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By Dierck-Ekkehard Liebscher (auth.)

ISBN-10: 3540232613

ISBN-13: 9783540232612

Cosmology offers with the present country of wondering the elemental questions on the middle of the sphere of cosmology. extra emphasis than traditional is wear the connections to comparable domain names of technological know-how, similar to geometry, relativity, thermodynamics, particle physics, and - specifically - at the intrinsic connections among different themes. The chapters are illustrated with many figures which are as distinctive as at the moment attainable, e.g. in relation to geometry and relativity. Readers collect a graduate-level wisdom of cosmology because it is needed to appreciate the cosmological influence in their specific learn subject matters, in addition to an advent into the present study within the field.

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We postpone the question of where the inhomogeneities come from (we may handle them like other matter components, of course). The various paths to follow the arguments are summarised in Fig. 9. References 1. Bahcall, J. , Steinhardt, C. : Does the fine-structure constant vary with cosmological epoch? Astrophys. J. 600 (2004), 520–543. 8 2. : Was there a big bang? Astron. Astrophys. 204 (1988), 1–2. 21 3. Nicolaus de Cusa: De docta ignorantia, liber secundus, P. ), Akademie-Verlag, Berlin (1440).

If the intention of cosmology of finding an explanation for the observed state of the universe in its evolution and not in its initial conditions is successfully achieved, we cannot tell anything observable about this beginning: it is not essential. The second answer is that the cosmological singularity shows the limitations of the physical laws whose extrapolation leads to this singularity. Most proposals of this kind consider the question of whether an appropriately constructed quantum theory of gravitation can avoid singular phenomena.

The Euler–Lagrange equations turn out to be ∂L − ∂Ψ ∂L ∂Ψ;k =0. ;k The variational derivative of the integral Smat with respect to the metric yields terms proportional to δΨ;k , which are, however, linear combinations of different (δgik );l . 3 General Relativity: Solving Galileo’s Paradox 45 through partial integration, and we finally obtain a linear combination of the δgik . The coefficients of this expression form what is called the metric energy– momentum tensor, √ √ δ(L −g) c = 2 −gT ik . δgik The invariance of the form of the Lagrange density with respect to coordinate substitutions √ √ ∂x (L −g)[x∗ ] = (L −g)[x[x∗ ]] , ∂x∗ together with the field equations, implies the covariant conservation theorem ∂T ik + T mk Γ imk + T im Γ kmk = 0 .

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Cosmology by Dierck-Ekkehard Liebscher (auth.)


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