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

Atomic Nuclei: Types of Nuclear Relaxation01:28

Atomic Nuclei: Types of Nuclear Relaxation

1.1K
Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers...
1.1K
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

1.4K
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.
1.4K
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

2.6K
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.
2.6K
Atomic Spectroscopy: Effects of Temperature01:27

Atomic Spectroscopy: Effects of Temperature

1.1K
Atomization, converting samples into gas-phase atoms and ions, is essential for atomic spectroscopy. The flame temperature required for atomization affects the efficiency of the atomic spectroscopic methods by increasing the atomization efficiency and the relative population of the excited and ground states.
At thermal equilibrium, the relative populations of excited and ground state atoms can be estimated using the Maxwell–Boltzmann distribution. For example, an increase in temperature...
1.1K
Temperature and Thermal Equilibrium01:11

Temperature and Thermal Equilibrium

10.0K
Heat and temperature are essential concepts for everyone every day. The study of heat and temperature is part of an area of physics known as thermodynamics. It is not always easy to distinguish heat and temperature.
The concept of temperature has evolved from the common concepts of hot and cold. The scientific definition of temperature explains more than just our sense of hot and cold. Temperature is operationally defined as the quantity measured with a thermometer. Furthermore, temperature is...
10.0K
Heating and Cooling Curves02:44

Heating and Cooling Curves

28.6K
When a substance—isolated from its environment—is subjected to heat changes, corresponding changes in temperature and phase of the substance is observed; this is graphically represented by heating and cooling curves.
For instance, the addition of heat raises the temperature of a solid; the amount of heat absorbed depends on the heat capacity of the solid (q = mcsolidΔT). According to thermochemistry, the relation between the amount of heat absorbed or released by a substance, q, and its...
28.6K

You might also read

Related Articles

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

Sort by
Same author

Erratum: Density effects on electronic configurations in dense plasmas [Phys. Rev. E 97, 023206 (2018)].

Physical review. E·2026
Same author

Erratum: Carbon ionization from a quantum average-atom model up to gigabar pressures [Phys. Rev. E 104, 025209 (2021)].

Physical review. E·2026
Same author

Erratum: Electron-ion coupling factor for temperature relaxation in dense plasmas [Phys. Rev. E 101, 023206 (2020)].

Physical review. E·2026
Same author

Author Correction: Helioseismic inference of the solar radiative opacity.

Nature communications·2025
Same author

Helioseismic inference of the solar radiative opacity.

Nature communications·2025
Same author

Equivalence between pressure- and structure-defined ionization in hot dense carbon.

Physical review. E·2022

Related Experiment Video

Updated: Mar 24, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
07:17

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

Published on: August 1, 2017

13.3K

Temperature relaxation in dense plasmas.

Gérald Faussurier1, Christophe Blancard1

  • 1CEA, DAM, DIF, F-91297 Arpajon, France.

Physical Review. E
|March 18, 2016
PubMed
Summary

We developed a model for calculating temperature relaxation rates in dense plasmas. This method uses an average-atom model to study electron-ion temperature dynamics in two-temperature systems.

Area of Science:

  • Plasma Physics
  • Computational Physics
  • Thermodynamics

Background:

  • Dense plasmas are crucial in astrophysics and inertial confinement fusion.
  • Understanding temperature relaxation is key to modeling plasma behavior.
  • Existing models may not fully capture complex electron-ion interactions in dense environments.

Purpose of the Study:

  • To introduce a novel model for calculating temperature-relaxation rates in dense plasmas.
  • To investigate electron-ion temperature dynamics within a two-temperature system.
  • To leverage the average-atom model for accurate thermodynamic and interaction potential calculations.

Main Methods:

  • Development of a theoretical model for temperature-relaxation rate calculation.
  • Utilization of an average-atom model to determine electron-ion interaction potentials.

More Related Videos

Trapping of Micro Particles in Nanoplasmonic Optical Lattice
07:20

Trapping of Micro Particles in Nanoplasmonic Optical Lattice

Published on: September 5, 2017

7.0K
Building Langmuir Probes and Emissive Probes for Plasma Potential Measurements in Low Pressure, Low Temperature Plasmas
08:10

Building Langmuir Probes and Emissive Probes for Plasma Potential Measurements in Low Pressure, Low Temperature Plasmas

Published on: May 25, 2021

5.9K

Related Experiment Videos

Last Updated: Mar 24, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
07:17

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

Published on: August 1, 2017

13.3K
Trapping of Micro Particles in Nanoplasmonic Optical Lattice
07:20

Trapping of Micro Particles in Nanoplasmonic Optical Lattice

Published on: September 5, 2017

7.0K
Building Langmuir Probes and Emissive Probes for Plasma Potential Measurements in Low Pressure, Low Temperature Plasmas
08:10

Building Langmuir Probes and Emissive Probes for Plasma Potential Measurements in Low Pressure, Low Temperature Plasmas

Published on: May 25, 2021

5.9K
  • Application of the model to a two-temperature electron-ion plasma system.
  • Main Results:

    • The model successfully calculates temperature-relaxation rates in dense plasmas.
    • The average-atom model provides essential input for thermodynamic properties and interaction potentials.
    • The study enables the analysis of temperature equilibration in complex plasma conditions.

    Conclusions:

    • The presented model offers a robust method for studying temperature relaxation in dense plasmas.
    • The integration of the average-atom model enhances the accuracy of plasma simulations.
    • This work contributes to a better understanding of energy transfer processes in plasmas.