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IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

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When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
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IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration01:16

IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration

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A covalently bonded heteronuclear diatomic molecule can be modeled as two vibrating masses connected by a spring. The vibrational frequency of the bond can be expressed using an equation derived from Hooke's law, which describes how the force applied to stretch or compress a spring is proportional to the displacement of the spring. In this case, the atoms behave like masses, and the bond acts like a spring.
According to Hooke's law, the vibrational frequency is directly proportional to...
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IR Spectrum Peak Broadening: Hydrogen Bonding01:23

IR Spectrum Peak Broadening: Hydrogen Bonding

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The vibrational frequency of a bond is directly proportional to its bond strength. As a result, stronger bonds vibrate at higher frequencies, while weaker bonds vibrate at lower frequencies. The stretching vibration of the strong O–H bond in alcohols and phenols (very dilute solution or gas phase) appears as a sharp peak at 3600–3650 cm−1.
However, the extent of hydrogen bonding influences the observed stretching frequency and band broadening. Intermolecular or intramolecular...
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Emission Spectra02:39

Emission Spectra

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When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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UV–Vis Spectroscopy: Molecular Electronic Transitions01:16

UV–Vis Spectroscopy: Molecular Electronic Transitions

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In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this...
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Molecular Spectroscopy: Absorption and Emission01:14

Molecular Spectroscopy: Absorption and Emission

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Molecules possess discrete energy levels called quantum states. Unlike atoms, which have simpler energy levels, molecules possess additional rotational and vibrational energy levels.  Each energy level is separated by an energy gap, with the gaps between adjacent electronic, vibrational, and rotational levels varying significantly. The three types of energy levels in a diatomic molecule are shown in Figure 1.
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  1. Home
  2. First Principles Rovibronic Absorption Spectra Of Hf Molecule.
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  2. First Principles Rovibronic Absorption Spectra Of Hf Molecule.

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First Principles Rovibronic Absorption Spectra of HF Molecule.

Nariman Abu El Kher1, Maha Shibli2, Mahmoud Korek2

  • 1Department of Physics, Khalifa University, Abu Dhabi, UAE.

Journal of Computational Chemistry
|February 24, 2026

View abstract on PubMed

Summary
This summary is machine-generated.

This study presents a detailed spectroscopic analysis of the hydrogen fluoride (HF) molecule using advanced computational methods. The generated line lists and simulated spectra provide crucial data for understanding HF in astrophysical environments.

Keywords:
ab initio calculationsline listsradiative lifetimerovibronic spectrumspectroscopic model

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Area of Science:

  • Quantum Chemistry and Spectroscopy
  • Computational Physics
  • Astrophysical Chemistry

Background:

  • Accurate spectroscopic data for molecules like hydrogen fluoride (HF) are essential for interpreting observations in various astrophysical environments.
  • Previous experimental data for HF rovibronic spectroscopy is limited, necessitating theoretical calculations to fill the gap.
  • Understanding the electronic structure and nuclear motion of diatomic molecules is fundamental to molecular spectroscopy.

Purpose of the Study:

  • To perform an ab initio study of the rovibronic spectroscopy of the hydrogen fluoride (HF) molecule.
  • To generate comprehensive line lists for the B 1Σ+–X 1Σ+ and C 1Π–X 1Σ+ band systems of HF.
  • To simulate temperature-dependent rovibronic absorption cross sections and compare them with experimental data.

Main Methods:

  • High-level electronic structure computations were employed to determine the potential energy surfaces.
  • Accurate calculations of the Schrödinger equation for nuclear motion were performed.
  • A combination of empirical and ab initio methods was used to construct the spectroscopic model and line lists.

Main Results:

  • Generated line lists covering the B 1Σ+–X 1Σ+ and C 1Π–X 1Σ+ band systems of HF.
  • Simulated temperature-dependent rovibronic absorption cross sections, showing good agreement with available experimental data.
  • Calculated radiative lifetimes for the B and C states, consistent with previous theoretical and experimental results.

Conclusions:

  • The developed spectroscopic model and line lists for HF are reliable and validated against experimental data.
  • The generated data can be used for spectroscopic modeling of HF in interstellar space and planetary atmospheres.
  • This work provides essential data for the interpretation of astronomical observations involving hydrogen fluoride.