Towards a Theory of Quantum Gravity Through Geometrization of Quantum Mechanics

Total Page:16

File Type:pdf, Size:1020Kb

Towards a Theory of Quantum Gravity Through Geometrization of Quantum Mechanics Towards a Theory of Quantum Gravity Through Geometrization of Quantum Mechanics Thesis by ChunJun Cao In Partial Fulfillment of the Requirements for the degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2018 (Defended May 1, 2018) ii © 2018 ChunJun Cao ORCID: 0000-0002-5761-5474 All rights reserved iii ACKNOWLEDGEMENTS Before I start my long list of appreciations, I think it is worth reminding myself that the greatest lesson I have learned in my past few years is that no accomplishment of mine is that of a single person; rather, it is insignificant in comparison to all the people who have made me the person I am today. I would like to begin by thanking my wonderful advisor, Sean Carroll, for his invaluable support and wisdom in physics as well as in life. I am immensely grateful for all the guidance and encouragement Sean has offered over the years. My academic life at Caltech has been fruitful and exhilarating thanks to Sean’s dedication to physics as well as the well-being of students. I am thankful to the members of my thesis committee, Clifford Cheung, David Hsieh, Anton Kapustin, and John Preskill, for offering their valuable insights and expertise. I also thank my collaborators, Ning Bao, Aidan Chatwin-Davies, Sebastian Fischetti, Nick Hunter-Jones, Cindy Keeler, Junyu Liu, Shaun Maguire, Liam McAllister, Spiros, Michalakis, Jason Pollack, Grant Remmen, Ashmeet Singh, Eugene Tang, Michael Walter, Zitao Wang, Zhao Yang, Yuan Yao, Ariel Zhitnitsky, and Claire Zukowski, with whom I have had a wonderful time exploring the realm of physics. I am especially thankful for Ning Bao and Ariel Zhitnitsky, who are wonderful collaborators and great mentors. I also thank my friend Aidan Chatwin-Davies, who is always considerate, vibrant and full of optimism throughout our five years at Caltech. I very much enjoyed my conversations with Zitao Wang, who has been patient in entertaining my wildest questions and speculations. I am indebted to Tony Bartolotta, Bartek Czech, Dan Harlow, Matthew Heydeman, Alex Kubica, Jenia Mozgunov, Ingmar Saberi, Brian Swingle, Xiao-Liang Qi, Gunther Uhlmann, Mark van Raamsdonk, Guifre Vidal, Tian Wang, Mark Wise,Yi-zhuang You, and many others for the interesting physics discussions. I also thank Caltech, for fostering an intellectually stimulating environment and for support its students. It truly has been a humbling experience to learn and walk among some of the giants of our time. My deepest appreciation to all my friends, who made my PhD years warm and full of life: Bob Briton, Alice Chik, Steven Dong, Frank Hong, Voonhui Lai, Jonas Lippuner, James Liu, John Pang, Alvin Phua, Jamie Rankin, Bekah Silva, Yong Sheng Soh, Zhan Su, Alex Tseng, Becky Wang, Dan Wu, and Lucie Xiang. My iv special thanks to John Pang, for his generousity and hospitality for letting me sleep on the couch and using his car when necessary. We had a lot of good times at Bridges, too. I am immensely grateful for my fellow group mates, Ashmeet Singh, Alec Ridgeway, and James St. Germaine-Fuller, for the consistent social and emotional support as well as wonderful physics interactions. I also thank the Dungeons and Dragons and our PC gaming crew: Aidan Chatwin-Davies, Mike Grudic,David Guszejnov, Florian Hoffmann, Seva Ivanov, Anna Komar, Alex Kubica, Clare Lahey, and Jenia Mozgunov. My thanks to the Caltech Ultimate Frisbee pickup group, and Caltech Concert Band and Chamber Music, which helped maintain my mental sanity during the initial years of graduate school. I recall some of the memory-making restaurants like Sansai for giving us cheap but mostly reliable food when I am too lazy to cook. I also very muched enjoyed my visits to the Counter and Abricott. I still think the Top Restaurant at Allen and Colorado makes the best chicken katsu, disagree with me all you