Superradiance and stimulated scattering in SNR 1987A
Jacques Moret-Bailly

TL;DR
This paper proposes that superradiance and stimulated scattering in the plasma of SNR 1987A explain the observed rings, with intense emission modes and self-accelerating cooling effects shaping the rings' brightness and structure.
Contribution
It introduces a novel model linking superradiance and stimulated scattering to the formation and brightness of the rings in SNR 1987A.
Findings
Superradiance occurs in high column density plasma at specific temperatures.
The model explains the elliptical shapes and pearls in the rings.
Energy transfer from star rays to rings is highly efficient.
Abstract
The rings observed around supernova remnant 1987A are emitted by a plasma mainly made of ionized and neutral hydrogen atoms. With a density of 10 power 10 atoms per cubic metre, and at least a dimension of plasma of 0.01 light-year, the column density is 10 power 24 atoms per square metre, much more than needed for an optically thick gas at Lyman frequencies (Case B). While, at 10000 K, the bulky gas would absorb Lyman lines fully, at 50000K it emits superradiant lines. As superradiance de-excites the atoms strongly, nearly all available energy is emitted in a few competing modes: Superradiance appears only for beams which cross the largest column densities; for an observation from Earth, these beams generate three elliptical hollow cylinders whose bases are the observed rings; admitting that the Earth is not in a privileged direction, these cylinders envelope ellipsoidal shells…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Gamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena
