Unveiling the Properties of Dark Compact Objects Through Gravitational Lensing

Friday 28 February 2025


The mysteries of dark matter and compact objects have long fascinated astronomers, but a recent study sheds new light on these enigmatic entities. Researchers have been studying the gravitational lensing effects of two strongly lensed supernovae, iPTF16geu and SN Zwicky, to better understand the properties of these objects.


Gravitational lensing occurs when the light from a distant object passes near a massive object, such as a galaxy or star, bending its trajectory. This phenomenon allows astronomers to study the mass distribution within these objects in great detail. In the case of iPTF16geu and SN Zwicky, their light is being bent by the gravitational fields of foreground galaxies.


The researchers used a combination of observations from various telescopes, including the Hubble Space Telescope, to analyze the lensing effects on both supernovae. They employed a novel technique called microlensing, which involves modeling the small-scale fluctuations in the mass distribution within these galaxies. This allowed them to constrain the properties of dark compact objects, such as their mass and density.


The study revealed that the dark compact objects are likely to be made up of normal matter, rather than exotic particles. The researchers also found that the fraction of dark compact objects in these galaxies is relatively small, with an upper limit of 0.19 (95%). This suggests that dark compact objects may not play a significant role in shaping the large-scale structure of the universe.


The findings of this study have important implications for our understanding of galaxy evolution and the nature of dark matter. By studying the lensing effects on multiple supernovae, astronomers can gain insights into the properties of these mysterious objects. This research also highlights the power of gravitational lensing as a tool for probing the internal structure of galaxies.


The authors used a combination of observations from various telescopes, including the Hubble Space Telescope, to analyze the lensing effects on both supernovae. They employed a novel technique called microlensing, which involves modeling the small-scale fluctuations in the mass distribution within these galaxies.


Cite this article: “Unveiling the Properties of Dark Compact Objects Through Gravitational Lensing”, The Science Archive, 2025.


Dark Matter, Compact Objects, Gravitational Lensing, Supernovae, Iptf16Geu, Sn Zwicky, Hubble Space Telescope, Microlensing, Galaxy Evolution, Normal Matter


Reference: Nikki Arendse, Edvard Mörtsell, Luke Weisenbach, Erin Hayes, Stephen Thorp, Suhail Dhawan, Ariel Goobar, Sacha Guerrini, Jacob Osman Hjortlund, Joel Johansson, et al., “Microlensing of lensed supernovae Zwicky & iPTF16geu: constraints on the lens galaxy mass slope and dark compact object fraction” (2025).


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