want. Thanks to Sam Woo’s for the interesting food making; it has certainly made an indelible impression on me during my last year. Lastly, I would like to thank my parents, who have been supportive in whatever goal I pursue, and for caring and guiding me throughout the past five years. I am grateful to my girlfriend who has been supportive even in my worse days. And thanks to God who sustains me by His grace and mercy. I would like to acknowledge the Natural Sciences and Engineering Research Council of Canada (NSERC) which help support my research. The research is funded in part by the Walter Burke Institute for Theoretical Physics at Caltech, by DOE grant DE-SC0011632, by the Foundational Questions Institute, by the Gordon and Betty Moore Foundation through Grant 776 to the Caltech Moore Center for Theoretical Cosmology and Physics, and by the Natural Sciences and Engineering Research Council of Canada (NSERC). v ABSTRACT In this thesis, we adapt an approach by assuming quantum mechanics as a funda- mental theory of nature and attempt to recover familiar concepts such as space-time geometry and gravity from quantum wavefunctions and their unitary evolutions. More specifically, we explore a number of approaches in “geometrizing” quantum systems using techniques such as tensor networks and manifold learning. We find that consistency conditions in quantum gravity can be used to put constraints on tensor network models that approximate the anti-de Sitter/Conformal Field Theory correspondence. Furthermore, quantum circuits and tensor networks can also be used to describe cosmological models and reproduce important features of space- time configurations such as de Sitter space. We find that a generic framework using quantum circuit to describe cosmology puts an upper bound on the number of e-folds during the inflationary phase of the Universe’s expansion. In addition to tensor network models, we also propose a Bulk Entanglement Gravity framework that analyzes the entanglement data of a quantum state in a Hilbert space without any a priori assumptions on geometry, such as the likes of a boundary conformal field theory. We find that from an amorphous configuration, one can directly re- cover geometry of bulk space-time from a generic class of wavefunctions that is fully characterized in this thesis via quantum entropy cone techniques. We find that under a number of assumptions, it is possible to derive linearized Einstein’s equation from a version of Jacobson’s entanglement equilibrium conditions for an emergent spacetime geometry in the weak field limit near Minkowski space. We show that non-local entanglement perturbations display features of wormhole-like configurations. We also clarify connections between Bulk Entanglement Gravity and highly generic features in quantum error correction codes that can be used to derive gravity. vi PUBLISHED CONTENT AND CONTRIBUTIONS [1] Ning Bao, ChunJun Cao, Sean M. Carroll, Aidan Chatwin-Davies, Nicholas Hunter-Jones, Jason Pollack, and Grant N. Remmen. “Consistency condi- tions for an AdS multiscale entanglement renormalization ansatz correspon- dence”. In: Phys. Rev. D91.12 (2015), p. 125036. doi: 10.1103/PhysRevD. 91.125036. arXiv: 1504.06632 [hep-th]. C. C participated in the conception of the project as well as the formulation of the main arguments, performed mathematical analysis of the entanglement bounds, and helped write the manuscript. [2] Ning Bao, ChunJun Cao, Sean M. Carroll, and Aidan Chatwin-Davies. “De Sitter Space as a Tensor Network: Cosmic No-Hair, Complementarity, and Complexity”. In: Phys. Rev. D96.12 (2017), p. 123536. doi: 10.1103/ PhysRevD.96.123536. arXiv: 1709.03513 [hep-th]. C. C participated in the conception of the project, drafted and performed mathematical analysis of the arguments, and helped write the manuscript. [3] Ning Bao, ChunJun Cao, Sean M. Carroll, and Liam McAllister. “Quantum Circuit Cosmology: The Expansion of the Universe Since the First Qubit”. In: (2017). arXiv: 1702.06959 [hep-th]. C. C