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相关论文: Astronomical masers and Dicke's superradiance

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We derive relativistic Maxwell-Bloch equations for potential applications in astronomical environments, where various radiative processes are known to occur, including the maser action and Dicke's superradiance. We show that for both…

量子物理 · 物理学 2026-04-15 Ningyan Fang , Victor Botez , Fereshteh Rajabi , Martin Houde

We present a comprehensive analysis of the periodic flares observed in the 6.7 GHz methanol transition in G22.356+0.066, utilizing the Maxwell-Bloch equations (MBEs) as a framework to model these phenomena. By solving the one-dimensional…

高能天体物理现象 · 物理学 2024-09-17 T. Rashidi , V. Anari , A. Bartkiewicz , P. Wolak , M. Szymczak , F. Rajabi

A change in the character of maser generation in a two-level system is found when the initial population inversion exceeds some threshold value proportional to the square root of the total number of atoms. Above this threshold, the number…

量子物理 · 物理学 2016-10-18 A. V. Kirichok , V. M. Kuklin , A. G. Zagorodny

We discuss the role that coherence phenomena can have on the intensity variability of spectral lines associated with maser radiation. We do so by introducing the fundamental cooperative radiation phenomenon of (Dicke's) superradiance and…

We report a time-resolved study of collective emission in dense ensembles of two-level atoms. We compare, on the same sample, the build-up of superradiance and subradiance from the ensemble when driven by a strong laser. This allows us to…

量子物理 · 物理学 2022-04-06 Antoine Glicenstein , Giovanni Ferioli , Antoine Browaeys , Igor Ferrier-Barbut

We have applied the concept of superradiance introduced by Dicke in 1954 to astrophysics by extending the corresponding analysis to the magnetic dipole interaction characterizing the atomic hydrogen 21 cm line. Although it is unlikely that…

星系天体物理 · 物理学 2016-08-17 Fereshteh Rajabi , Martin Houde

Collective emission behavior is usually described by the decay dynamics of the completely symmetric Dicke states. To study a more realistic scenario, we investigate alternative initial states inducing a more complex time evolution.…

量子物理 · 物理学 2021-04-21 Sebastian Fuchs , András Vukics , Stefan Yoshi Buhmann

We present new evidence for superradiance in the methanol 6.7 GHz spectral line for three different star-forming regions: S255IR-NIRS3, G24.329+0.144, and Cepheus A. Our analysis shows that some of the intensity flares exhibiting fast flux…

星系天体物理 · 物理学 2019-01-23 F. Rajabi , M. Houde , A. Bartkiewicz , M. Olech , M. Szymczak , P. Wolak

In this paper we re-analyse the amplification process of broadband continuum radiation by astronomical masers in one-dimensional case. The basic equations appropriate for the scalar maser and the random nature of the maser radiation field…

星系天体物理 · 物理学 2015-05-13 Dinh-V-Trung

We derive analytical results for various quantities related to the excited-state quantum phase transitions in a class of Dicke superradiance models in the semiclassical limit. Based on a calculation of a partition sum restricted to Dicke…

统计力学 · 物理学 2013-10-22 Tobias Brandes

We investigate the possibility of a Dicke-type superradiant phase transition of an atomic gas with an extended model which takes into account the short-range depolarizing interactions between atoms approaching each other as close as the…

量子物理 · 物理学 2016-09-13 Tobias Grießer , András Vukics , Peter Domokos

We apply Dicke's theory of superradiance introduced in 1954 to the methanol 6.7 GHz and water 22 GHz spectral lines, often detected in molecular clouds as signposts for the early stages of the star formation process. We suggest that…

星系天体物理 · 物理学 2017-04-06 Fereshteh Rajabi , Martin Houde

We report the experimental observation of superradiant emission emanating from an elongated dense ensemble of laser cooled two-level atoms, with a radial extent smaller than the transition wavelength. In the presence of a strong driving…

原子物理 · 物理学 2021-12-22 G. Ferioli , A. Glicenstein , F. Robicheaux , R. T. Sutherland , A. Browaeys , I. Ferrier-Barbut

We study systems of particles on a line which have a maximum, are locally finite and evolve with independent increments. ``Quasi-stationary states'' are defined as probability measures, on the \sigma-algebra generated by the gap variables,…

概率论 · 数学 2007-05-23 Anastasia Ruzmaikina , Michael Aizenman

Dicke superradiance describes the collective radiative decay of a fully inverted ensemble of two-level atoms. We experimentally investigate this effect for a chiral, i.e.,~direction-dependent light--matter coupling. Despite a fundamentally…

In recent years there have been significant advances in the study of many-body interactions between atoms and light confined to optical cavities. One model which has received widespread attention of late is the Dicke model, which under…

量子物理 · 物理学 2020-07-28 Kevin Stitely , Andrus Giraldo , Bernd Krauskopf , Scott Parkins

We analyze the stability of super- and subradiant states in a system of identical two-level atoms in the near-Dicke limit, i.e., when the atoms are very close to each other compared to the wavelength of resonant light. The dynamics of the…

量子物理 · 物理学 2008-11-20 Peter G. Brooke , Karl-Peter Marzlin , James D. Cresser , Barry C. Sanders

In this paper we will look at the phenomenon of Microwave Amplification by Stimulated Emission of Radiation (a maser system). We begin by deriving amplification by stimulated emission using time-dependent perturbation theory, in which the…

星系天体物理 · 物理学 2013-12-10 Eric S. Gentry

Dicke superradiance describes an ensemble of $N$ permutationally invariant two-level systems collectively emitting radiation with a peak radiated intensity scaling as $N^2$. Although individual Dicke states are typically entangled, the…

量子物理 · 物理学 2026-03-27 Nico S. Bassler

Dicke superradiance is essentially a case of correlated dissipation leading to the macroscopic quantum coherence. Superradiance for arrays of inverted emitters in free space requires interactions far beyond the nearest-neighbor, limiting…

光学 · 物理学 2025-09-17 Jun Ren , Shicheng Zhu , Z. D. Wang
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