PRIMORDIAL COSMOLOGY

Size: px
Start display at page:

Download "PRIMORDIAL COSMOLOGY"

Transcription

1 PRIMORDIAL COSMOLOGY Giovanni Montani ENEA - C.R. Frascati, ICFtANet and Dipartimento di Fisica, Universita di Roma "Sapienza", Italy Marco Valerio Battisti Dipartimento di Fisica, Universita di Roma "Sapienza", Italy and Centre de Physique Theorique, Luminy, Marseille, France Riccardo Benini ICRA and Dipartimento di Fisica," Universita di Roma "Sapienza", Italy Giovanni Imponente Queen Mary, University of London, UK World Scientific JERSEY. LONDON SINGAPORE- BEIJING SHANGHAI HONG KONG TAIPEI CHENNAI

2 Contents Preface List of Figures vii xxiii Historical and Basic Notions 1 1. Historical Picture 3 ''' 1.1 The Concept of Universe Through the Centuries... 3 < The ancient cultures... 3 i Ancient Greek and the Mediterranean 5 0" The Hellenistic era '.' I The philosophical point of view in the Old Age.. 11 I., " The Middle Age dogmas The Renaissance revolution ; The Scientific Revolution The Enlightenment Era The XIX Century Knowledge Geometrical formalisms Difficulties for the birth of a real cosmology: 01- bers' paradox / Luigi Bianchi and the developments of differential geometry Einstein vision of space-time Birth of Scientific Cosmology. 30 ' ' Einstein proposal of a static Universe... 31

3 dv f Primordial Cosmology Galaxies and their expansion: The Hubble's dis- ^ covery 1,4 The Genesis of the Hot Big Bang Model Recent developments' ^Discovery of the acceleration Generic nature of the cosmological singularity: The Cambridge and the Landau School The inflationary paradigm The idea of non-singular cosmology: The cyclic Universe and the Big Bounce 1.5 Guidelines to the Literature ; Fundamental Taols.' Einstein Equations Matter Fields.. : Perfect fluid Scalar field Electromagnetic field Yang-Mills fields and 9-sector Hamiltonian Formulation of the Dynamics Canonical General Relativity Hamilton-Jacobi equations for gravitational field The ADM reduction of the dynamics Synchronous Reference System. 2.5 Tetradic Formalism Gauge-like Formulation of GR Lagrangian formulation..., Hamiltonian formulation On the gauge group of GR Singularity Theorems...' Definition of a space-time singularity Fluid kinematics 273 The Raychaudhuri equation.. QO Singularity Theorems 2.8 Guidelines to the Literature... 64

4 Contents xv Physical Cosmology The Structure and Dynamics of the Isotropic Universe The RW Geometry Definition of isotropy Kinematics of the isotropic Universe The particle motion The Hubble law The Hubble length and the cosmological horizon Kinetic theory and thermodynamics in the expanding Universe: The hot Big Bang The FRW Cosmology....* Field equations for the isotropic Universe Asymptotic solution toward the Big Bang The de Sitter Solution Hamiltonian dynamics of the isotropic Universe Dissipative Cosmologies Bulk viscosity Matter creation in the expanding Universe Inhomogeneous Fluctuations in the Universe The meaning of cosmological perturbations The Jeans length in a static uniform fluid The Jeans length in an expanding Universe General Relativistic Perturbation Theory Perturbed Einstein equations Scalar-vector-tensor decomposition and Fourier expansion Perturbed conservation equations Gauge modes., Evolution of scalar modes.' 147 ; Adiabatic and isocurvature perturbations Imperfect fluids Kinetic theory The Lemaitre-Tolmann-Bondi Spherical Solution Guidelines to the Literature...'...' , Features of the Observed Universe 165 '- 4.1 Current Status: The Concordance Model. 166

5 xvi f Primordial Cosmology 4.2 The Large-Scale Structure Deviations from homogeneity Dark matter. ' The power spectrum of density fluctuations The Acceleration of the Universe The Cosmic Microwave Background Sources of anisotropy The power spectrum of CMB anisotropies Acoustic oscillations Effect of the cosmological parameters Guidelines to the Literature The Theory of Inflation The Shortcomings of the Standard Cosmology The horizon and flatness paradoxes The entropy problem and the unwanted relics paradox The Inflationary Paradigm Spontaneous symmetry breaking and the Higgs phenomenon Presence of a Self-interacting Scalar Field Coupling of the scalar field with the thermal bath Inflationary Dynamics Slow-rolling phase The reheating phase Solution to the Shortcomings of the Standard Cosmology Solution to the horizon and flatness paradoxes Solution to the entropy problem and to the unwanted relics paradox General Features : Slow-rolling phase Reheating phase '...: The Coleman-Weinberg model Genesis of the seeds for structure formation Possible Explanations for the Present Acceleration of the Universe, Dark energy Modified gravity theory Guidelines to the Literature 239

6 Contents xvii 6. Inhomogeneous Quasi-isotropic Cosmologies Quasi-isotropic Solution The Presence of Ultrarelativistic Matter The Role of a Massless Scalar Field The Role of an Electromagnetic Field Quasi-isotropic Inflation Geometry, matter and scalar field equations Inflationary dynamics Physical considerations Quasi-isotropic Viscous Solution Form of the energy density Comments on the adopted paradigm Solutions of the 00-Einstein and hydrodynamical equations The velocity and the three-metric Guidelines to the Literature...', '. 274 Mathematical Cosmology Homogeneous Universes Homogeneous Cosmological Models Definition of homogeneity Application to Cosmology Bianchi Classification and Line Element 286 ' ' ' 7.2 Kasner Solution 288? The role of matter 291 ' 7.3 The Dynamics of the Bianchi Models Bianchi type II: The concept of Kasner epoch.. 294! ' Bianchi type VII: The concept of Kasner era ; 7.4 Bianchi Types VIII and DC Models The oscillatory regime Stochastic properties and the Gaussian distribution Small oscillations 304 '' 7.5 Dynamical Systems Approach Equations for orthogonal Bianchi class A models. 310,". < The Bianchi I model and the Kasner circle ^ <' The Bianchi II model in vacuum. 315

