Measurement problem of structural-parametric identification on supernovae type SN Ia for cosmological distances scale of red shift based

Levin S.F.

Moscow Institute for expertise and tests, Department of metrology and metrological support, Moscow, Russia

E-mail: Levin AntoninaEL@rostest.ru

By data, on which basis within the limits of model Friedman–Robertson–Walker the conclusion has been drawn on the beginning of «accelerated expansion of Universe» about 6 billion years ago, the problem of calibration for interpolation models of distances scale with form parameter is solved. According to results of identification at them Doppler interpretations in «Universe expansion» about 2.64–3.18 billion years ago there was pause. The pause was replaced by accelerated expansion which by modern epoch has degenerated in Hubble's stream. On similar data of Sternberg Institute the interpolation model gives practically linear dependence of red shift on photometric distance.

Keywords: cosmological distances scale, interpolation model with form parameter, structurally-parametrical identification, «magnitude standard» of supernovae type SN Ia.

DOI: 10.18698/2309-7604-2015-1-299-310

Article file: Levin1.pdf