participated in the conception of the project as well as the formulation of the main arguments, performed mathematical analysis, and helped write the manuscript. [4] Ning Bao, ChunJun Cao, Michael Walter, and Zitao Wang. “Holographic entropy inequalities and gapped phases of matter”. In: JHEP 09 (2015), p. 203. doi: 10.1007/JHEP09(2015)203. arXiv: 1507.05650 [hep-th]. C. C participated in the conception of the project, performed analytical and numerical analysis that led to the theorems and their proofs, and helped write the manuscript. [5] ChunJun Cao, Sean M. Carroll, and Spyridon Michalakis. “Space from Hilbert Space: Recovering Geometry from Bulk Entanglement”. In: Phys. Rev. D95.2 (2017), p. 024031. doi: 10.1103/PhysRevD.95.024031. arXiv: 1606.08444 [hep-th]. C. C participated in the conception of the project, drafted and performed mathematical analysis of the arguments, and helped write the manuscript. [6] ChunJun Cao and Sean M. Carroll. “Bulk entanglement gravity without a boundary: Towards finding Einstein’s equation in Hilbert space”. In: Phys. Rev. D97.8 (2018), p. 086003. doi: 10.1103/PhysRevD.97.086003. arXiv: 1712.02803 [hep-th]. C. C participated in the conception of the project, drafted and performed mathematical analysis of the arguments, and helped write the manuscript. vii TABLE OF CONTENTS Acknowledgements . iii Abstract . v Published Content and Contributions . vi Table of Contents . vii List of Illustrations . x List of Tables . xvi Chapter I: Introduction . 1 Chapter II: Consistency Conditions for an AdS/MERA Correspondence . 7 2.1 Introduction . 7 2.2 AdS/MERA . 9 2.2.1 Review of the MERA . 9 2.2.2 An AdS/MERA Correspondence? . 12 2.3 MERA and Geometry . 15 2.3.1 Consistency conditions from matching trajectories . 15 2.3.2 Limits on sub-AdS scale physics . 17 2.4 Constraints from Boundary Entanglement Entropy . 18 2.4.1 MERA and CFT Entanglement Entropy . 19 2.4.2 Constraining SMERA ...................... 21 2.4.3 Matching to the CFT .
Recommended publications
  • The State of the Multiverse: the String Landscape, the Cosmological Constant, and the Arrow of Time
    The State of the Multiverse: The String Landscape, the Cosmological Constant, and the Arrow of Time Raphael Bousso Center for Theoretical Physics University of California, Berkeley Stephen Hawking: 70th Birthday Conference Cambridge, 6 January 2011 RB & Polchinski, hep-th/0004134; RB, arXiv:1112.3341 The Cosmological Constant Problem The Landscape of String Theory Cosmology: Eternal inflation and the Multiverse The Observed Arrow of Time The Arrow of Time in Monovacuous Theories A Landscape with Two Vacua A Landscape with Four Vacua The String Landscape Magnitude of contributions to the vacuum energy graviton (a) (b) I Vacuum fluctuations: SUSY cutoff: ! 10−64; Planck scale cutoff: ! 1 I Effective potentials for scalars: Electroweak symmetry breaking lowers Λ by approximately (200 GeV)4 ≈ 10−67. The cosmological constant problem −121 I Each known contribution is much larger than 10 (the observational upper bound on jΛj known for decades) I Different contributions can cancel against each other or against ΛEinstein. I But why would they do so to a precision better than 10−121? Why is the vacuum energy so small? 6= 0 Why is the energy of the vacuum so small, and why is it comparable to the matter density in the present era? Recent observations Supernovae/CMB/ Large Scale Structure: Λ ≈ 0:4 × 10−121 Recent observations Supernovae/CMB/ Large Scale Structure: Λ ≈ 0:4 × 10−121 6= 0 Why is the energy of the vacuum so small, and why is it comparable to the matter density in the present era? The Cosmological Constant Problem The Landscape of String Theory Cosmology: Eternal inflation and the Multiverse The Observed Arrow of Time The Arrow of Time in Monovacuous Theories A Landscape with Two Vacua A Landscape with Four Vacua The String Landscape Many ways to make empty space Topology and combinatorics RB & Polchinski (2000) I A six-dimensional manifold contains hundreds of topological cycles.