7 xviii Primordial Cosmology The Bianchi IX model and the Mixmaster attractor theorem Multidimensional Homogeneous Universes On the non-diagonal cases Guidelines to the Literature Hamiltonian Formulation of the Mixmaster Hamiltonian Formulation of the Dynamics.: The Mixmaster Model in the Misner Variables Metric reparametrization Kasner solution, Lagrangian formulation Reduced ADM Hamiltonian Mixmaster dynamics Misner-Chitre Like Variables The Jacobi metric and the billiard representation Some remarks on the billiard representation The Invariant Liouville Measure Invariant Lyapunov Exponent Chaos Covariance.. ; Shortcomings of Lyapunov exponents On the occurrence of fractal basin Cosmological Chaos as a Dimensional and Matter Dependent Phenomenon 353 k The role of a scalar field The role of a vector field." Isotropization Mechanism ' Guidelines to the Literature The Generic Cosmological Solution Near the Singularity Inhomogeneous Perturbations of Bianchi IX Formulation of the Generic Cosmological Problem The Generalized Kasner solution Inhomogeneous BKL solution Rotation of the Kasner axes : The Fragmentation Process Physical meaning of the BKL conjecture The Generic Cosmological Solution in Misner Variables. 375

8 Contents xix 9.5 Hamiltonian Formulation in a General Framework Local dynamics.." Dynamics of inhomogeneities The Generic Cosmological Problem in the Iwasawa Variables Asymptotic freezing of the Iwasawa variables Cosmological billiards Multidimensional Oscillatory Regime Dilatons, p-forms and Kac-Moody algebras Properties of the BKL Map Parametrization in a generic number of dimensions Ordering properties Properties of the BKL map in the v space Guidelines to the Literature 398 Quantum Cosmology Standard Quantum Cosmology Quantum Geometrodynamics The Wheeler-DeWitt Theory Relation with the Path Integral Quantization The Problem of Time Time before quantization Time after quantization Timeless physics 419! ' 10.3 What is Quantum Cosmology? Minisuperspace models Interpretation of the theory Quantum singularity avoidance Path Integral in the Minisuperspace 427 ' 10.5 Scalar Field as Relational Time Interpretation of the Wave Function of the Universe The semiclassical approximation An example: A quantum mechanism for the isotropization of the Universe Boundary Conditions 441 * No-boundary proposal Tunneling proposal 445

9 XX Primordial Cosmology Comparison between the two approaches Quantization of the FRW Model Filled with a Scalar Field The Poincare Half Plane -J Quantum Dynamics of the Taub Universe Classical framework Quantum framework Quantization of the Mixmaster in the Misner Picture The Quantum Mixmaster in the Poincare Half Plane Continuity equation and the Liouville theorem Schrodinger dynamics Eigenfunctions and the vacuum state Properties of the spectrum Guidelines to the Literature Generalized Approaches to Quantum Mechanics The Algebraic Approach Basic elements GNS construction and Fell theorem Polymer Quantum Mechanics From Schrodinger to polymer representation Kinematics Dynamics 11 3 On the Existence of a Fundamental Scale String Theory and Generalized Uncertainty Principle Heisenberg Algebras in Non-Commutative Snyder Space- Time f a ] 11.6 Quantum Mechanics in the GUP Framework Guidelines to the Literature ~' Modern Quantum Cosmology 12.1 Loop Quantum Gravity Kinematics Implementation of the constraints Quantum constraints algebra Loop Quantum Cosmology 51i Kinematics Quantum dynamics and Big Bounce Effective classical dynamics

10 Contents. xxi 12.3 Mixmaster Universe in LQC Loop quantum Bianchi IX Effective dynamics Triangulated Loop Quantum Cosmology The triangulated model Isotropic sector: FRW Anisotropic sector: Bianchi LX Full dipole model Quantization of the model Snyder-Deformed Quantum Cosmology GUP and Polymer Quantum Cosmology: The Taub Universe Deformed classical dynamics Deformed quantum dynamics Mixmaster Universe in the GUP Approach Guidelines to the Literature 550 Bibliography 553 Index 585

COSMOLOGY The Origin and Evolution of Cosmic Structure

COSMOLOGY The Origin and Evolution of Cosmic Structure COSMOLOGY The Origin and Evolution of Cosmic Structure Peter COLES Astronomy Unit, Queen Mary & Westfield College, University of London, United Kingdom Francesco LUCCHIN Dipartimento di Astronomia, Universita

More information

PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in

PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in LONDON BEIJING HONG TSINGHUA Report and Review in Physics Vol2 PRINCIPLES OF PHYSICS From Quantum Field Theory to Classical Mechanics Ni Jun Tsinghua University, China NEW JERSEY \Hp SINGAPORE World Scientific

More information

Relativity, Gravitation, and Cosmology

Relativity, Gravitation, and Cosmology Relativity, Gravitation, and Cosmology A basic introduction TA-PEI CHENG University of Missouri St. Louis OXFORD UNIVERSITY PRESS Contents Parti RELATIVITY Metric Description of Spacetime 1 Introduction

More information

The Theory of Inflationary Perturbations

The Theory of Inflationary Perturbations The Theory of Inflationary Perturbations Jérôme Martin Institut d Astrophysique de Paris (IAP) Indian Institute of Technology, Chennai 03/02/2012 1 Introduction Outline A brief description of inflation

