A Step Closer to Dark Energy
The first cosmological analysis of joint X-ray and optical weak-lensing data from more than 500 galaxy clusters paves the way for future research on larger datasets
Image caption: Three eFEDS clusters are shown across the panels from left to right. The top (bottom) row shows the X-ray (optical) imaging of the cluster observed by the eROSITA telescope (HSC survey). The cluster name, mass, and the redshift are labeled in the optical imaging on the bottom row. By combining optical and X-ray imaging, we can efficiently search for galaxy clusters and measure their masses at the same time.
Image courtesy: Dr. Matthias Klein.
In the late 20th century, the observation of a type one-A supernova led to the discovery of accelerating expansion of our universe. Up until now, however, scientists have not been able to fathom the energy driving this acceleration. Referred to as “Dark Energy,” this mysterious energy behaves like “anti-gravity,” pushing objects away from each other. Fortunately, the effects of this Dark Energy can be analyzed by focusing on the number and distribution of galaxy clusters, which are the largest objects in the known universe.
Galaxy clusters are, however, uncommon and locating them requires scanning a significant portion of the sky with extremely sophisticated telescopes. One such telescope, the eROSITA X-ray space telescope, launched in 2019 by the Max Planck Institute for Extraterrestrial Physics in Germany, is set to carry out the deepest full-sky survey in X-rays. Nonetheless, a dataset from a mini-survey called the eROSITA Final Equatorial Depth Survey (eFEDS), containing a sample of about 550 galaxy clusters, has already been published.
Against this backdrop, research group led by Professor I-Non Chiu from National Cheng Kung University (NCKU), Taiwan decided to conduct the first cosmological study on the eFEDS data, which also serves as the first cosmological study on galaxy clusters identified by eROSITA. Their paper was published in Volume 522, Issue 2 of Monthly Notices of the Royal Astronomical Society on April 21, 2023.
In this first-ever synergistic study combining data from X-ray and optical surveys, the researchers combined the eFEDS X-ray data with state-of-the-art optical data from the Hyper Suprime-Cam Subaru Strategic Program led by Taiwan, Japan, and Princeton University, USA. To reduce contamination (noise), the team first built a galaxy cluster sample using the X-ray telescope data. They then further cleaned this sample using optical data and estimated the clusters’ masses to perform cosmological calculations.
Comparing their results with theoretical predictions, the researchers found that Dark Energy occupies up to 76% of the total energy density in the universe. Additionally, the equation of state of Dark Energy described the relationship between its pressure and energy density, as well as the constraints on Dark Energy.
Prof. Chiu explains, “Based on our results, the energy density of Dark Energy appears to be uniform in space and constant in time, resembling a true constant in the Universe, and in good agreement with other independent experiments.” Indeed, observational evidence from the study suggests that Dark Energy can be described by a simple constant, namely the cosmological constant Λ.
Highlighting the need for larger datasets, Prof. Chiu says, “Future studies using the full-sky sample will significantly improve our understanding of Dark Energy. Our study has laid a solid foundation for subsequent works towards this goal.” The researchers anticipate that faster computational approaches will be required in the future, given the massive increase in data size a full-sky survey will entail, and are already taking this into consideration.
We certainly hope that the eROSITA survey will help clarify one of the deepest mysteries of the cosmos!
ReferenceTitle of original paper
Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
Monthly Notices of the Royal Astronomical Society