Quantum Mixmaster As a Model of the Primordial Universe
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GRAVITATION The Crab Nebula (NGC 1952), the remains of the supernova of July 1054, an event observed and recorded at the Sung national observatory at K'ai-feng. In the intervening 900 years, the debris from the explosion has moved out about three lightyears; i.e., with a speed about 1/ 300 of that of light. Tn 1934 Walter Baade and Fritz Zwicky pre dicted that neutron stars should be produced in supernova explosions. Among the first half~dozen pulsars found in 1968 was one at the center of the Crab Nebula, pulsing 30 times per second, for which there is today no acceptable explanation other than a spinning neutron star. The Chinese historical record shown here lists unusual astronomical phenomena observed during the Northern Sung dynasty. It comes from the "Journal of Astronomy," part 9, chapter 56, of the Sung History (Sung Shih), first printed in the 1340's. The photograph of that standard record used in this montage is copyright by, and I,nay not be reproduced without permission of, the Trustees of the British Museum. With a new foreword by David I. KAISER and a new preface by Charles W. MISNER and Kip S. THORNE PRINCETON UNIVERSITY PRESS PRINCETON AND OXFORD Copyright © 2017 by Charles W. Misner, Kip S. Thorne, and the Estate of John Archibald Wheeler Foreword to the 2017 edition copyright © 2017 by Princeton University Press Requests for permission to reproduce material from this work should be sent to Permissions, Princeton University Press Published by Princeton University Press, 41 William Street, Princeton, New Jersey 08540 In the United Kingdom: Princeton University Press, 6 Oxford Street, Woodstock, Oxfordshire OX20 1TR press.princeton.edu Cover illustration by Kenneth Gwin Errata and additional information on sources may be found at the following webpage: http://press.princeton.edu/titles/11169.html All Rights Reserved ISBN 978- 0- 691- 17779-3 Library of Congress Control Number: 2017950565 Original edition published in 1973 by W. -
Quasi-Isotropic Cycles and Nonsingular Bounces in a Mixmaster Cosmology
View metadata, citation and similar papers at core.ac.uk brought to you by CORE PHYSICAL REVIEW LETTERS 123, 201301 (2019) provided by Portsmouth University Research Portal (Pure) Quasi-Isotropic Cycles and Nonsingular Bounces in a Mixmaster Cosmology † Chandrima Ganguly1,* and Marco Bruni2,3, 1Department of Physics and Astronomy, Wilder Laboratories, Dartmouth College, Hanover, New Hampshire 03755, USA 2Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX, United Kingdom 3INFN Sezione di Trieste, Via Valerio 2, 34127 Trieste, Italy (Received 13 March 2019; revised manuscript received 11 September 2019; published 12 November 2019) A Bianchi type-IX mixmaster spacetime is the most general spatially homogeneous solution of Einstein’s equations and it can represent the space-averaged universe. We introduce two novel mechanisms resulting in a mixmaster universe with nonsingular bounces that are quasi-isotropic. Matter with a nonlinear equation of state allows these bounces. Using a negative anisotropic stress successfully isotropizes this universe and mitigates the well-known mixmaster chaotic behavior. The Universe can be an eternal mixmaster spacetime, going through an infinite series of quasi-isotropic cycles separated by bounces. DOI: 10.1103/PhysRevLett.123.201301 μν Introduction.—Cosmological parameter extraction from ρ_ ¼ −3Hðρ þ PÞ − πμνσ ; ð2Þ Planck [1–3] and other studies [4] place tight constraints on α the anisotropy of the current day Universe, ðσS=HÞo ∼ where ρ_ ≡ u ∇αρ is the proper time derivative along the −11 α α 10 ,whereσS represent the contribution of the (scalar fluid flow lines with 4-velocity u , 3H ¼ ∇αu is part of) shear anisotropic expansion, and H is the isotropic the expansion of the fluid, σμν is its shear, and πμν is the expansion rate. -
Observational Cosmology - 30H Course 218.163.109.230 Et Al
