Titlebook: Structure Formation in the Universe; Robert G. Crittenden,Neil G. Turok Book 2001 Springer Science+Business Media Dordrecht 2001 Gravity.I

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Apogee

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Book 2001on Institute in Cambridge in August, 1999. The ASI was held at a critical juncture in the development of physical cosmology, when a flood of new data concerning the large scale structure of the Universe was just be­ coming available. There was an air of excitement and anticipation: would the standar

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Cosmic Inflationsis of recent successes and open questions. There is a special discussion of the physics of “cosmic coherence“ in the primordial perturbations. The issue of coherence is at the heart of much of the success inflation theory has achieved at the hands of the new microwave background data. While much of

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Before Inflationhysical mechanism for generating the inhomogeneities we see inVol.ves the amplification of quantum fluctuations during a period of inflation. Developing the theory further will require progress in quantum cosmology, connecting inflation to a theory of the initial state of the Universe. I discuss rec

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Quantum Cosmologyile quantum fluctuations are small and can be treated as perturbations. Prior to this stage, however, genuinely quantum phenomena almost certainly took place. Although it is not clear whether they have left any observable foot- prints, it is of interest to try to understand them, as this may shed li

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Observational Tests for the Cosmological Principle and World Modelsckground, the Lyman-α forest and the Cosmic Microwave Background are used to set constraints on inhomogeneous models and in particular on fractal-like models. Assuming the Cosmological Principle and the FRW metric, we estimate cosmological parameters by joint analysis of peculiar velocities, the CMB

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