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Related Concept Videos

Potential Energy00:52

Potential Energy

The energy stored by a structure and location of matter in space is called potential energy. For instance, raising a kettlebell changes its spatial location and increases its potential energy. Similarly, a stretched rubber band contains potential energy which, under certain conditions, can be converted into other forms of energy, such as kinetic energy.
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Irradiation of a spin-active nucleus causes an increase or decrease in the signal intensity of neighboring nuclei that are not necessarily chemically bonded or involved in J-coupling. This phenomenon, called the nuclear Overhauser enhancement (NOE), results from through-space interactions between the nuclear spins. The NOE effect decreases with increasing internuclear distance and is generally not observed beyond 4 angstroms. In NOE, dipole-dipole interactions between neighboring spin-active...
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Elastic potential energy is the energy stored as a result of the deformation of an elastic object, such as the stretching of a spring. An object is elastic if it returns to its original shape and size after being deformed. 
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Thermodynamic potentials are state functions that are extremely useful in analyzing a thermodynamic system. They have dimensions of energy. The four important thermodynamic potentials are internal energy, enthalpy, Helmholtz free energy, and Gibbs free energy. These thermodynamic potentials can be expressed using two of the following variables: pressure, volume, temperature, and entropy. These two variables are expressed as the rate of change of the thermodynamic potential with respect to other...
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Nuclear Binding Energy

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 are bound together;...
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An ionic compound is stable because of the electrostatic attraction between its positive and negative ions. The lattice energy of a compound is a measure of the strength of this attraction. The lattice energy (ΔHlattice) of an ionic compound is defined as the energy required to separate one mole of the solid into its component gaseous ions. For the ionic solid sodium chloride, the lattice energy is the enthalpy change of the process:

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High-Pressure Inelastic Neutron Spectroscopy: Experimental Validation of Machine-Learned Interatomic Potential Energy

Jeff Armstrong1,2, Adam Jackson3, Alin Elena4

  • 1ISIS Neutron and Muon Source, Science and Technology Facilities Council, UK Research and Innovation, Rutherford Appleton Laboratory, Harwell Campus, Didcot, OX11 0QX, U.K.

The Journal of Physical Chemistry Letters
|June 5, 2026
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Summary
This summary is machine-generated.

High-pressure inelastic neutron spectroscopy (INS) experimentally validates machine-learned interatomic potentials (MLIPs). This method confirms MLIP accuracy under pressure, crucial for reliable materials modeling.

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Area of Science:

  • Computational Materials Science
  • Spectroscopy
  • Machine Learning

Background:

  • Machine-learned interatomic potentials (MLIPs) offer accurate and cost-effective atomistic modeling.
  • Experimental validation of MLIP reliability beyond training data is challenging.

Purpose of the Study:

  • To use pressure-dependent inelastic neutron spectroscopy (INS) to experimentally probe MLIP transferability.
  • To validate the predictive accuracy of MLIPs under varying thermodynamic conditions.

Main Methods:

  • Measurement of INS spectra of crystalline 2,5-diiodothiophene at 10 K under atmospheric pressure and 1.5 GPa using a high-pressure clamp cell.
  • Development and fine-tuning of MACE-based MLIPs using density-functional theory (DFT) data.
  • Finite-temperature molecular dynamics simulations.

Main Results:

  • MLIPs accurately reproduced experimental INS spectra across 0-1200 cm-1 at both atmospheric pressure and 1.5 GPa.
  • MLIPs remained stable in molecular dynamics simulations at 300 K.
  • The models successfully captured pressure-induced spectral shifts, including blue shifts from steric effects and an anomalous red shift due to intermolecular interactions.

Conclusions:

  • Pressure-dependent INS serves as a practical experimental method for validating MLIPs.
  • This technique assesses not only equilibrium structure but also the pressure-dependent potential energy surface.
  • High-pressure INS is essential for establishing the transferability and reliability of MLIPs for molecular materials.