More information

IoP. An Introduction to the Science of Cosmology. Derek Raine. Ted Thomas. Series in Astronomy and Astrophysics

IoP. An Introduction to the Science of Cosmology. Derek Raine. Ted Thomas. Series in Astronomy and Astrophysics Series in Astronomy and Astrophysics An Introduction to the Science of Cosmology Derek Raine Department of Physics and Astronomy University of Leicester, UK Ted Thomas Department of Physics and Astronomy

More information

Patrick Peter. Institut d Astrophysique de Paris Institut Lagrange de Paris. Evidences for inflation constraints on alternatives

Patrick Peter. Institut d Astrophysique de Paris Institut Lagrange de Paris. Evidences for inflation constraints on alternatives Patrick Peter Institut d Astrophysique de Paris Institut Lagrange de Paris Evidences for inflation constraints on alternatives Thanks to Jérôme Martin For his help Planck 2015 almost scale invariant quantum

More information

School Observational Cosmology Angra Terceira Açores 3 rd June Juan García-Bellido Física Teórica UAM Madrid, Spain

School Observational Cosmology Angra Terceira Açores 3 rd June Juan García-Bellido Física Teórica UAM Madrid, Spain School Observational Cosmology Angra Terceira Açores 3 rd June 2014 Juan García-Bellido Física Teórica UAM Madrid, Spain Outline Lecture 1 Shortcomings of the Hot Big Bang The Inflationary Paradigm Homogeneous

More information

Research Center for the Early Universe (RESCEU) Department of Physics. Jun ichi Yokoyama

Research Center for the Early Universe (RESCEU) Department of Physics. Jun ichi Yokoyama Research Center for the Early Universe (RESCEU) Department of Physics Jun ichi Yokoyama time size Today 13.8Gyr Why is Our Universe Big, dark energy Old, and full of structures? galaxy formation All of

More information

The BKL proposal and cosmic censorship

The BKL proposal and cosmic censorship - 1 - The BKL proposal and cosmic censorship Lars Andersson University of Miami and Albert Einstein Institute (joint work with Henk van Elst, Claes Uggla and Woei-Chet Lim) References: Gowdy phenomenology

More information

Graceful exit from inflation for minimally coupled Bianchi A scalar field models

Graceful exit from inflation for minimally coupled Bianchi A scalar field models Graceful exit from inflation for minimally coupled Bianchi A scalar field models Florian Beyer Reference: F.B. and Leon Escobar (2013), CQG, 30(19), p.195020. University of Otago, Dunedin, New Zealand

More information

Inflation and the Primordial Perturbation Spectrum

Inflation and the Primordial Perturbation Spectrum PORTILLO 1 Inflation and the Primordial Perturbation Spectrum Stephen K N PORTILLO Introduction The theory of cosmic inflation is the leading hypothesis for the origin of structure in the universe. It

More information

Scale symmetry a link from quantum gravity to cosmology

Scale symmetry a link from quantum gravity to cosmology Scale symmetry a link from quantum gravity to cosmology scale symmetry fluctuations induce running couplings violation of scale symmetry well known in QCD or standard model Fixed Points Quantum scale symmetry

More information

Archaeology of Our Universe YIFU CAI ( 蔡一夫 )

Archaeology of Our Universe YIFU CAI ( 蔡一夫 ) Archaeology of Our Universe YIFU CAI ( 蔡一夫 ) 2013-11-05 Thermal History Primordial era 13.8 billion years by WMAP/NASA Large Scale Structure (LSS) by 2MASS Cosmic Microwave Background (CMB) by ESA/Planck

More information

Structures in the early Universe. Particle Astrophysics chapter 8 Lecture 4

Structures in the early Universe. Particle Astrophysics chapter 8 Lecture 4 Structures in the early Universe Particle Astrophysics chapter 8 Lecture 4 overview Part 1: problems in Standard Model of Cosmology: horizon and flatness problems presence of structures Part : Need for

More information

MASAHIDE YAMAGUCHI. Quantum generation of density perturbations in the early Universe. (Tokyo Institute of Technology)

MASAHIDE YAMAGUCHI. Quantum generation of density perturbations in the early Universe. (Tokyo Institute of Technology) Quantum generation of density perturbations in the early Universe MASAHIDE YAMAGUCHI (Tokyo Institute of Technology) 03/07/16@Symposium: New Generation Quantum Theory -Particle Physics, Cosmology, and

More information

Emergent Universe by Tunneling. Pedro Labraña, ICC, Universidad de Barcelona and Facultad de Ciencias, Universidad del Bío-Bío, Chile.

Emergent Universe by Tunneling. Pedro Labraña, ICC, Universidad de Barcelona and Facultad de Ciencias, Universidad del Bío-Bío, Chile. Emergent Universe by Tunneling Pedro Labraña, ICC, Universidad de Barcelona and Facultad de Ciencias, Universidad del Bío-Bío, Chile. The Emergent Universe scenario Is Eternal Inflation, past eternal?

More information

4 Evolution of density perturbations

4 Evolution of density perturbations Spring term 2014: Dark Matter lecture 3/9 Torsten Bringmann (torsten.bringmann@fys.uio.no) reading: Weinberg, chapters 5-8 4 Evolution of density perturbations 4.1 Statistical description The cosmological

More information

Contents. Part I The Big Bang and the Observable Universe

Contents. Part I The Big Bang and the Observable Universe Contents Part I The Big Bang and the Observable Universe 1 A Historical Overview 3 1.1 The Big Cosmic Questions 3 1.2 Origins of Scientific Cosmology 4 1.3 Cosmology Today 7 2 Newton s Universe 13 2.1

More information

Cosmology Winter School 5/12/2011! Jean-Philippe UZAN!

