Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes

A moving mass makes a gravitational wake in the partially ionized interstellar medium, which acts as a lens for radio-frequency light. Consequently, plasma microlensing could complement gravitational microlensing in the search for invisible massive objects, such as stellar remnants or compact dark m...

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Main Author: M. Sten Delos
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad96b1
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author M. Sten Delos
author_facet M. Sten Delos
author_sort M. Sten Delos
collection DOAJ
description A moving mass makes a gravitational wake in the partially ionized interstellar medium, which acts as a lens for radio-frequency light. Consequently, plasma microlensing could complement gravitational microlensing in the search for invisible massive objects, such as stellar remnants or compact dark matter. This work explores the spatial structure of the plasma lens associated with a gravitational wake. Far away from the moving mass, the characteristic lensing signal is the steady demagnification or magnification of a radio source as the wake passes in front of it at the speed of sound. Sources can be plasma-lensed at a much greater angular distance than they could be gravitationally lensed to the same degree by the same object. However, only the wakes of objects greatly exceeding stellar mass are expected to dominate over the random turbulence in the interstellar medium.
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spelling doaj-art-1a89298c037d4ae7a3b63d2bb60f2e722025-08-20T01:57:24ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-0197817110.3847/1538-4357/ad96b1Detecting Dark Objects with Plasma Microlensing by Their Gravitational WakesM. Sten Delos0https://orcid.org/0000-0003-3808-5321Carnegie Observatories , 813 Santa Barbara Street, Pasadena, CA 91101, USA ; mdelos@carnegiescience.eduA moving mass makes a gravitational wake in the partially ionized interstellar medium, which acts as a lens for radio-frequency light. Consequently, plasma microlensing could complement gravitational microlensing in the search for invisible massive objects, such as stellar remnants or compact dark matter. This work explores the spatial structure of the plasma lens associated with a gravitational wake. Far away from the moving mass, the characteristic lensing signal is the steady demagnification or magnification of a radio source as the wake passes in front of it at the speed of sound. Sources can be plasma-lensed at a much greater angular distance than they could be gravitationally lensed to the same degree by the same object. However, only the wakes of objects greatly exceeding stellar mass are expected to dominate over the random turbulence in the interstellar medium.https://doi.org/10.3847/1538-4357/ad96b1Interstellar mediumDark matterBlack holesInterstellar scintillationAstrophysical fluid dynamicsAnalytical mathematics
spellingShingle M. Sten Delos
Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes
The Astrophysical Journal
Interstellar medium
Dark matter
Black holes
Interstellar scintillation
Astrophysical fluid dynamics
Analytical mathematics
title Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes
title_full Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes
title_fullStr Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes
title_full_unstemmed Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes
title_short Detecting Dark Objects with Plasma Microlensing by Their Gravitational Wakes
title_sort detecting dark objects with plasma microlensing by their gravitational wakes
topic Interstellar medium
Dark matter
Black holes
Interstellar scintillation
Astrophysical fluid dynamics
Analytical mathematics
url https://doi.org/10.3847/1538-4357/ad96b1
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