Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

Nuclear Binding Energy02:13

Nuclear Binding Energy

12.3K
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons...
12.3K
Atomic Nuclei: Nuclear Spin01:08

Atomic Nuclei: Nuclear Spin

5.1K
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 contribute...
5.1K
Atomic Nuclei: Nuclear Magnetic Moment00:59

Atomic Nuclei: Nuclear Magnetic Moment

3.0K
All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
3.0K
Atomic Nuclei: Nuclear Spin State Overview01:03

Atomic Nuclei: Nuclear Spin State Overview

1.9K
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 one, the...
1.9K
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

1.7K
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.
1.7K
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

3.5K
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession,...
3.5K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

In Situ Insights into Enhanced Cooperative Ligand Exchange Kinetics via Solvent-Induced Restacking in a 2D Metal-Organic Framework.

Journal of the American Chemical Society·2026
Same author

The CP2K Program Package Made Simple.

The journal of physical chemistry. B·2026
Same author

Nitrile Groups as Build-In Molecular Sensors for Interfacial Effects at Electrocatalytically Active Carbon-Nitrogen Materials.

ACS applied materials & interfaces·2025
Same author

Robust Computation and Analysis of Vibrational Spectra of Layered Framework Materials Including Host-Guest Interactions.

Journal of chemical theory and computation·2024
Same author

Benchmarking the accuracy of the separable resolution of the identity approach for correlated methods in the numeric atom-centered orbitals framework.

The Journal of chemical physics·2024
Same author

Accelerating Core-Level <i>GW</i> Calculations by Combining the Contour Deformation Approach with the Analytic Continuation of <i>W</i>.

Journal of chemical theory and computation·2023

Related Experiment Video

Updated: May 1, 2026

Assembly of Nucleosomal Arrays from Recombinant Core Histones and Nucleosome Positioning DNA
10:40

Assembly of Nucleosomal Arrays from Recombinant Core Histones and Nucleosome Positioning DNA

Published on: September 11, 2013

22.1K

GW Plus Cumulant Approach for Predicting Core-Level Shakeup Satellites in Large Molecules.

Jannis Kockläuner1, Dorothea Golze1

  • 1Faculty of Chemistry and Food Chemistry, Technische Universität Dresden, 01062 Dresden, Germany.

Journal of Chemical Theory and Computation
|March 3, 2025
PubMed
Summary
This summary is machine-generated.

The GW+C approach accurately predicts molecular shakeup satellite features in X-ray photoemission spectroscopy. This method provides crucial insights into interpreting experimental data for conjugated molecules.

More Related Videos

Immunofluorescence Analysis of Endogenous and Exogenous Centromere-kinetochore Proteins
05:35

Immunofluorescence Analysis of Endogenous and Exogenous Centromere-kinetochore Proteins

Published on: March 3, 2016

15.0K
Label-Free Immunoprecipitation Mass Spectrometry Workflow for Large-scale Nuclear Interactome Profiling
11:19

Label-Free Immunoprecipitation Mass Spectrometry Workflow for Large-scale Nuclear Interactome Profiling

Published on: November 17, 2019

18.0K

Related Experiment Videos

Last Updated: May 1, 2026

Assembly of Nucleosomal Arrays from Recombinant Core Histones and Nucleosome Positioning DNA
10:40

Assembly of Nucleosomal Arrays from Recombinant Core Histones and Nucleosome Positioning DNA

Published on: September 11, 2013

22.1K
Immunofluorescence Analysis of Endogenous and Exogenous Centromere-kinetochore Proteins
05:35

Immunofluorescence Analysis of Endogenous and Exogenous Centromere-kinetochore Proteins

Published on: March 3, 2016

15.0K
Label-Free Immunoprecipitation Mass Spectrometry Workflow for Large-scale Nuclear Interactome Profiling
11:19

Label-Free Immunoprecipitation Mass Spectrometry Workflow for Large-scale Nuclear Interactome Profiling

Published on: November 17, 2019

18.0K

Area of Science:

  • Quantum chemistry
  • Spectroscopy
  • Computational physics

Background:

  • The GW approximation is a powerful tool for calculating core-level binding energies.
  • However, standard GW methods struggle to accurately predict shakeup satellite features in spectroscopy.
  • These features arise from electron excitations accompanying ionization events.

Purpose of the Study:

  • To extend the GW plus cumulant (GW+C) approach for accurate calculation of molecular 1s excitations.
  • To establish reliable conditions for applying GW+C to shakeup processes.
  • To provide a computationally efficient and accurate method for analyzing spectroscopic data.

Main Methods:

  • Developed an efficient O(N^4) GW+C implementation using an all-electron, numeric atom-centered orbital framework.
  • Investigated the importance of decoupling core and valence electron spaces for localized basis functions.
  • Validated basis set convergence for satellite spectra, emphasizing diffuse augmenting functions.

Main Results:

  • The GW+C scheme accurately predicts dominant shakeup satellite features in π-conjugated molecules (up to 40 atoms) within 0.5 eV of experimental values.
  • Demonstrated the critical role of core-valence decoupling and diffuse basis functions for accurate results.
  • Successfully applied the method to the acene series (benzene to pentacene).

Conclusions:

  • The extended GW+C method offers a reliable and accurate approach for computing molecular shakeup satellite spectra.
  • This work provides critical insights into the interpretation of experimentally observed satellite features in conjugated systems.
  • The efficient implementation enables accurate predictions for larger molecular systems.