Gravitational Lensing and Microlensing in Clusters: Clusters as Dark Matter Telescopes

TL;DR

This paper discusses how galaxy clusters act as natural gravitational telescopes, magnifying distant galaxies and enabling the study of the early universe, while also exploring microlensing events in globular clusters to detect planets and black holes.

Contribution

It proposes utilizing galaxy clusters as dark matter telescopes for high-redshift galaxy observation and continuing microlensing surveys to detect planets and intermediate-mass black holes.

Findings

Clusters significantly magnify distant galaxies, revealing objects from the Dark Ages.

Lensing boosts enable detection of otherwise faint high-redshift galaxies.

Microlensing surveys can identify planets and intermediate-mass black holes.

Abstract

Gravitational lensing is brightening of background objects due to deflection of light by foreground sources. Rich clusters of galaxies are very effective lenses because they are centrally concentrated. Such natural Gravitational Telescopes provide us with strongly magnified galaxies at high redshifts otherwise too faint to be detected or analyzed. With a lensing boost, we can study galaxies shining at the end of the `Dark Ages'. We propose to exploit the opportunity provided by the large field of view and depth, to search for sources magnified by foreground clusters in the vicinity of the cluster critical curves, where enhancements can be of several tens in brightness. Another aspect is microlensing (ML), where we would like to continue our survey of a number of Galactic globular clusters over time-scales of weeks to years to search for ML events from planets to hypothesized central intermediate-mass black holes (IMBH).