Observational cosmology - 30h course 218.163.109.230 et al. (2004–2014) PDF generated using the open source mwlib toolkit. See http://code.pediapress.com/ for more information. PDF generated at: Thu, 31 Oct 2013 03:42:03 UTC Contents Articles Observational cosmology 1 Observations: expansion, nucleosynthesis, CMB 5 Redshift 5 Hubble's law 19 Metric expansion of space 29 Big Bang nucleosynthesis 41 Cosmic microwave background 47 Hot big bang model 58 Friedmann equations 58 Friedmann–Lemaître–Robertson–Walker metric 62 Distance measures (cosmology) 68 Observations: up to 10 Gpc/h 71 Observable universe 71 Structure formation 82 Galaxy formation and evolution 88 Quasar 93 Active galactic nucleus 99 Galaxy filament 106 Phenomenological model: LambdaCDM + MOND 111 Lambda-CDM model 111 Inflation (cosmology) 116 Modified Newtonian dynamics 129 Towards a physical model 137 Shape of the universe 137 Inhomogeneous cosmology 143 Back-reaction 144 References Article Sources and Contributors 145 Image Sources, Licenses and Contributors 148 Article Licenses License 150 Observational cosmology 1 Observational cosmology Observational cosmology is the study of the structure, the evolution and the origin of the universe through observation, using instruments such as telescopes and cosmic ray detectors. Early observations The science of physical cosmology as it is practiced today had its subject material defined in the years following the Shapley-Curtis debate when it was determined that the universe had a larger scale than the Milky Way galaxy. This was precipitated by observations that established the size and the dynamics of the cosmos that could be explained by Einstein's General Theory of Relativity. -
Quasi-Isotropic Cycles and Nonsingular Bounces in a Mixmaster Cosmology
PHYSICAL REVIEW LETTERS 123, 201301 (2019) Quasi-Isotropic Cycles and Nonsingular Bounces in a Mixmaster Cosmology † Chandrima Ganguly1,* and Marco Bruni2,3, 1Department of Physics and Astronomy, Wilder Laboratories, Dartmouth College, Hanover, New Hampshire 03755, USA 2Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX, United Kingdom 3INFN Sezione di Trieste, Via Valerio 2, 34127 Trieste, Italy (Received 13 March 2019; revised manuscript received 11 September 2019; published 12 November 2019) A Bianchi type-IX mixmaster spacetime is the most general spatially homogeneous solution of Einstein’s equations and it can represent the space-averaged universe. We introduce two novel mechanisms resulting in a mixmaster universe with nonsingular bounces that are quasi-isotropic. Matter with a nonlinear equation of state allows these bounces. Using a negative anisotropic stress successfully isotropizes this universe and mitigates the well-known mixmaster chaotic behavior. The Universe can be an eternal mixmaster spacetime, going through an infinite series of quasi-isotropic cycles separated by bounces. DOI: 10.1103/PhysRevLett.123.201301 μν Introduction.—Cosmological parameter extraction from ρ_ ¼ −3Hðρ þ PÞ − πμνσ ; ð2Þ Planck [1–3] and other studies [4] place tight constraints on α the anisotropy of the current day Universe, ðσS=HÞo ∼ where ρ_ ≡ u ∇αρ is the proper time derivative along the −11 α α 10 ,whereσS represent the contribution of the (scalar fluid flow lines with 4-velocity u , 3H ¼ ∇αu is part of) shear anisotropic expansion, and H is the isotropic the expansion of the fluid, σμν is its shear, and πμν is the expansion rate. -
Publications List
Publications of Bei-Lok Hu 胡悲樂 June 2016 A. Papers Published in Refereed Journals: Physics and Astronomy Research 1. "VIBRATIONAL ENERGY TRANSFER IN CO2 LASERS" C. B. Moore, R. E. Wood, B. L. Hu and J. T. Yardley Journal of Chemical Physics 46, 4222 (1967). 2. "PERBURBATIONS ON THE MIXMASTER UNIVERSE" B. L. Hu and T. Regge, Physical Review Letters 29, 1616 (1972). 3. "SCALAR WAVES IN THE MIXMASTER UNIVERSE I. Helmholtz Equation in a Fixed Background", Physical Review D8, 1048 (1973). 4. "QUANTIZED SCALAR FIELDS IN a CLOSED ANISOTROPIC UNIVERSE' B. L. Hu, S. A. Fulling and L. Parker, Physical Review D8, 2377 (1973) . 5. "SCALAR WAVES IN THE MIXMASTER UNIVERSE II. Particle Creation" Physical Review D9, 3263 (1974). 6. "SEPARATION OF TENSOR EQUATIONS IN A HOMOGENEOUS SPACE BY GROUP THEORETICAL METHODS" Journal of Mathematical Physics 15, 1748 (1974). 7. "CONFORMAL ENERGY-MOMENTUM TENSOR IN CURVED SPACETIMES: Adiabatic Regularization and Renormalization" S. A. Fulling, L. Parker and B. L. Hu, Physical Review D10, 3905 (1974). 8. "NUMERICAL EXAMPLES FROM PERTURBATION ANALYSIS OF THE MIXMASTER UNIVERSE" Physical Review D12, 1551 (1975). 9. "EFFECT OF GRAVITON CREATION IN ISOTROPICALLY EXPLANDING UNIVERSES” B. L. Hu and L. Parker, Physics Letters 63A, 217 (1977). 10. "ANISOTROPY DAMPING THROUGH QUANTUM EFFECTS IN THE EARLY UNIVERSE" B. L. Hu and L. Parker, Physical Review D17, 933 (1978). 11. "GRAVITATIONAL WAVES IN A BIANCHI TYPE I UNIVERSE" Physical Review D18, 969 (1978). 12. "CALCULATION OF TRACE ANOMALY OF CONFORMAL TENSOR ENERGY- MOMENTUM IN KASNER SPACETIME BY ADIABATIC REGULARIZATION" Physical Review D18, 4460 (1978). 13. "TRACE ANOMALY OF THE ENERGY-MOMENTUM TENSOR OF QUANTIZED SCALAR FIELDS IN ROBERTSON-WALKER SPACETIME" Physics Letters 71A, 169-173 (1979) 14. -
