Abstract
We conclude with short descriptions of a few important problems of cosmological physics. These tie together several topics from previous chapters. We discuss (1) Homogeneity scale and superlarge structures, (2) Detection of baryonic acoustic oscillations, (3) Dark energy in the neighbourhood of the Local Group, and (4) Conceptual problems of the expanding space physics.
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Notes
- 1.
These deep galaxy surveys are COSMOS (Cosmic Evolution Survey), FDF (FORS Deep Field of the ESO VLT), HUDF (Hubble Ultra Deep Field), and HDF-N (Hubble Deep Field North). The COSMOS survey contains about half a million photometric redshifts evaluated using 30 filters for over 600 000 galaxies in a field of 77′×77′, with the limiting B magnitude of 26. The other samples are smaller in galaxy number and field size, but extend deeper, with the limiting magnitudes 27–30.
- 2.
The ALHAMBRA project (Moles et al. 2008), with observations of 8 deep fields in 20 filters and a total of 6.6×105 galaxies, is currently in the process of completion.
- 3.
\(A=1/H_{\mathrm{V}} =(\frac{8 \pi G}{3} \rho_{\mathrm{V}})^{-1/2} \simeq5 \times10^{17} s\simeq1.5 \times10^{28}\) cm is a characteristic vacuum time/length, the inverse value of the “vacuum Hubble constant” H V.
- 4.
This is the same 1.7 as in the global scale factor ratio leading to z v=0.7. Namely, the requirement that the global acceleration is zero when ρ V=0.5ρ m(z V) leads in terms of the current mass density to the condition 2ρ V=(1+z V)3 ρ m or (2ρ loc/ρ m)1/3=(1+z V)=1.7.
- 5.
The LTB models, which are asymptotically Friedmann-like on large scales, have three possible initial conditions: the density distribution, the velocity field, and the bang time function, and any two of these determine the third one. Therefore, Gromov et al. (2001) pointed out that the Hubble law may be linear even inside a fractal distribution if the bang time function is suitably broad. This explanation may sound too artificial; however, a variant of it has been applied by Célérier et al. (2010) to explain the Hubble diagram of distant SNIa supernovae without the need to assume a big local hole (or dark energy).
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Baryshev, Y., Teerikorpi, P. (2012). Some Outstanding Problems of Cosmological Physics. In: Fundamental Questions of Practical Cosmology. Astrophysics and Space Science Library, vol 383. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-2379-5_12
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