    [Show full text]
  • On Asymptotically De Sitter Space: Entropy & Moduli Dynamics
    On Asymptotically de Sitter Space: Entropy & Moduli Dynamics To Appear... [1206.nnnn] Mahdi Torabian International Centre for Theoretical Physics, Trieste String Phenomenology Workshop 2012 Isaac Newton Institute , CAMBRIDGE 1 Tuesday, June 26, 12 WMAP 7-year Cosmological Interpretation 3 TABLE 1 The state of Summarythe ofart the cosmological of Observational parameters of ΛCDM modela Cosmology b c Class Parameter WMAP 7-year ML WMAP+BAO+H0 ML WMAP 7-year Mean WMAP+BAO+H0 Mean 2 +0.056 Primary 100Ωbh 2.227 2.253 2.249−0.057 2.255 ± 0.054 2 Ωch 0.1116 0.1122 0.1120 ± 0.0056 0.1126 ± 0.0036 +0.030 ΩΛ 0.729 0.728 0.727−0.029 0.725 ± 0.016 ns 0.966 0.967 0.967 ± 0.014 0.968 ± 0.012 τ 0.085 0.085 0.088 ± 0.015 0.088 ± 0.014 2 d −9 −9 −9 −9 ∆R(k0) 2.42 × 10 2.42 × 10 (2.43 ± 0.11) × 10 (2.430 ± 0.091) × 10 +0.030 Derived σ8 0.809 0.810 0.811−0.031 0.816 ± 0.024 H0 70.3km/s/Mpc 70.4km/s/Mpc 70.4 ± 2.5km/s/Mpc 70.2 ± 1.4km/s/Mpc Ωb 0.0451 0.0455 0.0455 ± 0.0028 0.0458 ± 0.0016 Ωc 0.226 0.226 0.228 ± 0.027 0.229 ± 0.015 2 +0.0056 Ωmh 0.1338 0.1347 0.1345−0.0055 0.1352 ± 0.0036 e zreion 10.4 10.3 10.6 ± 1.210.6 ± 1.2 f t0 13.79 Gyr 13.76 Gyr 13.77 ± 0.13 Gyr 13.76 ± 0.11 Gyr a The parameters listed here are derived using the RECFAST 1.5 and version 4.1 of the WMAP[WMAP-7likelihood 1001.4538] code.
    [Show full text]
  • University of California Santa Cruz Quantum
    UNIVERSITY OF CALIFORNIA SANTA CRUZ QUANTUM GRAVITY AND COSMOLOGY A dissertation submitted in partial satisfaction of the requirements for the degree of DOCTOR OF PHILOSOPHY in PHYSICS by Lorenzo Mannelli September 2005 The Dissertation of Lorenzo Mannelli is approved: Professor Tom Banks, Chair Professor Michael Dine Professor Anthony Aguirre Lisa C. Sloan Vice Provost and Dean of Graduate Studies °c 2005 Lorenzo Mannelli Contents List of Figures vi Abstract vii Dedication viii Acknowledgments ix I The Holographic Principle 1 1 Introduction 2 2 Entropy Bounds for Black Holes 6 2.1 Black Holes Thermodynamics ........................ 6 2.1.1 Area Theorem ............................ 7 2.1.2 No-hair Theorem ........................... 7 2.2 Bekenstein Entropy and the Generalized Second Law ........... 8 2.2.1 Hawking Radiation .......................... 10 2.2.2 Bekenstein Bound: Geroch Process . 12 2.2.3 Spherical Entropy Bound: Susskind Process . 12 2.2.4 Relation to the Bekenstein Bound . 13 3 Degrees of Freedom and Entropy 15 3.1 Degrees of Freedom .............................. 15 3.1.1 Fundamental System ......................... 16 3.2 Complexity According to Local Field Theory . 16 3.3 Complexity According to the Spherical Entropy Bound . 18 3.4 Why Local Field Theory Gives the Wrong Answer . 19 4 The Covariant Entropy Bound 20 4.1 Light-Sheets .................................. 20 iii 4.1.1 The Raychaudhuri Equation .................... 20 4.1.2 Orthogonal Null Hypersurfaces ................... 24 4.1.3 Light-sheet Selection ......................... 26 4.1.4 Light-sheet Termination ....................... 28 4.2 Entropy on a Light-Sheet .......................... 29 4.3 Formulation of the Covariant Entropy Bound . 30 5 Quantum Field Theory in Curved Spacetime 32 5.1 Scalar Field Quantization .........................