Cosmology Winter School 5/12/2011! Jean-Philippe UZAN! Cosmology Winter School 5/12/2011! Lecture 1:! Cosmological models! Jean-Philippe UZAN! Cosmological models! We work in the framework of general relativity so that the Universe is described by a spacetime

More information

Quantum gravity and aspects of relativity

Quantum gravity and aspects of relativity Quantum gravity and aspects of relativity Branislav Nikolic Institute for Theoretical Physics, University of Cologne Bonn-Cologne Graduate School in Physics and Astronomy who are we??? Gravitation and

More information

PoS(FFP14)170. Loop Quantum Effects on a Viscous Dark Energy Cosmological Model. N.Mebarki1. S.Benchick

PoS(FFP14)170. Loop Quantum Effects on a Viscous Dark Energy Cosmological Model. N.Mebarki1. S.Benchick Loop Quantum Effects on a Viscous Dark Energy Cosmological Model Laboratoire de Physique Mathematique et Subatomique, Mentouri University Route Ain El Bey, Constantine 25000, Algeria E-mail: nnmebarki@yahoo.fr

More information

Stephen Blaha, Ph.D. M PubHsMtw

Stephen Blaha, Ph.D. M PubHsMtw Quantum Big Bang Cosmology: Complex Space-time General Relativity, Quantum Coordinates,"Dodecahedral Universe, Inflation, and New Spin 0, 1 / 2,1 & 2 Tachyons & Imagyons Stephen Blaha, Ph.D. M PubHsMtw

More information

Non-singular quantum cosmology and scale invariant perturbations

Non-singular quantum cosmology and scale invariant perturbations th AMT Toulouse November 6, 2007 Patrick Peter Non-singular quantum cosmology and scale invariant perturbations Institut d Astrophysique de Paris GRεCO AMT - Toulouse - 6th November 2007 based upon Tensor

More information

Cosmology Course Gustavo Niz

Cosmology Course Gustavo Niz Cosmology Course Gustavo Niz Camille Flammarion L'atmosphère: météorologie populaire Content Brief history & scales Observations & the Understanding the CMB Inflation and the early Universe (EFTs in cosmology

More information

Connecting Quarks to the Cosmos

Connecting Quarks to the Cosmos Connecting Quarks to the Cosmos Institute for Nuclear Theory 29 June to 10 July 2009 Inflationary Cosmology II Michael S. Turner Kavli Institute for Cosmological Physics The University of Chicago Michael

More information

The Big Crunch/Big Bang Transition. 1. Measure for inflation 2. Passing through singularities - no beginning proposal

The Big Crunch/Big Bang Transition. 1. Measure for inflation 2. Passing through singularities - no beginning proposal The Big Crunch/Big Bang Transition Neil Turok, Perimeter Institute 1. Measure for inflation 2. Passing through singularities - no beginning proposal 2 inflation * initial conditions * fine-tuned potentials

More information

Theoretical Astrophysics and Cosmology

Theoretical Astrophysics and Cosmology Theoretical Astrophysics and Cosmology What is COSMOLOGY? -The study of the Universe as a whole, namely as the collection of its matter/energy components and its constituent phenomena, and of its evolution.

More information

Primordial perturbations from inflation. David Langlois (APC, Paris)

Primordial perturbations from inflation. David Langlois (APC, Paris) Primordial perturbations from inflation David Langlois (APC, Paris) Cosmological evolution Homogeneous and isotropic Universe Einstein s equations Friedmann equations The Universe in the Past The energy

More information

Oddities of the Universe

Oddities of the Universe Oddities of the Universe Koushik Dutta Theory Division, Saha Institute Physics Department, IISER, Kolkata 4th November, 2016 1 Outline - Basics of General Relativity - Expanding FRW Universe - Problems

More information

Bianchi Type VI0 Inflationary Universe with Constant Deceleration Parameter and Flat Potential in General Relativity

Bianchi Type VI0 Inflationary Universe with Constant Deceleration Parameter and Flat Potential in General Relativity Advances in Astrophysics, Vol., No., May 7 https://dx.doi.org/.66/adap.7. 67 Bianchi ype VI Inflationary Universe with Constant Deceleration Parameter and Flat Potential in General Relativity Raj Bali

More information

INFLATION. - EARLY EXPONENTIAL PHASE OF GROWTH OF SCALE FACTOR (after T ~ TGUT ~ GeV)

INFLATION. - EARLY EXPONENTIAL PHASE OF GROWTH OF SCALE FACTOR (after T ~ TGUT ~ GeV) INFLATION - EARLY EXPONENTIAL PHASE OF GROWTH OF SCALE FACTOR (after T ~ TGUT ~ 10 15 GeV) -Phenomenologically similar to Universe with a dominant cosmological constant, however inflation needs to end

More information

COSMIC INFLATION AND THE REHEATING OF THE UNIVERSE

COSMIC INFLATION AND THE REHEATING OF THE UNIVERSE COSMIC INFLATION AND THE REHEATING OF THE UNIVERSE Francisco Torrentí - IFT/UAM Valencia Students Seminars - December 2014 Contents 1. The Friedmann equations 2. Inflation 2.1. The problems of hot Big

More information

Closed Universes, de Sitter Space and Inflation

Closed Universes, de Sitter Space and Inflation Closed Universes, de Sitter Space and Inflation Chris Doran Cavendish Laboratory Based on astro-ph/0307311 by Lasenby and Doran The Cosmological Constant Dark energy responsible for around 70% of the total

More information

Electromagnetic spikes

Electromagnetic spikes Electromagnetic spikes Ernesto Nungesser (joint work with Woei Chet Lim) Trinity College Dublin ANZAMP, 29th of November, 2013 Overview Heuristic picture of initial singularity What is a Bianchi spacetime?

