Dark energy

The Euclid Space Telescope blasting off atop a Falcon 9 rocket (Image courtesy SpaceX)

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A little while ago, ESA’s Euclid Space Telescope was launched atop a SpaceX Falcon 9 rocket from Cape Canaveral. After just over 40 minutes, it successfully separated from the rocket’s last stage and entered its course that will take it towards the so-called L2 point, about 1.5 million kilometers from Earth, where its scientific mission will begin with an investigation of the dark universe.

The Euclid Space Telescope mission is focused on the cosmological mysteries connected to dark matter and dark energy. Cosmological research in recent decades indicates that the universe we see with the ordinary matter that forms galaxies constitutes only a small part of the cosmos. Astronomers and physicists are having difficulty investigating parts of the cosmos that we can neither see nor directly detect. It’s a problem that makes it difficult to test models that try to explain the effects that led to hypothesize the existence of dark matter and dark energy. For this reason, ESA developed a scientific mission focused on these cosmological problems.

Deep field image (Image Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA Acknowledgments: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani (NSF’s NOIRLab) & D. de Martin (NSF’s NOIRLab))

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29 articles report various aspects of the results of a major cosmological research on the largest sample of galaxies – 226 million of them – ever observed to produce the most accurate measurements of the composition and growth of the universe. More than 400 scientists from the DES (Dark Energy Survey) Collaboration used images captured by the Dark Energy Camera in the first three years of the program, which started in 2013, to obtain results. The goal is to improve our knowledge of the universe, in particular, the nature of dark matter and dark energy.

The extent of the expansion of the universe is increasingly precise and stresses the discrepancy between the measurements

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An article published in “The Astrophysical Journal” reports a new measurement of the expansion of the universe, which is approximately 9% faster than the estimates made by studying the early universe. A team of astronomers led by Nobel laureate Adam Riess combined observations made with the Hubble Space Telescope of 70 variable stars called Cepheid variables used for measurements with others conducted by the Araucaria project to obtain extremely precise measurements of their brightness. The discrepancy between the measurements of the expansion of the near universe and those of the early universe remains and it’s important to improve the measurements to obtain clues to the origin of the discrepancy.

A measurement of the Hubble constant based on quasars suggests possible changes to cosmological models

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An article published in the journal “Nature Astronomy” describes the use of quasars as cosmic tracers to measure the expansion of the universe up to 12 billion years ago. Guido Risaliti of the University of Florence and Elisabeta Lusso of Durham University studied the X-ray and optical emissions of a number of quasars using the comparison between those emissions to accurately assess their distances. The results could explain the discrepancies between the different measurements carried out with other methods suggesting that the density of the mysterious dark energy isn’t constant over time.

Artist's concept of the universe on a 5D bubble (Image courtesy Suvendu Giri)

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An article published in the journal “Physical Review Letters” describes a new model of the universe that proposes that it exists on the edge of an expanding bubble in a five-dimension space-time. A team of researchers from the Swedish University of Uppsala used string theory to hypothesize that the matter existing in the universe is accomodated at the edges of strings that extend into the fifth dimension. According to this hypothesis, what is called dark energy is an effect described by a cosmological constant in the four-dimension Friedmann equations.