    [Show full text]
  • States with Regards to Finding If the Cosmological Constant Is, Or Is Not a ‘Vacuum’ Field Andrew Beckwith, [email protected]
    Consequences of squeezing initially coherent (semi classical) states with regards to finding if the cosmological constant is, or is not a ‘vacuum’ field Andrew Beckwith, [email protected], Abstract The following document is to prepare an analysis on if the cosmological constant is a vacuum field. Candidates for how to analyze this issue come up in terms of brane theory, modified treatments of WdM theory (pseudo time component added) and/ or how to look at squeezing of vacuum states, as initially coherent semi classical constructions, or string theory versions of coherent states. The article presents a thought experiment if there is a non zero graviton mass, and at the end, in the conclusion states experimental modeling criteria which may indicate if a non zero graviton mass is measurable, which would indicate the existence, de facto of a possible replacement for DE, based upon non zero mass gravitons, and indications for a replacement for a cosmological constant. Introduction: Dr. Karim1 mailed the author with the following question which will be put in quotes: The challenge of resolving the following question: At the Big Bang the only form of energy released is in the form of geometry – gravity. intense gravity field lifts vacuum fields to positive energies, So an electromagnetic vacuum of density 10122 kg/m3 should collapse under its own gravity. But this does not happen - that is one reason why the cosmological constant cannot be the vacuum field. Why? Answering this question delves into what the initial state of the universe should be, in terms of either vacuum energy, or something else.
    [Show full text]
  • On the Limits of Effective Quantum Field Theory
    RUNHETC-2019-15 On the Limits of Effective Quantum Field Theory: Eternal Inflation, Landscapes, and Other Mythical Beasts Tom Banks Department of Physics and NHETC Rutgers University, Piscataway, NJ 08854 E-mail: [email protected] Abstract We recapitulate multiple arguments that Eternal Inflation and the String Landscape are actually part of the Swampland: ideas in Effective Quantum Field Theory that do not have a counterpart in genuine models of Quantum Gravity. 1 Introduction Most of the arguments and results in this paper are old, dating back a decade, and very little of what is written here has not been published previously, or presented in talks. I was motivated to write this note after spending two weeks at the Vacuum Energy and Electroweak Scale workshop at KITP in Santa Barbara. There I found a whole new generation of effective field theorists recycling tired ideas from the 1980s about the use of effective field theory in gravitational contexts. These were ideas that I once believed in, but since the beginning of the 21st century my work in string theory and the dynamics of black holes, convinced me that they arXiv:1910.12817v2 [hep-th] 6 Nov 2019 were wrong. I wrote and lectured about this extensively in the first decade of the century, but apparently those arguments have not been accepted, and effective field theorists have concluded that the main lesson from string theory is that there is a vast landscape of meta-stable states in the theory of quantum gravity, connected by tunneling transitions in the manner envisioned by effective field theorists in the 1980s.
    [Show full text]
  • Geometric Origin of Coincidences and Hierarchies in the Landscape
    Geometric origin of coincidences and hierarchies in the landscape The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Bousso, Raphael et al. “Geometric origin of coincidences and hierarchies in the landscape.” Physical Review D 84.8 (2011): n. pag. Web. 26 Jan. 2012. © 2011 American Physical Society As Published http://dx.doi.org/10.1103/PhysRevD.84.083517 Publisher American Physical Society (APS) Version Final published version Citable link http://hdl.handle.net/1721.1/68666 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PHYSICAL REVIEW D 84, 083517 (2011) Geometric origin of coincidences and hierarchies in the landscape Raphael Bousso,1,2 Ben Freivogel,3 Stefan Leichenauer,1,2 and Vladimir Rosenhaus1,2 1Center for Theoretical Physics and Department of Physics, University of California, Berkeley, California 94720-7300, USA 2Lawrence Berkeley National Laboratory, Berkeley, California 94720-8162, USA 3Center for Theoretical Physics and Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA (Received 2 August 2011; published 14 October 2011) We show that the geometry of cutoffs on eternal inflation strongly constrains predictions for the time scales of vacuum domination, curvature domination, and observation. We consider three measure proposals: the causal patch, the fat geodesic, and the apparent horizon cutoff, which is introduced here for the first time. We impose neither anthropic requirements nor restrictions on landscape vacua. For vacua with positive cosmological constant, all three measures predict the double coincidence that most observers live at the onset of vacuum domination and just before the onset of curvature domination.
