Unified approach to redshift in cosmological /black hole spacetimes and synchronous frame A. V. Toporensky Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect, 13, Moscow 119991, Russia and Kazan Federal University, Kremlevskaya 18, Kazan 420008, Russia∗ O. B. Zaslavskii Department of Physics and Technology, Kharkov V.N. Karazin National University, 4 Svoboda Square, Kharkov 61022, Ukraine and Kazan Federal University, Kremlevskaya 18, Kazan 420008 Russia† S. B. Popov Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky Prospect, 13, Moscow 119991, Russia Usually, interpretation of redshift in static spacetimes (for example, near black holes) is opposed to that in cosmology. In this methodological note we show that both explanations are unified in a natural picture. This is achieved if, considering the static spacetime, one (i) makes a transition to a synchronous frame, and (ii) returns to the original frame by means of local Lorentz boost. To reach our goal, we consider arXiv:1704.08308v3 [gr-qc] 1 Mar 2018 a rather general class of spherically symmetric spacetimes. In doing so, we construct frames that generalize the well-known Lemaitre and Painlev´e–Gullstand ones and elucidate the relation between them. This helps us to understand, in an unifying approach, how gravitation reveals itself in different branches of general relativity. This framework can be useful for general relativity university courses. PACS numbers: 04.20.-q; 04.20.Cv; 04.70.Bw ∗Electronic address:
[email protected] †Electronic address:
[email protected] 2 I. INTRODUCTION Though the calculation of redshifts in General Relativity (GR) has no principal diffi- culties, their interpretation continues to be a source of debates.