2012
DOI: 10.1007/s10714-012-1495-4
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On the nature of cosmological redshift and spectral shift in Schwarzschild-like and other spacetimes

Abstract: The kinematical nature of the spectral shift in different types of spacetime, cosmological redshift and frequency shift in Schwarzschild spacetime being the most prominent representatives, has been a subject of recent interest. We demonstrate that the kinematical nature of the spectral shift is an inherent feature of the particular type of spacetimes. The general solution is found: necessary and sufficient conditions for the spectral shift arising from a kinematical origin are formulated. The status of the rel… Show more

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Cited by 6 publications
(5 citation statements)
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“…These results are in agreement with those of [15] and [5] (in the latter case they were derived with the help of the Kruskal coordinates). As noted above, in FRW cosmology, these formulas are valid only for the de Sitter solution (see more comments on this in the following).…”
Section: Fl Flsupporting
confidence: 90%
“…These results are in agreement with those of [15] and [5] (in the latter case they were derived with the help of the Kruskal coordinates). As noted above, in FRW cosmology, these formulas are valid only for the de Sitter solution (see more comments on this in the following).…”
Section: Fl Flsupporting
confidence: 90%
“…These results are in agreement with those of [15] and [5] (in the latter case they were derived with the help of the Kruskal coordinates). As noted above, in FRW cosmology, these formulas are valid only for the de Sitter solution (see more comments on this in the following).…”
Section: Behavior Of Wavelengthsupporting
confidence: 90%
“…( 1) by replacing the DM halo velocity contributions, v 2 dark , with the relative curvature convolution ṽ2 lcm . It has been shown in previous work (Cisneros et al 2015;Radosz et al 2013) that curvature effects can be phrased kinematically. The LCM prediction of the total observed shifted frequencies, ω interpreted via the LD, is then :…”
Section: Lorentz Kinematics and The Lcm Rotation Curve Formulamentioning
confidence: 93%