Probing the integrated Sachs-Wolfe effect using embedded lens models
Bin Chen, Ronald Kantowski

TL;DR
This paper introduces embedded lens models using Fermat potential formalism to explain the observed ringed temperature structures in the ISW effect around cosmic voids, aligning with recent Planck observations.
Contribution
It develops a novel embedded lens theory and models for the ISW effect, providing a better understanding of the temperature rings observed around cosmic voids.
Findings
Models produce hot rings around cold void centers
Adding central over-density matches positive temperature excess
Embedded lens theory effectively models ISW effects
Abstract
The photometry profile of the integrated Sachs-Wolfe (ISW) effect recently obtained by the Planck consortium by stacking patches of Cosmic Microwave Background (CMB) sky maps around a large number of cosmic voids, contains a cold ring at about half the void's effective radius surrounded by a hot ring near the void's boundary. The source of the temperature structure is assumed to be the ISW effect but the exact cause of the ringed structure is not currently well understood, particularly the outer hot ring. Numerical simulations have suggested that hot/cold ring structures can be produced by motions associated with nonlinear growths of cosmic structures whose gravitational potentials produce the ISW effect. We have recently developed the embedded lens theory and the Fermat potential formalism which can be used to model the ISW effect caused by intervening individual lens inhomogeneities…
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