More information

PERTURBATIONS IN LOOP QUANTUM COSMOLOGY

PERTURBATIONS IN LOOP QUANTUM COSMOLOGY PERTURBATIONS IN LOOP QUANTUM COSMOLOGY William Nelson Pennsylvania State University Work with: Abhay Astekar and Ivan Agullo (see Ivan s ILQG talk, 29 th March ) AUTHOR, W. NELSON (PENN. STATE) PERTURBATIONS

More information

arxiv: v3 [gr-qc] 30 Mar 2009

arxiv: v3 [gr-qc] 30 Mar 2009 THE JEANS MECHANISM AND BULK-VISCOSITY EFFECTS Nakia Carlevaro a, b and Giovanni Montani b, c, d, e a Department of Physics, Polo Scientifico Università degli Studi di Firenze, INFN Section of Florence,

More information

The oldest science? One of the most rapidly evolving fields of modern research. Driven by observations and instruments

The oldest science? One of the most rapidly evolving fields of modern research. Driven by observations and instruments The oldest science? One of the most rapidly evolving fields of modern research. Driven by observations and instruments Intersection of physics (fundamental laws) and astronomy (contents of the universe)

More information

The multi-field facets of inflation. David Langlois (APC, Paris)

The multi-field facets of inflation. David Langlois (APC, Paris) The multi-field facets of inflation David Langlois (APC, Paris) Introduction After 25 years of existence, inflation has been so far very successful to account for observational data. The nature of the

More information

Space, time, Spacetime

Space, time, Spacetime Space, time, Spacetime Marc September 28, 2011 1 The vanishing of time A? 2 Time ersatz in GR special relativity general relativity Time in general relativity Proper in GR 3 4 5 gravity and Outline The

More information

Inflationary model building, reconstructing parameters and observational limits

Inflationary model building, reconstructing parameters and observational limits Inflationary model building, reconstructing parameters and observational limits Sayantan Choudhury Physics and Applied Mathematics Unit Indian Statistical Institute, Kolkata Date: 30/09/2014 Contact: sayanphysicsisi@gmail.com

More information

Cosmology: An Introduction. Eung Jin Chun

Cosmology: An Introduction. Eung Jin Chun Cosmology: An Introduction Eung Jin Chun Cosmology Hot Big Bang + Inflation. Theory of the evolution of the Universe described by General relativity (spacetime) Thermodynamics, Particle/nuclear physics

More information

Effects of the field-space metric on Spiral Inflation

Effects of the field-space metric on Spiral Inflation Effects of the field-space metric on Spiral Inflation Josh Erlich College of William & Mary digitaldante.columbia.edu Miami 2015 December 20, 2015 The Cosmic Microwave Background Planck collaboration Composition

More information

VU lecture Introduction to Particle Physics. Thomas Gajdosik, FI & VU. Big Bang (model)

VU lecture Introduction to Particle Physics. Thomas Gajdosik, FI & VU. Big Bang (model) Big Bang (model) What can be seen / measured? basically only light _ (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)

More information

Inflationary Massive Gravity

Inflationary Massive Gravity New perspectives on cosmology APCTP, 15 Feb., 017 Inflationary Massive Gravity Misao Sasaki Yukawa Institute for Theoretical Physics, Kyoto University C. Lin & MS, PLB 75, 84 (016) [arxiv:1504.01373 ]

More information

Towards a new scenario of inflationary magnetogenesis. Shinji Mukohyama (YITP, Kyoto U) Based on PRD94, 12302(R) (2016)

Towards a new scenario of inflationary magnetogenesis. Shinji Mukohyama (YITP, Kyoto U) Based on PRD94, 12302(R) (2016) Towards a new scenario of inflationary magnetogenesis Shinji Mukohyama (YITP, Kyoto U) Based on PRD94, 12302(R) (2016) Why modified gravity? Inflation Dark Energy Big Bang Singularity Dark Matter http://map.gsfc.nasa.gov/

More information

Pedro and the WOLF: the quantum and the vacuum in cosmology

Pedro and the WOLF: the quantum and the vacuum in cosmology Pedro's Universes, 4 December 2018 Guillermo A. Mena Marugán, IEM-CSIC Pedro and the WOLF: the quantum and the vacuum in cosmology Pedro's Universes, 4 December 2018 Guillermo A. Mena Marugán, IEM-CSIC

More information

Fundamentals of Neutrino Physics and Astrophysics

Fundamentals of Neutrino Physics and Astrophysics Fundamentals of Neutrino Physics and Astrophysics Carlo Giunti Istituto Nazionale di Fisica Nucleare, Sezione di Torino and Dipartimento di Fisica Teorica, Universita di Torino, Italy Chung W. Kim Korea

More information

Stable violation of the null energy condition and non-standard cosmologies

Stable violation of the null energy condition and non-standard cosmologies Paolo Creminelli (ICTP, Trieste) Stable violation of the null energy condition and non-standard cosmologies hep-th/0606090 with M. Luty, A. Nicolis and L. Senatore What is the NEC? Energy conditions: Singularity

More information

Modern Cosmology / Scott Dodelson Contents

Modern Cosmology / Scott Dodelson Contents Modern Cosmology / Scott Dodelson Contents The Standard Model and Beyond p. 1 The Expanding Universe p. 1 The Hubble Diagram p. 7 Big Bang Nucleosynthesis p. 9 The Cosmic Microwave Background p. 13 Beyond

More information

German physicist stops Universe

German physicist stops Universe Big bang or freeze? NATURE NEWS Cosmologist claims Universe may not be expanding Particles' changing masses could explain why distant galaxies appear to be rushing away. Jon Cartwright 16 July 2013 German

More information

Modern Geometric Structures and Fields

Modern Geometric Structures and Fields Modern Geometric Structures and Fields S. P. Novikov I.A.TaJmanov Translated by Dmitry Chibisov Graduate Studies in Mathematics Volume 71 American Mathematical Society Providence, Rhode Island Preface

