The very local Hubble flow: simulating the transition from chaos to order

Details The very local Hubble flow: simulating the transition from chaos to order The very local Hubble flow: simulating the transition from chaos to order

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007a%26a...467..933c&link_type=abstract

Astronomy and Astrophysics, Volume 467, Issue 3, June I 2007, pp.933-941

Astronomy and Astrophysics

Astrophysics

8

Galaxies: Local Group

Scientific paper

The physical nature of the very local (<3 Mpc) Hubble flow is studied on the basis of the recent high-precision observations in the Local Volume. A model including both analytical treatment and computer simulations describes the flow's dynamical evolution from a chaotic Little Bang initial state to the present-day state of a quasi-regular expansion. The dynamical effect of the uniform cosmic vacuum (time-independent dark energy or the cosmological constant) is taken into account.

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