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Related Concept Videos

Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

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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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Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

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In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
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Atomic Nuclei: Nuclear Spin State Overview01:03

Atomic Nuclei: Nuclear Spin State Overview

938
NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of...
938
Atomic Nuclei: Nuclear Spin01:08

Atomic Nuclei: Nuclear Spin

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All atomic particles possess an intrinsic angular momentum, or 'spin'. Electrons, protons, and neutrons each have a spin value of ½, although protons and neutrons in nuclei may have higher half-integer spins owing to energetic factors.
Atomic nuclei have a net nuclear spin, , which can have an integer or half-integer value. In atomic nuclei, the spins of protons are paired against each other but not with neutrons, and vice versa. Consequently, an even number of protons does not...
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Spin–Spin Coupling: Two-Bond Coupling (Geminal Coupling)01:20

Spin–Spin Coupling: Two-Bond Coupling (Geminal Coupling)

1.0K
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.
The central atom need not be NMR-active because its electrons are affected by the electron polarization of the spin-active atoms. However, spin information is transmitted less effectively than in one-bond coupling, and 2J values are usually weaker than 1J values. The energy of...
1.0K
¹H NMR: Interpreting Distorted and Overlapping Signals01:02

¹H NMR: Interpreting Distorted and Overlapping Signals

1.0K
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.
As Δν decreases and the signals move closer, the doublets appear increasingly distorted. The intensities of the inner lines increase at the cost of those of the outer lines as the signals are...
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Updated: Jun 28, 2025

Excitonic Hamiltonians for Calculating Optical Absorption Spectra and Optoelectronic Properties of Molecular Aggregates and Solids
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Analytic Nuclear Gradients for Complete Active Space Linearized Pair-Density Functional Theory.

Matthew R Hennefarth1, Matthew R Hermes1, Donald G Truhlar2

  • 1Department of Chemistry and Chicago Center for Theoretical Chemistry, University of Chicago, Chicago, Illinois 60637, United States.

Journal of Chemical Theory and Computation
|April 19, 2024
PubMed
Summary
This summary is machine-generated.

This study introduces analytic gradients for linearized pair-density functional theory (L-PDFT), a cost-effective method for modeling complex photochemical reactions. These gradients accurately predict molecular geometries and excitation energies for various molecules.

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Area of Science:

  • Computational Chemistry
  • Quantum Chemistry
  • Photochemistry

Background:

  • Modeling photochemical reactions is challenging due to conical intersections and multiconfigurational excited states.
  • Accurate potential energy surface calculations require multistate methods with state interaction.
  • Traditional multireference methods are computationally expensive.

Purpose of the Study:

  • To derive and implement analytic gradients for linearized pair-density functional theory (L-PDFT).
  • To demonstrate the utility of L-PDFT gradients for predicting molecular properties.
  • To provide a cost-effective alternative for accurate excited-state calculations.

Main Methods:

  • Derivation of analytic gradients for L-PDFT.
  • Implementation of L-PDFT gradients in the PySCF-forge software.
  • Application to formaldehyde, s-trans-butadiene, phenol, and cytosine.

Main Results:

  • Successful derivation and implementation of L-PDFT analytic gradients.
  • Accurate prediction of ground- and excited-state equilibrium geometries.
  • Reliable calculation of adiabatic excitation energies.

Conclusions:

  • L-PDFT with analytic gradients is a powerful and cost-effective tool for studying photochemical reactions.
  • The method accurately models potential energy surfaces with strong nuclear-electronic coupling.
  • This advancement facilitates more accurate predictions of molecular behavior in excited states.