6 papers · 1 filter
The very local Hubble flow: Simulating transition from chaos to order
A. D. Chernin, I. D. Karachentsev, M. J. Valtonen +3
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…
Cosmic internal symmetry in a finite universe
Arthur D. Chernin
Cosmic internal symmetry (COINS) relates cosmic vacuum, dark matter, baryons and radiation, in a finite universe. Evidence for COINS comes from the concordance data, including the…
The Hubble Flow Why Does the Cosmological Expansion Preserve its Kinematical Identity from a Few MPC Distance to the Observation Horizon?
Igor D. Karachentsev, Arthur D. Chernin, Pekka Teerikorpi
The problem of the physical nature of the Hubble flow in the Local Volume ( Mpc) stated by Sandage(1986, 1999) is studied. New observational data on galaxy motions and matt…
The Friedmann integrals and physical vacuum in the framework of macroscopic extra dimensions
A. D. Chernin
The structure and origin of the Friedmann integrals are analyzed within the framework of large extra dimensions proposed by Arkani-Hamed et all. (1998). It is demonstrated that the…
Discovering internal symmetry in cosmology
Arthur D. Chernin
Internal (non-geometric) symmetry is recognized and studied as a new phenomenon in cosmology. Symmetry relates cosmic vacuum to non-vacuum forms of cosmic energies, which are dark…
Why is the Hubble flow so quiet?
Arthur Chernin, Pekka Teerikorpi, Yurij Baryshev
The cosmological vacuum, which is perfectly uniform, dominates by density over all the forms of cosmic matter. It makes the Universe be actually more uniform than it could be seen…