期刊
NATURE ASTRONOMY
卷 3, 期 3, 页码 272-277出版社
NATURE RESEARCH
DOI: 10.1038/s41550-018-0657-z
关键词
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资金
- ASI-INAF [2017-14-H.0]
- European Union COFUND/Durham Junior Research Fellowship [609412]
- Alfred P. Sloan Foundation
- National Science Foundation
- United States Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
- American Museum of Natural History
- Astrophysical Institute Potsdam
- University of Basel
- University of Cambridge
- Case Western Reserve University
- University of Chicago
- Drexel University
- Fermilab
- Institute for Advanced Study
- Japan Participation Group
- Johns Hopkins University
- Joint Institute for Nuclear Astrophysics
- Kavli Institute for Particle Astrophysics and Cosmology
- Korean Scientist Group
- Chinese Academy of Sciences (LAMOST)
- Los Alamos National Laboratory
- Max Planck Institute for Astronomy (MPIA)
- Max Planck Institute for Astrophysics (MPA)
- New Mexico State University
- Ohio State University
- University of Pittsburgh
- University of Portsmouth
- Princeton University
- United States Naval Observatory
- University of Washington
- US Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- French Participation Group
- German Participation Group
- Harvard University
- Instituto de Astrofisica de Canarias
- Michigan State/Notre Dame/JINA Participation Group
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- New York University
- Pennsylvania State University
- Spanish Participation Group
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- Yale University
The concordance model (Lambda cold dark matter (Lambda CDM) model, where Lambda is the cosmological constant) reproduces the main current cosmological observations(1-4) assuming the validity of general relativity at all scales and epochs and the presence of CDM and of Lambda, equivalent to dark energy with a constant density in space and time. However, the Lambda CDM model is poorly tested in the redshift interval between the farthest observed type Ia supernovae(5) and the cosmic microwave background. We present measurements of the expansion rate of the Universe based on a Hubble diagram of quasars. Quasars are the most luminous persistent sources in the Universe, observed up to redshifts of z approximate to 7.5 (refs. (6,7)). We estimate their distances following a method developed by our group(8-10), based on the X-ray and ultraviolet emission of the quasars. The distance modulus/redshift relation of quasars at z < 1.4 is in agreement with that of supernovae and with the concordance model. However, a deviation from the Lambda CDM model emerges at higher redshift, with a statistical significance of similar to 4 sigma. If an evolution of the dark energy equation of state is allowed, the data suggest dark energy density increasing with time.
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