More information

PAPER 71 COSMOLOGY. Attempt THREE questions There are seven questions in total The questions carry equal weight

PAPER 71 COSMOLOGY. Attempt THREE questions There are seven questions in total The questions carry equal weight MATHEMATICAL TRIPOS Part III Friday 31 May 00 9 to 1 PAPER 71 COSMOLOGY Attempt THREE questions There are seven questions in total The questions carry equal weight You may make free use of the information

More information

Black Hole Physics. Basic Concepts and New Developments KLUWER ACADEMIC PUBLISHERS. Valeri P. Frolov. Igor D. Nbvikov. and

Black Hole Physics. Basic Concepts and New Developments KLUWER ACADEMIC PUBLISHERS. Valeri P. Frolov. Igor D. Nbvikov. and Black Hole Physics Basic Concepts and New Developments by Valeri P. Frolov Department of Physics, University of Alberta, Edmonton, Alberta, Canada and Igor D. Nbvikov Theoretical Astrophysics Center, University

More information

Quantum cosmology from spinfoam theory

Quantum cosmology from spinfoam theory 1 DOTTORATO DI RICERCA IN FISICA, XXX CICLO PROGETTO DETTAGLIATO DI TESI Quantum cosmology from spinfoam theory Candidate: Gabriele Vittorio Stagno, Supervisors: proff. Giovanni Montani, Carlo Rovelli

More information

Microcosmo e Macrocosmo

Microcosmo e Macrocosmo Microcosmo e Macrocosmo Paolo de Bernardis Dipartimento di Fisica Sapienza Università di Roma Lezioni della Cattedra Fermi 23 Gennaio 2014 Dipartimento di Fisica Sapienza Università di Roma Friedman s

More information

List of Comprehensive Exams Topics

List of Comprehensive Exams Topics List of Comprehensive Exams Topics Mechanics 1. Basic Mechanics Newton s laws and conservation laws, the virial theorem 2. The Lagrangian and Hamiltonian Formalism The Lagrange formalism and the principle

More information

Quantum. Mechanics. Y y. A Modern Development. 2nd Edition. Leslie E Ballentine. World Scientific. Simon Fraser University, Canada TAIPEI BEIJING

Quantum. Mechanics. Y y. A Modern Development. 2nd Edition. Leslie E Ballentine. World Scientific. Simon Fraser University, Canada TAIPEI BEIJING BEIJING TAIPEI Quantum Mechanics A Modern Development 2nd Edition Leslie E Ballentine Simon Fraser University, Canada Y y NEW JERSEY LONDON SINGAPORE World Scientific SHANGHAI HONG KONG CHENNAI Contents

More information

Tensor Calculus, Relativity, and Cosmology

Tensor Calculus, Relativity, and Cosmology Tensor Calculus, Relativity, and Cosmology A First Course by M. Dalarsson Ericsson Research and Development Stockholm, Sweden and N. Dalarsson Royal Institute of Technology Stockholm, Sweden ELSEVIER ACADEMIC

More information

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016

Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 We are directly observing the history of the universe as we look deeply into the sky. JUN 30, 2016 ZZXianyu (CMSA) 2 At ~10 4 yrs the universe becomes

More information

Lecture Notes on General Relativity

Lecture Notes on General Relativity Lecture Notes on General Relativity Matthias Blau Albert Einstein Center for Fundamental Physics Institut für Theoretische Physik Universität Bern CH-3012 Bern, Switzerland The latest version of these

More information

Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION. Wolfgang Rindler. Professor of Physics The University of Texas at Dallas

Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION. Wolfgang Rindler. Professor of Physics The University of Texas at Dallas Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION Wolfgang Rindler Professor of Physics The University of Texas at Dallas OXPORD UNIVERSITY PRESS Contents Introduction l 1 From absolute space

More information

1 Introduction QUANTUM BIRTH OF A HOT UNIVERSE

1 Introduction QUANTUM BIRTH OF A HOT UNIVERSE QUANTUM BIRTH OF A HOT UNIVERSE I.G. Dymnikova Institute of Mathematics, Informatics and Physics, University of Olsztyn, Żo lnierska 4, 0-56, Olsztyn, Poland; e-mail: irina@matman.uwn.edu.pl M.L. Fil chenkov

More information

General Relativity (2nd part)

General Relativity (2nd part) General Relativity (2nd part) Electromagnetism Remember Maxwell equations Conservation Electromagnetism Can collect E and B in a tensor given by And the charge density Can be constructed from and current

More information

Exact Solution of an Ekpyrotic Fluid and a Primordial Magnetic Field in an Anisotropic Cosmological Space-Time of Petrov D

Exact Solution of an Ekpyrotic Fluid and a Primordial Magnetic Field in an Anisotropic Cosmological Space-Time of Petrov D Advanced Studies in Theoretical Physics Vol. 11, 2017, no. 12, 601-608 HIKARI Ltd, www.m-hikari.com https://doi.org/10.12988/astp.2017.7835 Exact Solution of an Ekpyrotic Fluid and a Primordial Magnetic

More information

EQUATION LANGEVIN. Physics, Chemistry and Electrical Engineering. World Scientific. With Applications to Stochastic Problems in. William T.

EQUATION LANGEVIN. Physics, Chemistry and Electrical Engineering. World Scientific. With Applications to Stochastic Problems in. William T. SHANGHAI HONG WorlrfScientific Series krtonttimfjorary Chemical Physics-Vol. 27 THE LANGEVIN EQUATION With Applications to Stochastic Problems in Physics, Chemistry and Electrical Engineering Third Edition

More information

A Field Theory approach to important Cosmological Issues including Dark Energy and the. Energy -Anupam Singh, L.N.M. I.I.T.

