science, Computing and Engineering Technologies, Swinburne University of Technology , Melbourne, Victoria 3122, Australia
                Author notes
                Author information
                https://orcid.org/0000-0002-6584-0516
                Article
                10.1021/acsomega.2c04632
                9558250
                36249405
                d81904d0-35cb-4252-b980-8420fe6ac606
                © 2022 The Authors. Published by American Chemical Society

                Permits non-commercial access and re-use, provided that author attribution and integrity are maintained; but does not permit creation of adaptations or other derivative works ( https://creativecommons.org/licenses/by-nc-nd/4.0/).

                History
                : 22 July 2022
                : 24 August 2022
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                ao2c04632

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