Export citation

Export citation

Choose format for download:

Download Citation

    Initiation of superradiance from different collective-spin states

    Adnan N. Alabbar1,2,*, Zhenghao Zhang1,2, and Girish S. Agarwal1,2,3

    • 1Institute for Quantum Science and Engineering, Texas A&M University, College Station, Texas 77843, USA
    • 2Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
    • 3Department of Biological and Agricultural Engineering, Texas A&M University, College Station, Texas 77843, USA

    • *Contact author: Adnan.alabbar94@tamu.edu

    Phys. Rev. A 114, 033713 – Published 10 September, 2026

    DOI: https://doi.org/10.1103/vrsw-rfwl

    Abstract

    Superradiance is an extensive cooperative spontaneous emission phenomenon, exhibited by some atomic collective-spin states. However, distinct initial states differ in their decay dynamics. Dicke states |j,m〉 with distinct numbers of excitations n=m+j, driven by vacuum fluctuations, have their peak emission intensity shifted in time. Rotating Dicke states relative to the decay axis introduces an interesting parity structure that affects the pulse profile and photon correlations. Squeezed-bath prepared states undergo a squeezing-controlled crossover to the rotated Dicke states, making the emission character dependent on the amount of squeezing transferred from light to the atomic state. For semiclassical states with a macroscopic dipole moment, like the atomic coherent state, the emission intensity depends on their polarization. We present detailed results on the superradiant dynamics of a representative selection of states expanded in Dicke states to highlight the initial state as an independent dynamical control parameter. For large-N, we are able to predict fairly accurately the pulse profile in each case using the mean-field approximation, an approach based on the Fokker-Planck equation. We also present comparative results on the intensity correlation function, quantify the coherent and incoherent contributions of the emission, and contrast between small and large ensembles.

    Physics Subject Headings (PhySH)

    Authorization Required

    We need you to provide your credentials before accessing this content.

    References (Subscription Required)

    Outline

    Information

    Sign In to Your Journals Account

    Filter

    Filter

    Article Lookup

    Enter a citation