A Field Theory approach to important Cosmological Issues including Dark Energy and the. Energy -Anupam Singh, L.N.M. I.I.T. A Field Theory approach to important Cosmological Issues including Dark Energy and the gravitational collapse of Dark Energy -Anupam Singh, L.N.M. I.I.T. Outline Introduction and Motivation Field Theory:

More information

Introduction to Cosmology

Introduction to Cosmology Introduction to Cosmology Subir Sarkar CERN Summer training Programme, 22-28 July 2008 Seeing the edge of the Universe: From speculation to science Constructing the Universe: The history of the Universe:

More information

Cosmic Inflation Lecture 16 - Monday Mar 10

Cosmic Inflation Lecture 16 - Monday Mar 10 Physics 224 Spring 2008 Origin and Evolution of the Universe Cosmic Inflation Lecture 16 - Monday Mar 10 Joel Primack University of California, Santa Cruz Outline L15 L16 WMAP 5-year Data and Papers Released

More information

Key: cosmological perturbations. With the LHC, we hope to be able to go up to temperatures T 100 GeV, age t second

Key: cosmological perturbations. With the LHC, we hope to be able to go up to temperatures T 100 GeV, age t second Lecture 3 With Big Bang nucleosynthesis theory and observations we are confident of the theory of the early Universe at temperatures up to T 1 MeV, age t 1 second With the LHC, we hope to be able to go

More information

Nonsingular big-bounce cosmology from spin and torsion

Nonsingular big-bounce cosmology from spin and torsion Nonsingular big-bounce cosmology from spin and torsion Nikodem J. Popławski Department of Physics, Indiana University, Bloomington, IN 22 nd Midwest Relativity Meeting University of Chicago, Chicago, IL

More information

Gravity, Strings and Branes

Gravity, Strings and Branes Gravity, Strings and Branes Joaquim Gomis Universitat Barcelona Miami, 23 April 2009 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model Basic building blocks, quarks,

More information

The Search for the Complete History of the Cosmos. Neil Turok

The Search for the Complete History of the Cosmos. Neil Turok The Search for the Complete History of the Cosmos Neil Turok * The Big Bang * Dark Matter and Energy * Precision Tests * A Cyclic Universe? * Future Probes BIG Questions * What are the Laws of Nature?

More information

Quantum Mechanics: Foundations and Applications

Quantum Mechanics: Foundations and Applications Arno Böhm Quantum Mechanics: Foundations and Applications Third Edition, Revised and Enlarged Prepared with Mark Loewe With 96 Illustrations Springer-Verlag New York Berlin Heidelberg London Paris Tokyo

More information

State of the Universe Address

State of the Universe Address State of the Universe Address Prof. Scott Watson ( Syracuse University ) This talk is available online at: https://gswatson.expressions.syr.edu This research was supported in part by: Theoretical Cosmology

More information

Holographic Model of Cosmic (P)reheating

Holographic Model of Cosmic (P)reheating Holographic Model of Cosmic (P)reheating Yi-Fu Cai 蔡一夫 University of Science & Technology of China New perspectives on Cosmology, APCTP, Feb 13 th 2017 In collaboration with S. Lin, J. Liu & J. Sun, Based

More information

Physics Nobel Prize 2006

Physics Nobel Prize 2006 Physics Nobel Prize 2006 Ghanashyam Date The Institute of Mathematical Sciences, Chennai http://www.imsc.res.in shyam@imsc.res.in Nov 4, 2006. Organization of the Talk Organization of the Talk Nobel Laureates

More information

Intrinsic Time Quantum Geometrodynamics (ITQG)

Intrinsic Time Quantum Geometrodynamics (ITQG) Intrinsic Time Quantum Geometrodynamics (ITQG) Assistant Professor Eyo Ita Eyo Eyo Ita Physics Department LQG International Seminar United States Naval Academy Annapolis, MD 27 October, 2015 Outline of

More information

Theory of galaxy formation

Theory of galaxy formation Theory of galaxy formation Bibliography: Galaxy Formation and Evolution (Mo, van den Bosch, White 2011) Lectures given by Frank van den Bosch in Yale http://www.astro.yale.edu/vdbosch/teaching.html Theory

More information

Introduction to Inflation

Introduction to Inflation Introduction to Inflation Miguel Campos MPI für Kernphysik & Heidelberg Universität September 23, 2014 Index (Brief) historic background The Cosmological Principle Big-bang puzzles Flatness Horizons Monopoles

More information

Inflationary cosmology. Andrei Linde

Inflationary cosmology. Andrei Linde Inflationary cosmology Andrei Linde Problems of the Big Bang theory: What was before the Big Bang? Why is our universe so homogeneous? Why is it isotropic? Why its parts started expanding simultaneously?

More information

Exploring the Early Universe. Chapter Twenty-Nine. Guiding Questions. The Isotropy Problem

Exploring the Early Universe. Chapter Twenty-Nine. Guiding Questions. The Isotropy Problem Exploring the Early Universe Chapter Twenty-Nine Guiding Questions 1. Has the universe always expanded as it does today, or might it have suddenly inflated? 2. How did the fundamental forces of nature

More information

Triple unification of inflation, dark matter and dark energy

Triple unification of inflation, dark matter and dark energy Triple unification of inflation, dark matter and dark energy May 9, 2008 Leonard Susskind, The Anthropic Landscape of String Theory (2003) A. Liddle, A. Ureña-López, Inflation, dark matter and dark energy

More information

Chapter 9. Perturbations in the Universe

Chapter 9. Perturbations in the Universe Chapter 9 Perturbations in the Universe In this chapter the theory of linear perturbations in the universe are studied. 9.1 Differential Equations of Linear Perturbation in the Universe A covariant, linear,

