mathbf {O}(D,D)$$ completion of the Friedmann equations | The European Physical Journal C
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SOLVED: Show that the equation of state associated with the energy density of the cosmological constant is P = -, with a negative pressure. Two different ways to do this are as
![SOLVED: 2. In this question you will derive the Friedmann-Lemaitre equations for cosmology a) Compute all non-zero Christoffel symbols for the Robertson-Walker metric: That is compute:T1;T22;133;T1;T1;T22;T33;T2;12;T33;13;T13;T23[13 marks] b) Show that ...](https://cdn.numerade.com/ask_images/cd627b1cf1a84d86b19759716693743c.jpg "SOLVED: 2. In this question you will derive the Friedmann-Lemaitre equations for cosmology a) Compute all non-zero Christoffel symbols for the Robertson-Walker metric: That is compute:T1;T22;133;T1;T1;T22;T33;T2;12;T33;13;T13;T23[13 marks] b) Show that ...")
SOLVED: 2. In this question you will derive the Friedmann-Lemaitre equations for cosmology a) Compute all non-zero Christoffel symbols for the Robertson-Walker metric: That is compute:T1;T22;133;T1;T1;T22;T33;T2;12;T33;13;T13;T23[13 marks] b) Show that ...
PPT - Derivation of the Friedmann Equations PowerPoint Presentation, free download - ID:5374016
Growth of perturbations in an expanding universe with Bose-Einstein condensate dark matter | Astronomy & Astrophysics (A&A)
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How to derive the energy continuity equation from the Friedmann Equations
The Friedmann Equations Explained: A Complete Guide – Profound Physics
The Friedmann Equations Explained: A Complete Guide – Profound Physics
Relativity
arXiv:1208.2482v3 [astro-ph.CO] 9 Feb 2013
Cosmological Guy (@laxmanaquanta) / X
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PDF) Bernoulli's Equation and Continuity Equation in terms of Energy/Mass Conservation
