Fulltext

The signature of dark energy on the local Hubble flow

Macciò, Andrea V. ; Governato, Fabio ; Horellou, Cathy

In: Monthly Notices of the Royal Astronomical Society, 2005, vol. 359, no. 3, p. 941-948

Zum persönliche Liste hinzufügen
    Titel
    • The signature of dark energy on the local Hubble flow
    Autor
    • Macciò, Andrea V.. Institute for Theoretical Physics, University of Zürich, CH-8057 Zürich, Switzerland
    • Governato, Fabio. Department of Astronomy, University of Washington, Seattle, WA 98195, USA
    • Horellou, Cathy. Onsala Space Observatory, Chalmers University of Technology, SE-43992 Onsala, Sweden
    Dokumententyp
    • Postprint
    Sprache
    • Englisch
    Veröffentlicht in
    • Monthly Notices of the Royal Astronomical Society, 2005, vol. 359, no. 3, p. 941-948. Blackwell Science Ltd
    Andere elektronische Ausgabe
    OAI-PMH-ID
    • oai:doc.rero.ch:299748
    Summary
    Using N-body simulations of flat, dark energy-dominated cosmologies, we show that galaxies around simulated binary systems resembling the Local Group (LG) have low peculiar velocities, in good agreement with observational data. We have compared results for LG-like systems selected from large, high-resolution simulations of three cosmologies: a ΛCDM model, a ΛWDM model with a 2-keV warm dark matter candidate, and a quintessence (QCDM) model with an equation-of-state parameter w=−0.6. The Hubble flow is significantly colder around LGs selected in a flat, Λ-dominated cosmology than around LGs in open or critical models, showing that a dark energy component manifests itself on the scales of nearby galaxies, cooling galaxy peculiar motions. Flows in the ΛWDM and QCDM models are marginally colder than in the ΛCDM one. The results of our simulations have been compared to existing data and to a new data set of 28 nearby galaxies with robust distance measures (Cepheids and surface brightness fluctuations). The measured line-of-sight velocity dispersion is given by σH= (88 ± 20 km s−1) × (R/7 Mpc). The best agreement with observations is found for LGs selected in the ΛCDM cosmology in environments with −0.1 < δρ/ρ < 0.6 on scales of 7 Mpc, in agreement with existing observational estimates on the local matter density. These results provide new, independent evidence for the presence of dark energy on scales of a few megaparsecs, corroborating the evidence gathered from observations of distant objects and the early Universe