    [Show full text]
  • Arxiv:Hep-Th/0209231 V1 26 Sep 2002 Tbs,Daai N Uigi Eurdfrsae Te Hntetemlvcu Olead to Vacuum Thermal the Anisotropy
    SLAC-PUB-9533 BRX TH-505 October 2002 SU-ITP-02/02 Initial conditions for inflation Nemanja Kaloper1;2, Matthew Kleban1, Albion Lawrence1;3;4, Stephen Shenker1 and Leonard Susskind1 1Department of Physics, Stanford University, Stanford, CA 94305 2Department of Physics, University of California, Davis, CA 95616 3Brandeis University Physics Department, MS 057, POB 549110, Waltham, MA 02454y 4SLAC Theory Group, MS 81, 2575 Sand Hill Road, Menlo Park, CA 94025 Free scalar fields in de Sitter space have a one-parameter family of states invariant under the de Sitter group, including the standard thermal vacuum. We show that, except for the thermal vacuum, these states are unphysical when gravitational interactions are arXiv:hep-th/0209231 v1 26 Sep 2002 included. We apply these observations to the quantum state of the inflaton, and find that at best, dramatic fine tuning is required for states other than the thermal vacuum to lead to observable features in the CMBR anisotropy. y Present and permanent address. *Work supported in part by Department of Energy Contract DE-AC03-76SF00515. 1. Introduction In inflationary cosmology, cosmic microwave background (CMB) data place a tanta- lizing upper bound on the vacuum energy density during the inflationary epoch: 4 V M 4 1016 GeV : (1:1) ∼ GUT ∼ Here MGUT is the \unification scale" in supersymmetric grand unified models, as predicted by the running of the observed strong, weak and electromagnetic couplings above 1 T eV in the minimal supersymmetric standard model. If this upper bound is close to the truth, the vacuum energy can be measured directly with detectors sensitive to the polarization of the CMBR.
    [Show full text]
  • Geometric Approaches to Quantum Field Theory
    GEOMETRIC APPROACHES TO QUANTUM FIELD THEORY A thesis submitted to The University of Manchester for the degree of Doctor of Philosophy in the Faculty of Science and Engineering 2020 Kieran T. O. Finn School of Physics and Astronomy Supervised by Professor Apostolos Pilaftsis BLANK PAGE 2 Contents Abstract 7 Declaration 9 Copyright 11 Acknowledgements 13 Publications by the Author 15 1 Introduction 19 1.1 Unit Independence . 20 1.2 Reparametrisation Invariance in Quantum Field Theories . 24 1.3 Example: Complex Scalar Field . 25 1.4 Outline . 31 1.5 Conventions . 34 2 Field Space Covariance 35 2.1 Riemannian Geometry . 35 2.1.1 Manifolds . 35 2.1.2 Tensors . 36 2.1.3 Connections and the Covariant Derivative . 37 2.1.4 Distances on the Manifold . 38 2.1.5 Curvature of a Manifold . 39 2.1.6 Local Normal Coordinates and the Vielbein Formalism 41 2.1.7 Submanifolds and Induced Metrics . 42 2.1.8 The Geodesic Equation . 42 2.1.9 Isometries . 43 2.2 The Field Space . 44 2.2.1 Interpretation of the Field Space . 48 3 2.3 The Configuration Space . 50 2.4 Parametrisation Dependence of Standard Approaches to Quan- tum Field Theory . 52 2.4.1 Feynman Diagrams . 53 2.4.2 The Effective Action . 56 2.5 Covariant Approaches to Quantum Field Theory . 59 2.5.1 Covariant Feynman Diagrams . 59 2.5.2 The Vilkovisky–DeWitt Effective Action . 62 2.6 Example: Complex Scalar Field . 66 3 Frame Covariance in Quantum Gravity 69 3.1 The Cosmological Frame Problem .
    [Show full text]
  • 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.
