Accelerating expansion or inhomogeneity? II. Mimicking acceleration with the energy function in the Lemaître-Tolman model

Andrzej Krasiński
Phys. Rev. D 90, 023524 – Published 16 July 2014

Abstract

This is a continuation of the paper published in Phys. Rev. D 89, 023520 (2014). Here we investigate how the luminosity distance–redshift relation DL(z) of the ΛCDM model is duplicated in the Lemaître-Tolman (L-T) model with Λ=0, constant bang-time function tB and the energy function E(r) mimicking accelerated expansion on the observer’s past light cone (r is a uniquely defined comoving radial coordinate). Numerical experiments show that E>0 necessarily. The functions z(r) and E(r) are numerically calculated from the initial point at the observer’s position, then backward from the initial point at the apparent horizon (AH). Reconciling the results of the two calculations allows one to determine the values of E/r2 at r=0 and at the AH. The problems connected with continuing the calculation through the AH are discussed in detail and solved. Then z(r) and E(r) are continued beyond the AH, up to the numerical crash that signals the contact of the light cone with the big bang. Similarly, the light cone of the L-T model is calculated by proceeding from the two initial points, and compared with the ΛCDM light cone. The model constructed here contains shell crossings, but they can be removed by matching the L-T region to a Friedmann background, without causing any conflict with the type Ia supernovae observations. The mechanism of imitating the accelerated expansion by the E(r) function is explained in a descriptive way.

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  • Received 26 May 2014

DOI:https://doi.org/10.1103/PhysRevD.90.023524

© 2014 American Physical Society

Authors & Affiliations

Andrzej Krasiński*

  • Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, Bartycka 18, 00 716 Warszawa, Poland

  • *akr@camk.edu.pl

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Issue

Vol. 90, Iss. 2 — 15 July 2014

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