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Atomic Nuclei: Nuclear Relaxation Processes01:23

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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 Population Distribution01:14

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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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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.
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Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
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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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Multitemperature atomic ensemble: Nonequilibrium evolution after ultrafast electronic excitation.

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Area of Science:

  • Condensed matter physics
  • Materials science
  • Physical chemistry

Background:

  • Ultrafast laser radiation and particle beams excite electronic systems in solids, leading to transient thermal non-equilibrium.
  • Both electronic and atomic subsystems can exist far from equilibrium during this process.

Purpose of the Study:

  • To define atomic temperatures in electronically excited solids from first principles.
  • To investigate the behavior of atomic temperatures during non-thermal phase transitions induced by electronic excitation.
  • To propose a formulation for multitemperature heat transport equations.

Main Methods:

  • Derivation of atomic temperature definitions for excited ensembles.
  • Analysis of kinetic temperature in the momentum subspace.
  • Proposal and application of configurational atomic temperature for electronic-temperature-dependent interatomic potentials, including ab initio molecular dynamics.
  • Study of temperature evolution during non-thermal phase transitions.

Main Results:

  • The kinetic temperature of atoms in the momentum subspace remains unaffected by electronic excitation.
  • A configurational atomic temperature is defined for situations where electronic and atomic temperatures differ.
  • Solids under ultrafast irradiation exhibit a temporary multitemperature state with distinct momentum and configurational equilibria.
  • Complete equilibration of atomic temperatures occurs over longer timescales, leading to energy equipartition.

Conclusions:

  • The study provides a theoretical framework for understanding atomic temperatures in non-equilibrium excited solids.
  • The proposed configurational temperature is crucial for simulations like ab initio molecular dynamics under electronic excitation.
  • The identification of a temporary multitemperature state necessitates the development of advanced heat transport models.