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Spin systems where the difference in chemical shifts of the coupled nuclei is greater than ten times J are called first-order spin systems. These nuclei are weakly coupled, and their chemical shifts and coupling constant can generally be estimated from the well-separated signals in the spectrum.
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In bromoethane, the three methyl protons are coupled to the two methylene protons that are three bonds away. In accordance with the n+1 rule, the signal from the methyl protons is split into three peaks with 1:2:1 relative intensities. The methylene protons appear as a quartet, with the relative intensities of 1:3:3:1.
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Spin–Spin Coupling: One-Bond Coupling01:17

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Coupling interactions are strongest between NMR-active nuclei bonded to each other, where spin information can be transmitted directly through the pair of bonding electrons. While nuclei polarize their electrons to the opposite spins, the bonding electron pair has opposite spins. Configurations with antiparallel nuclear spins are expected to be lower in energy. When coupling makes antiparallel states more favorable, J is considered to have a positive value. The one-bond coupling constant, 1J,...
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Spin–Spin Coupling: Two-Bond Coupling (Geminal Coupling)01:20

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Two NMR-active nuclei bonded to a central atom can be involved in geminal or two-bond coupling. Geminal coupling is commonly seen between diastereotopic protons in chiral molecules and unsymmetrical alkenes, among others.
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Atomic Nuclei: Nuclear Spin State Population Distribution01:14

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Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
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Spin–Spin Coupling: Three-Bond Coupling (Vicinal Coupling)01:22

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Vicinal or three-bond coupling is commonly observed between protons attached to adjacent carbons. Here, nuclear spin information is primarily transferred via electron spin interactions between adjacent C‑H bond orbitals. This generally favors the antiparallel arrangement of spins, so 3J values are usually positive.
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The Grassmann interpolation method for spin-unrestricted open-shell systems.

Jake A Tan1, Ka Un Lao1

  • 1Department of Chemistry, Virginia Commonwealth University, Richmond, Virginia 23284, USA.

The Journal of Chemical Physics
|June 1, 2023
PubMed
Summary
This summary is machine-generated.

Grassmann interpolation (G-Int) was extended for spin-unrestricted open-shell systems. This method provides accurate initial guesses for self-consistent field calculations, improving efficiency and enabling direct atomic charge calculations.

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Area of Science:

  • Computational Chemistry
  • Quantum Chemistry

Background:

  • The Grassmann interpolation (G-Int) method offers efficient density matrix interpolation.
  • Spin-unrestricted open-shell systems require separate interpolation for alpha and beta spin density matrices.

Purpose of the Study:

  • To extend and evaluate the performance of the G-Int method for spin-unrestricted open-shell systems.
  • To assess the utility of G-Int density matrices as initial guesses for self-consistent field (SCF) calculations.
  • To explore the direct calculation of atomic charges using G-Int density matrices.

Main Methods:

  • Application of G-Int to spin-unrestricted open-shell systems, specifically CO●+ and nickelocene.
  • Comparison of G-Int performance against conventional SCF guess schemes.
  • Direct calculation of atomic charges using Mulliken and ChElPG population analyses with G-Int density matrices.

Main Results:

  • The Frobenius norm errors for alpha and beta spin density matrices were found to be comparable.
  • G-Int density matrices significantly outperformed conventional SCF guess schemes.
  • Direct SCF energy evaluation without iterations is possible with G-Int density matrices, depending on accuracy requirements.
  • First-time use of spin-unrestricted G-Int density matrices for direct atomic charge calculations.

Conclusions:

  • The extended G-Int method is effective for spin-unrestricted open-shell systems.
  • G-Int provides superior initial guesses for SCF calculations, enhancing computational efficiency.
  • The method enables direct calculation of atomic charges, expanding its applicability in electronic structure analysis.