Tornar a resultats destacats 2024

DESI Year 1 results:

Verde, Licia (UB)

Experimental Sciences & Mathematics

The Dark Energy Spectroscopic Instrument (DESI) represents the culmination of multi-years efforts and advanced spectroscopic techniques. Placed at Mayall 4-meter Telescope, DESI harnesses the power of 5,000 robotic fiber positioners, coupled with state-of-the-art spectrographs, to capture the spectral signatures of millions of galaxies and quasars with unprecedented precision. DESI success is also based on the collaborative spirit of its community, more than 400 scientists over 72 institutions. DESI started taking data in 2021 and is planned to observe fora total of 5 years.This data release (DESIY1) and the two sets of results announcements on April 14 and November 19 2024 (accompanied by two press releases) correspond to the first year of observations. In terms of cosmological constraints, DESIY1 surpassed the statistical power of 20 years of observations from the 2.5m Apache point Sloan Telescope that gave us the SDSS (2012), BOSS (2015) and e-BOSS (2021) surveys. DESI data provide unprecedented constraints on cosmological parameters, the expansion history of the Universe, the formation and growth of cosmic structures, the properties of dark energy and the properties of neutrinos. Key parts of the analysis pipeline (in particular the blind analysis strategy, algorithm and procedure, and the improved compressed variables approach "ShapeFit") were developed by my research group.DESIY1 has confirmed many aspects of the standard cosmological model, as well as its major shortcomings, in particular the famous Hubble tension. In addition, DESIY1 has shown tantalising hints that the late-time expansion history of the Universe might not match that expected from observations of the early Universe, which can be interpreted as a possible hint of dynamical dark energy, as non-standard neutrino properties or as a new "tension" in the standard cosmological model, although the statistical significance is still too low to draw definitive conclusions. The tree year data are being actively analysed and a new release is expected in spring 2025. The DESIY1 papers will be published in a special issue of the JCAP journal but are already available open access at the link below.

DESI has made the largest 3D map of our universe to date. Earth is at the center of this thin slice of the full map. In the magnified section, it is easy to see the underlying structure of matter in our universe. Claire Lamman/DESI collaboration; custom colormap package by cmastro

DESI’s Hubble diagram plots a characteristic pattern – baryon acoustic oscillations, or BAO “bubbles” – at different ages of the universe. The amount of dark energy determines how fast the universe grows, and therefore the size of the bubbles. The solid line is how big Lambda CDM predicts the bubbles will be, while the dashed line shows the prediction from a different model where dark energy evolves with time. DESI will gather more data to determine which model is a better description of the universe. (Credit: Arnaud de Mattia/DESI collaboration)

DESI’s measurements of growth of structure evolution at different ages of the universe. The amount of cosmic growth of structure determines how fast dark matter and galaxies are being formed in the universe at a certain time. The dashed black line is how Einstein's General Relativity predicts this structure growth has been, while the coloured lines show the prediction from different models where gravity is weaker or stronger than General Relativity. The current data shows no significant deviation from Einstein's prediction. Credit: Héctor Gil Marín / DESI collaboration