Congratulations to PhD candidate Leo Kim, postdoc Melissa Diamond, and professor Joe Bramante who recently had their paper accepted by the Physical Review Letters (PRL). The paper also has been selected to be featured as an Editor’s Choice in the April publication.

 

A novel way to search for puffed-up clouds of dark matter

Dark matter being a lampshade for stars

Left: A compact object microlensing light from a star, causing a star to appear brighter. Middle: A puffy dark matter cloud which is no longer compact enough to produce a microlensing effect. Right: A puffy dark matter cloud acting as a lampshade, causing starlight to dim due to interactions between photons from the star and constituent dark matter particles in the lampshade.

Physicists at Queen’s have found a new way to search for puffed-up clouds of dark matter by looking to see if stars "wink" in the night sky. Despite making up 85% of the matter content in the Universe, the true nature of dark matter remains a mystery. In some models, the dark matter particles can form large clumps. A prominent way to look for them is through microlensing, an effect where a dark clump can gravitationally bend the light from a star it passes in front of, briefly increasing the starlight received at a telescope. However, this phenomenon no longer works if the dark matter clump is too large. In this letter, the authors showed that for these "puffy" dark matter clouds, they can instead dim starlight, similar to how a regular lampshade dims a lightbulb. These "lampshade" dark matter clumps can be searched for in the already-existing microlensing data sets, and can be used to constrain and differentiate between candidates for dark matter.

 

Paper to be published on April 8, 2025: Dimming starlight with dark compact objects.

 

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