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1 Erratum to: Eur. Phys. J. C (2015) 75:411 DOI 10.1140/epjc/s10052-015-3614-3
The present remarks as regards Ref. [1] result from a useful discussion with Helbig, one of the authors of Ref. [2]. We would like to clarify this in what follows.
In Ref. [1] we derived the generalized differential equation (32) using such tools as null geodesics and the ratio of longitudinal to transverse angular momentum of a photon. We also repeated calculations using the focusing equation [3], where we proved that the general form of the equation for the angular diameter distance in \(\Lambda CDM\) is
Equation (1) is the generalised version of the Dashevskii equation in [4] for a model with the equation of state for several components with arbitrary equations of state. (Note that in this form, it is assumed that all of these components clump in the same manner.) Displaying the components for the \(\Lambda CDM\) model we obtain
Using the equations of state for baryonic matter (\(p_M=0\)), dark energy (\(p_\Lambda =-\rho _\Lambda \)), and radiation (\(p_R=\rho _R/3\)), we convert Eq. (2) to
Using (3), Eq. (1) acquires the form
Then if we set \(\rho _R=0\) we will obtain the Dashevskii equation in [4]. This result was not known to us at the time when we were writing Ref. [1]; that is why we wrote that the authors [2] obtained a wrong result. The authors of [2] started from the old Dashevskii equation, but not from (4). This means that the equation obtained by Dashevskii for the model without \(\Lambda \) (or dark energy) term is still valid in \(\Lambda CDM\), which was not obvious.
Because in such a setup the Dashevskii equation remains valid in \(\Lambda CDM\), the final equation for the ADD measurement is true. Nevertheless we should note that it is unnecessary to use the equation from [2], because it is much simpler to integrate the Dashevskii equation itself, after converting the redshift to cosmic time, as was shown in Ref. [1].
Thus we can summarize as follows:
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The more general version of the differential equation for the angular diameter distance for models containing components with arbitrary equations of state is our result Eq. (1).
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If the dark energy equation of state is \(p_\Lambda = -\rho _\Lambda \) and \(\rho _R = 0\), which corresponds to the cosmological constant, then the original Dashevskii equation is valid for \(\Lambda CDM\). This explains why Ref. [2] produces valid results.
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The code presented in [2] produces correct results.
References
A.V. Nikolaev, S.V. Chervon, EPJC 75, 411 (2015)
R. Kayser, P. Helbig, T. Schramm, Astron. Astrophys. 318, 680 (1997)
A. Nikolaev, S. Chervon, Gravit. Cosmol. 22, 208 (2016)
V.M. Dashevskii, V.I. Slysh, Sov. A 9, 671 (1965)
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Nikolaev, A.V., Chervon, S.V. Erratum to: Development of Zeldovich’s approach for cosmological distances measurement in the Friedmann Universe. Eur. Phys. J. C 77, 446 (2017). https://doi.org/10.1140/epjc/s10052-017-5026-z
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DOI: https://doi.org/10.1140/epjc/s10052-017-5026-z