Quantum cosmology

Results: 296



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51Astronomy How does cosmic structure form? We study planets, stellar evolution, stellar seismology, compact stellar remnants, gravity waves, neutron star emission, supernovae, gamma-ray bursters, galaxy dynamics and evolu

Astronomy How does cosmic structure form? We study planets, stellar evolution, stellar seismology, compact stellar remnants, gravity waves, neutron star emission, supernovae, gamma-ray bursters, galaxy dynamics and evolu

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Source URL: physics.unc.edu

Language: English - Date: 2014-11-12 17:54:38
52On some possible mathematical connections concerning Noncommutative Minisuperspace Cosmology, Noncommutative Quantum Cosmology in low-energy String Action, Noncommutative Kantowsky-Sachs Quantum Model, Spectral Action Pr

On some possible mathematical connections concerning Noncommutative Minisuperspace Cosmology, Noncommutative Quantum Cosmology in low-energy String Action, Noncommutative Kantowsky-Sachs Quantum Model, Spectral Action Pr

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Source URL: empslocal.ex.ac.uk

Language: English - Date: 2008-01-16 04:37:12
53Preface Introductory Comments.  General relativity is one of the greatest triumphs of the human mind. Together with quantum field theory, general relativity lies at the foundation of contemporary physics and currently

Preface Introductory Comments.  General relativity is one of the greatest triumphs of the human mind. Together with quantum field theory, general relativity lies at the foundation of contemporary physics and currently

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Source URL: www.uscibooks.com

Language: English - Date: 2012-10-11 10:20:48
54Second-order gauge-invariant cosmological perturbation theory NAKAMURA, Kouji (NAOJ) Due to the precise measurement of the Cosmic Microwave Background (CMB) by WMAP, the “precision cosmology” has begun. The farthest

Second-order gauge-invariant cosmological perturbation theory NAKAMURA, Kouji (NAOJ) Due to the precise measurement of the Cosmic Microwave Background (CMB) by WMAP, the “precision cosmology” has begun. The farthest

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Source URL: www.nao.ac.jp

Language: English - Date: 2012-07-25 04:23:20
55PHD QUALIFY EXAMINATION — GALACTIC AND EXTRAGALACTIC ASTROPHYSICS 25th September, points) (a) (5 points) What are the luminosity function Φ(M ), the initial luminosity function

PHD QUALIFY EXAMINATION — GALACTIC AND EXTRAGALACTIC ASTROPHYSICS 25th September, points) (a) (5 points) What are the luminosity function Φ(M ), the initial luminosity function

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
56

PDF Document

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Source URL: www.ulb.ac.be

Language: English - Date: 2012-04-20 07:30:49
57Construction of Gauge-invariant Variables of Linear Metric Perturbations on an Arbitrary Background Spacetime NAKAMURA, Kouji (NAOJ) Perturbation techiques are powerful in many areas of

Construction of Gauge-invariant Variables of Linear Metric Perturbations on an Arbitrary Background Spacetime NAKAMURA, Kouji (NAOJ) Perturbation techiques are powerful in many areas of

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Source URL: www.nao.ac.jp

Language: English - Date: 2015-03-23 03:19:20
58This presentation was made using free software under the GNU/Linux operating system. This is what you can save by using free software: New Ways to Make Old Strings

This presentation was made using free software under the GNU/Linux operating system. This is what you can save by using free software: New Ways to Make Old Strings

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Source URL: theory.tifr.res.in

Language: English
59U (1) ⊗ U (1) Gauge Fields on Domain Walls Damien George Supervisor: Prof. Raymond Volkas Part IV honours thesis November 2004 Abstract

U (1) ⊗ U (1) Gauge Fields on Domain Walls Damien George Supervisor: Prof. Raymond Volkas Part IV honours thesis November 2004 Abstract

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Source URL: dpgeorge.net

Language: English - Date: 2008-10-20 01:21:38
60Introduction to AdS/CFT ................ ................ Introduction to Introduction

Introduction to AdS/CFT ................ ................ Introduction to Introduction

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Source URL: insti.physics.sunysb.edu

Language: English