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Titlebook: Dark Energy and the Formation of the Large Scale Structure of the Universe; Jér?me Gleyzes Book 2016 The Editor(s) (if applicable) and The

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樓主: 傳家寶
11#
發(fā)表于 2025-3-23 11:52:31 | 只看該作者
12#
發(fā)表于 2025-3-23 14:49:54 | 只看該作者
Hans-Jürgen Lange,H. Peter Ohly,Jo ReichertzI feel particularly lucky to have been working on my Ph.D. at such an exciting time for cosmology. With the fantastic results of the Planck mission?[.], our picture of the Universe and its history has become much clearer.
13#
發(fā)表于 2025-3-23 19:34:34 | 只看該作者
Aufbau betrieblicher InformationssystemeWhen looking at alternatives to the standard .CDM+GR model.
14#
發(fā)表于 2025-3-24 00:57:25 | 只看該作者
Die Normalisierung von RelationenIn this thesis, I have condensed what I thought were the most interesting results that I obtained during my Ph.D. I have voluntarily left out parts of the technical details and focused on the physical origin of these results, as well as their impact.
15#
發(fā)表于 2025-3-24 04:23:44 | 只看該作者
Introduction,I feel particularly lucky to have been working on my Ph.D. at such an exciting time for cosmology. With the fantastic results of the Planck mission?[.], our picture of the Universe and its history has become much clearer.
16#
發(fā)表于 2025-3-24 10:06:34 | 只看該作者
The Effective Field Theory of Dark Energy,When looking at alternatives to the standard .CDM+GR model.
17#
發(fā)表于 2025-3-24 12:34:32 | 只看該作者
Conclusion,In this thesis, I have condensed what I thought were the most interesting results that I obtained during my Ph.D. I have voluntarily left out parts of the technical details and focused on the physical origin of these results, as well as their impact.
18#
發(fā)表于 2025-3-24 14:59:43 | 只看該作者
19#
發(fā)表于 2025-3-24 21:09:33 | 只看該作者
20#
發(fā)表于 2025-3-24 23:57:17 | 只看該作者
XLeitf?den der angewandten Informatikinformation on cosmology, the next step is to rely on the large scale structure, via galaxy surveys for example. This has two main advantages. First, contrarily to the CMB which is a 2-D surface, galaxy surveys span the full 3-D space, which greatly increases their statistical power. Second, they pr
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