Related Experiment Video
Updated: May 7, 2026

05:39
Scalable Quantum Integrated Circuits on Superconducting Two-Dimensional Electron Gas Platform
Published on: August 2, 2019
10.2K
Excited-state quantum phase transitions in Dicke superradiance models
1Institut für Theoretische Physik, Technische Universität Berlin, Hardenbergstraße 36, D-10623 Berlin, Germany.
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|October 16, 2013
Summary
We analyzed quantum phase transitions in Dicke superradiance models. Criticality is energy-dependent, showing similarities to the Lipkin-Meshkov-Glick model.
Area of Science:
- Quantum optics
- Condensed matter physics
- Statistical mechanics
Background:
- Dicke superradiance models exhibit complex quantum phenomena.
- Understanding excited-state quantum phase transitions (ESQPTs) is crucial for quantum systems.
- The semiclassical limit offers insights into macroscopic quantum behaviors.
Purpose of the Study:
- To derive analytical results for ESQPTs in Dicke superradiance models.
- To investigate the semiclassical behavior of these models.
- To identify critical phenomena and their dependencies.
Main Methods:
- Calculation of a partition sum restricted to Dicke states.
- Analysis of the derivative of the density of states.
- Examination of observables like atomic inversion and photon number fluctuations.
Main Results:
- Singular behavior in the density of states derivative was identified.
- Mean atomic inversion and boson number were calculated at arbitrary energies.
- Criticality was found to depend on energy and a parameter controlling rotating/counterrotating terms.
Conclusions:
- The study reveals energy-dependent criticality in Dicke models.
- An analogy was drawn to nonanalyticities observed in the Lipkin-Meshkov-Glick model.
- These findings contribute to understanding quantum phase transitions in open quantum systems.
Related Concept Videos
Deactivation Processes: Jablonski Diagram
2.3K
Luminescence, the emission of light by a substance that has absorbed energy, is a process that involves the interaction of molecules with light. The energy-level diagram, or Jablonski diagram, is a graphical representation of these interactions, illustrating the various states and transitions a molecule can undergo. In a typical Jablonski diagram, the lowest horizontal line represents the ground-state energy of the molecule, which is usually a singlet state. This state represents the energies...
2.3K
Molecular Spectroscopy: Absorption and Emission
4.3K
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.
4.3K
UV–Vis Spectroscopy: Molecular Electronic Transitions
3.0K
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...
3.0K
¹H NMR: Interpreting Distorted and Overlapping Signals
1.3K
Spin systems where the difference in chemical shifts of the coupled nuclei is greater than ten times J are called first-order spin systems. These nuclei are weakly coupled, and their chemical shifts and coupling constant can generally be estimated from the well-separated signals in the spectrum.
As Δν decreases and the signals move closer, the doublets appear increasingly distorted. The intensities of the inner lines increase at the cost of those of the outer lines as the signals are...
As Δν decreases and the signals move closer, the doublets appear increasingly distorted. The intensities of the inner lines increase at the cost of those of the outer lines as the signals are...
1.3K
Phase Transitions
19.1K
Whether solid, liquid, or gas, a substance's state depends on the order and arrangement of its particles (atoms, molecules, or ions). Particles in the solid pack closely together, generally in a pattern. The particles vibrate about their fixed positions but do not move or squeeze past their neighbors. In liquids, although the particles are closely spaced, they are randomly arranged. The position of the particles are not fixed—that is, they are free to move past their neighbors to...
19.1K
Phase Transitions
131
A phase transition is the process in which a substance changes from one state of matter to another, like from a solid to a liquid, liquid to gas, or vice versa, at a specific temperature and under given pressure conditions. This change is spontaneous and is affected by alterations in temperature and pressure. These parameters impact the strength of the forces between molecules (intermolecular forces) in the substance.During a phase transition, both the initial and final phases of the substance...
131