More information

Intro to Inflationary Cosmology

Intro to Inflationary Cosmology Times are bad. Children no longer obey their parents and everyone is writing a book. Cicero, 43 BC Bruce A. Bassett Intro to Inflationary Cosmology SAAO & UCT Cosmic Problem 1 : Isotropy COBE satellite

More information

The early and late time acceleration of the Universe

The early and late time acceleration of the Universe The early and late time acceleration of the Universe Tomo Takahashi (Saga University) March 7, 2016 New Generation Quantum Theory -Particle Physics, Cosmology, and Chemistry- @Kyoto University The early

More information

CMB Polarization in Einstein-Aether Theory

CMB Polarization in Einstein-Aether Theory CMB Polarization in Einstein-Aether Theory Masahiro Nakashima (The Univ. of Tokyo, RESCEU) With Tsutomu Kobayashi (RESCEU) COSMO/CosPa 2010 Introduction Two Big Mysteries of Cosmology Dark Energy & Dark

More information

General Relativity Lecture 20

General Relativity Lecture 20 General Relativity Lecture 20 1 General relativity General relativity is the classical (not quantum mechanical) theory of gravitation. As the gravitational interaction is a result of the structure of space-time,

More information

I V E R S U N. The Hot Big Bang I T Y T H E O F E. Andrew Liddle R G. Image: NASA/WMAP Science Team

I V E R S U N. The Hot Big Bang I T Y T H E O F E. Andrew Liddle R G. Image: NASA/WMAP Science Team The Hot Big Bang Andrew Liddle T H E O F E U N D I I V E R S N U B R G I T Y H Image: NASA/WMAP Science Team The Standard Model The discovery of the Higgs particle completes the Standard Model of Particle

More information

Topics for the Qualifying Examination

Topics for the Qualifying Examination Topics for the Qualifying Examination Quantum Mechanics I and II 1. Quantum kinematics and dynamics 1.1 Postulates of Quantum Mechanics. 1.2 Configuration space vs. Hilbert space, wave function vs. state

More information

El Universo en Expansion. Juan García-Bellido Inst. Física Teórica UAM Benasque, 12 Julio 2004

El Universo en Expansion. Juan García-Bellido Inst. Física Teórica UAM Benasque, 12 Julio 2004 El Universo en Expansion Juan García-Bellido Inst. Física Teórica UAM Benasque, 12 Julio 2004 5 billion years (you are here) Space is Homogeneous and Isotropic General Relativity An Expanding Universe

More information

The Cosmological Principle

The Cosmological Principle Cosmological Models John O Byrne School of Physics University of Sydney Using diagrams and pp slides from Seeds Foundations of Astronomy and the Supernova Cosmology Project http://www-supernova.lbl.gov

More information

Astronomy 182: Origin and Evolution of the Universe

Astronomy 182: Origin and Evolution of the Universe Astronomy 182: Origin and Evolution of the Universe Prof. Josh Frieman Lecture 14 Dec. 2, 2015 Today The Inflationary Universe Origin of Density Perturbations Gravitational Waves Origin and Evolution of

More information

Modeling the Universe A Summary

Modeling the Universe A Summary Modeling the Universe A Summary Questions to Consider 1. What does the darkness of the night sky tell us about the nature of the universe? 2. As the universe expands, what, if anything, is it expanding

More information

Cosmic Bubble Collisions

Cosmic Bubble Collisions Outline Background Expanding Universe: Einstein s Eqn with FRW metric Inflationary Cosmology: model with scalar field QFTà Bubble nucleationà Bubble collisions Bubble Collisions in Single Field Theory

More information

The Evolving Cosmological Constant (Problem)

The Evolving Cosmological Constant (Problem) The Evolving Cosmological Constant (Problem) N. Itzhaki, (PU) PiPT 2006 Outline The CC problem: then and now (experimental hints). Abbott s model (85). Abbott s model string landscape + anthropic principle.

More information

Inflation. Week 9. ASTR/PHYS 4080: Introduction to Cosmology

Inflation. Week 9. ASTR/PHYS 4080: Introduction to Cosmology Inflation ASTR/PHYS 4080: Intro to Cosmology Week 9 1 Successes of the Hot Big Bang Model Consists of: General relativity Cosmological principle Known atomic/nuclear/particle physics Explains: dark night

More information

Graviton contributions to the graviton self-energy at one loop order during inflation

Graviton contributions to the graviton self-energy at one loop order during inflation Graviton contributions to the graviton self-energy at one loop order during inflation PEDRO J. MORA DEPARTMENT OF PHYSICS UNIVERSITY OF FLORIDA PASI2012 1. Description of my thesis problem. i. Graviton

More information

Cosmology OXFORD. Steven Weinberg. University of Texas at Austin UNIVERSITY PRESS

Cosmology OXFORD. Steven Weinberg. University of Texas at Austin UNIVERSITY PRESS Cosmology Steven Weinberg University of Texas at Austin OXFORD UNIVERSITY PRESS 1 THE EXPANSION OF THE UNIVERSE 1 1.1 Spacetime geometry 2 Robertson Walker metric 0 Co-moving coordinates q Proper distances

More information

Observational signatures in LQC?

Observational signatures in LQC? Observational signatures in LQC? Ivan Agullo Penn State International Loop Quantum Gravity Seminar, March 29 2011 Talk based on: I.A., A. Ashtekar, W. Nelson: IN PROGRESS! CONTENT OF THE TALK 1. Inflation

More information

The Early Universe John Peacock ESA Cosmic Vision Paris, Sept 2004

The Early Universe John Peacock ESA Cosmic Vision Paris, Sept 2004 The Early Universe John Peacock ESA Cosmic Vision Paris, Sept 2004 The history of modern cosmology 1917 Static via cosmological constant? (Einstein) 1917 Expansion (Slipher) 1952 Big Bang criticism (Hoyle)

More information