    [Show full text]
  • Arxiv:1707.01092V2 [Gr-Qc]
    September 2017 Holographic Entanglement Entropy and Cyclic Cosmology Paul H. Frampton∗ Dipartimento di Matematica e Fisica ”Ennio De Giorgi” Universit`adel Salento and INFN Lecce, Via Arnesano 73100 Lecce,Italy. Abstract We discuss a cyclic cosmology in which the visible universe, or introverse, is all that is accessible to an observer while the extroverse represents the total spacetime originating from the time when the dark energy began to dominate. It is argued that entanglement entropy of the introverse is the more appropriate quantity to render infinitely cyclic, rather than the entropy of the total universe. Since vanishing entanglement entropy implies disconnected spacetimes, at the turnaround when the introverse entropy is zero the disconnected extroverse can be jettisoned with impunity. arXiv:1707.01092v2 [gr-qc] 1 Sep 2017 ∗email: [email protected] 1 Introduction Cyclic cosmology with an infinite number of cycles which include – expansion, turnaround, contraction, bounce – is an appealing theory, and one of the most recent attempts at a solution was in [1]. As emphasized first by Tolman [2,3], entropy and the second law of thermodynamics provide a significant challenge to implementing a cyclic theory. The approach was based on the so-called Come Back Empty (CBE) principle which chooses the turnaround as the point in the cycles where entropy is jettisoned. A successful universe must be selected with zero entropy at the turnaround to begin an adiabatic contraction to the bounce while empty of all matter including black holes. In this article we provide a better understanding of CBE based on the holographic principle [4–6].
    [Show full text]
  • Ads/CFT and Black Holes - Lecture 3
    2230-3 Spring School on Superstring Theory and Related Topics 28 March - 5 April, 2011 AdS/CFT and Black Holes - Lecture 3 A. MALONEY McGill University Montreal Canada A de Sitter Farey Tail ICTP Alex Maloney, McGill University Castro, Lashkari & A. M. Overview The Problem Quantum cosmology is confusing: What are the appropriate observables for eternal inflation? What is the meaning and origin of the entropy of a cosmological horizon? Is quantum mechanics the right language to describe cosmology? We were able to answer analogous questions about black hole physics using AdS/CFT. Let us be bold and apply the same techniques to cosmology. de Sitter Space de Sitter space is the maximally symmetric solution of general relativity with a positive cosmological constant. √ 1 − − 2 S(g)= g R 2 G M The universe inflates eternally. The three dimensional theory can be solved exactly, in the sense that the partition function − [ ] Z = Dge S g can be computed exactly. We will be inspired by AdS/CFT but we will not use it. The Idea The saddle point approximation is 1 −S[g] −kS0+S1+ S2+... Z = Dge = e k g0 where k = /G is the coupling. The approximation becomes exact if we can Find all classical saddles Compute all perturbative corrections around each saddle We can do it! The new classical saddles have a straightforward physical interpretation and lead to quantum gravitational effects for de Sitter observers. The Plan for Today: • The de Sitter Farey Tail • The Partition Function • Discussion Causal Structure of de Sitter Eternal inflation is the ultimate existential nightmare.
    [Show full text]
  • Xavier Calmet Editor Quantum Aspects of Black Holes Fundamental Theories of Physics
    Fundamental Theories of Physics 178 Xavier Calmet Editor Quantum Aspects of Black Holes Fundamental Theories of Physics Volume 178 Series editors Henk van Beijeren Philippe Blanchard Paul Busch Bob Coecke Dennis Dieks Detlef Dürr Roman Frigg Christopher Fuchs Giancarlo Ghirardi Domenico J.W. Giulini Gregg Jaeger Claus Kiefer Nicolaas P. Landsman Christian Maes Hermann Nicolai Vesselin Petkov Alwyn van der Merwe Rainer Verch R.F. Werner Christian Wuthrich More information about this series at http://www.springer.com/series/6001 Xavier Calmet Editor Quantum Aspects of Black Holes 123 Editor Xavier Calmet Department of Physics and Astronomy University of Sussex Brighton UK ISBN 978-3-319-10851-3 ISBN 978-3-319-10852-0 (eBook) DOI 10.1007/978-3-319-10852-0 Library of Congress Control Number: 2014951685 Springer Cham Heidelberg New York Dordrecht London © Springer International Publishing Switzerland 2015 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. Exempted from this legal reservation are brief excerpts in connection with reviews or scholarly analysis or material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Duplication of this publication or parts thereof is permitted only under the provisions of the Copyright Law of the Publisher’s location, in its current version, and permission for use must always be obtained from Springer.
    [Show full text]