Mixmaster Universe in Horava-Lifshitz Gravity
CPHT-RR111.1109 LMU-ASC 48/09 MPP-2009-180 Mixmaster universe in Hoˇrava-Lifshitz gravity 1 † 2 ‡ 3,4 § 2 Ioannis Bakas∗ , Francois Bourliot , Dieter Lüst and Marios Petropoulos 1 Department of Physics, University of Patras 26500 Patras, Greece 2 Centre de Physique Théorique, Ecole Polytechnique CNRS UMR 7644, 91128 Palaiseau Cedex, France 3 Max-Planck-Institut für Physik Föhringer Ring 6, 80805 München, Germany 4 Arnold-Sommerfeld-Center für Theoretische Physik Department für Physik, Ludwig-Maximilians-Universität München Theresienstraße 37, 80333 München, Germany October 25, 2018 ABSTRACT We consider spatially homogeneous (but generally non-isotropic) cosmologies in the recently proposed Hoˇrava-Lifshitz gravity and compare them to those of general rel- ativity using Hamiltonian methods. In all cases, the problem is described by an effec- tive point particle moving in a potential well with exponentially steep walls. Focusing on the closed-space cosmological model (Bianchi type IX), the mixmaster dynamics is arXiv:0911.2665v1 [hep-th] 13 Nov 2009 now completely dominated by the quadratic Cotton tensor potential term for very small volume of the universe. Unlike general relativity, where the evolution towards the initial singularity always exhibits chaotic behavior with alternating Kasner epochs, the anisotropic universe in Hoˇrava-Lifshitz gravity (with parameter λ > 1/3) is de- scribed by a particle moving in a frozen potential well with fixed (but arbitrary) energy E. Alternating Kasner epochs still provide a good description of the early universe for very large E, but the evolution appears to be non-ergodic. For very small E there are harmonic oscillations around the fully isotropic model. -
Durham E-Theses
Durham E-Theses Spacelike Geodesics and Other Puzzles in the Mixmaster Universe KENWAY, ANGHARAD,SONIA How to cite: KENWAY, ANGHARAD,SONIA (2012) Spacelike Geodesics and Other Puzzles in the Mixmaster Universe, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/3457/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk Spacelike Geodesics and Other Puzzles in the Mixmaster Universe Angharad Sonia Kenway A Thesis presented for the degree of Doctor of Philosophy Centre for Particle Theory Department of Mathematical Sciences University of Durham England October 2011 Dedicated to my family Spacelike Geodesics and Other Puzzles in the Mixmaster Universe Angharad Sonia Kenway Submitted for the degree of Doctor of Philosophy October 2011 Abstract In this thesis we are going to investigate the behaviour of geodesics in a metric with a singularity known as the \Mixmaster Universe". -
Classical and Quantum Features of the Mixmaster Singularity
Classical and Quantum Features of the Mixmaster Singularity Giovanni Montani, ICRA, International Center for Relativistic Astrophysics ENEA C.R. Frascati, Dipartimento F.P.N., Frascati, Roma, Italy Dipartimento di Fisica Universit´a“Sapienza”, P.le a. Moro 5, 00185 Roma, Italy ICRANet, International Relativistic Astrophysics Network, Pescara, Italy [email protected] Marco Valerio Battisti, ICRA, International Center for Relativistic Astrophysics Dipartimento di Fisica Universit´a“Sapienza”, P.le a. Moro 5, 00185 Roma, Italy [email protected] Riccardo Benini ICRA, International Center for Relativistic Astrophysics Dipartimento di Fisica Universit´a“Sapienza”, P.le a. Moro 5, 00185 Roma, Italy [email protected] Giovanni Imponente arXiv:0712.3008v3 [gr-qc] 12 Sep 2008 Museo Storico della Fisica e Centro Studi e Ricerche “E. Fermi”, Roma, Italy Dipartimento di Fisica Universit´a“Sapienza”, P.le a. Moro 5, 00185 Roma, Italy [email protected] Abstract This review article is devoted to analyze the main properties characterizing the cosmo- logical singularity associated to the homogeneous and inhomogeneous Mixmaster model. After the introduction of the main tools required to treat the cosmological issue, we re- view in details the main results got along the last forty years on the Mixmaster topic. We firstly assess the classical picture of the homogeneous chaotic cosmologies and, after a presentation of the canonical method for the quantization, we develop the quantum Mix- master behavior. Finally, we extend both the classical and quantum features to the fully inhomogeneous case. Our survey analyzes the fundamental framework of the Mixmaster picture and completes it by accounting for recent and peculiar outstanding results.