More on the analogy between disclinations and cosmic strings

Size: px
Start display at page:

Download "More on the analogy between disclinations and cosmic strings"

Transcription

1 More on the analogy between disclinations and cosmic strings Fernando Moraes Grupo de Matéria Condensada Mole e Física Biológica Departamento de Física Universidade Federal da Paraíba João Pessoa, PB Brazil UFCG p.1/17

2 genesis in the early universe, a sequence of symmetry-breaking phase transitions G H... SU(3) SU(2) U(1) SU(3) U(1) left behind topological defects (global monopoles, cosmic strings, domain walls, textures and other hybrid creatures) as relics of the higher temperature phases UFCG p.2/17

3 nematics symmetry-breaking phase transitions in liquid crystals SO(3) T(3) SO(2) T(3) SO(2) T(2) T 1 T 2 <T c T 3 TEMPERATURA also generate topological defects UFCG p.3/17

4 hedgehogs, disclinations, textures z y x they have been used as a laboratory for cosmology with respect to defect formation, evolution and dynamics T. Kibble Phase-transition dynamics in the lab and the universe Physics Today, Sept. 2007, p. 47 UFCG p.4/17

5 geometrical optics in nematics Kline & Kay: light rays in inhomogeneous anisotropic media are extremals of Fermat s functional Born & Wolf: light rays obeying Fermat s principle are geodesics in some Riemannian space N = n 2 ocos 2 (β) + n 2 esin 2 (β) UFCG p.5/17

6 effective geometry for light propagating near defects in nematics F = B A Ndl = B A i,j g ijdx i dx j C. Sátiro and F. Moraes Lensing effects in a nematic liquid crystal with topological defects, Eur. Phys. J. E 20 (2006)173 On the deflection of light by topological defects in nematic liquid crystals, Eur. Phys. J. E 25 (2008) 425 UFCG p.6/17

7 assorted line defects ϕ(θ) = kθ + c where k is the winding number and c = ϕ(0) UFCG p.7/17

8 line defect geometry we found ds 2 2D = {n2 o cos 2 [(k 1)θ + c] + n 2 e sin 2 [(k 1)θ + c]}dr 2 +{n 2 o sin 2 [(k 1)θ + c] + n 2 e cos 2 [(k 1)θ + c]}r 2 dθ 2 {2(n 2 e n 2 o) 2 sin[(k 1)θ + c] cos[(k 1)θ + c]}rdrdθ which, for n o = n e, reduces to the Euclidean line element ds 2 2D = dr2 + r 2 dθ 2 UFCG p.8/17

9 conical defect for k = 1, c = π/2 the effective geometry is conical: ds 2 2D = dr2 + α 2 r 2 dθ 2 where α = n o n e so is the spacetime of a cosmic string: ds 2 4D = dt2 dz 2 dr 2 α 2 r 2 dθ 2 where α = 1 4Gµ C. Sátiro and F. Moraes A liquid crystal analogue of the cosmic string Mod. Phys. Lett. A 20 (2005) 2561 UFCG p.9/17

10 curvature from the metric ds 2 2D = {n2 o cos 2 [(k 1)θ + c] + n 2 e sin 2 [(k 1)θ + c]}dr 2 +{n 2 o sin 2 [(k 1)θ + c] + n 2 e cos 2 [(k 1)θ + c]}r 2 dθ 2 {2(n 2 e n 2 o) 2 sin[(k 1)θ + c] cos[(k 1)θ + c]}rdrdθ we found that the only nonzero Riemann curvature tensor components are R rθrθ = R θrθr = R θrrθ = R rθθr = k(k 1)(n 2 e n 2 o) cos{2[(k 1)θ + c]} UFCG p.10/17

11 curvature and, for ξ(θ) = (k 1)θ + c, the curvature (Ricci) scalar is R = 2 α (1 α)δ(ρ) ρ for k = 1 and R = 2k α [ ( )] α + 1 δ(ρ) + 2k(k 1)(α2 1) cos(2ξ) for k 1 α ρ α 2 ρ 2 the idealized defects have a δ-function curvature singularity at ρ = 0 and for ρ 0 there is a ρ- and θ- dependent curvature as one goes around the defects the curvature alternates between positive and negative values UFCG p.11/17

12 curvature profile disclinations with k 1: k = 3 2, 1, 1 2, 1 2 and 2 UFCG p.12/17

13 asymmetric strings inspired by disclinations in nematics, we propose a new family of cosmic strings by writing ds 2 4D = dt2 dz 2 ds 2 2D Einstein equation R µν 1 2 g µνr = 8πGT µν gives us the energy-momentum tensor { Tt t = Tz z = 1 8πG k α + 2k(k 1)(1 α2 ) α 2 ρ 2 [ ( )] α + 1 δ(ρ) α ρ } cos {2 [(k 1)θ]} which is the source of the geometry associated to the string UFCG p.13/17

14 asymmetric strings contrasting to ordinary cosmic strings, the mass distribution profile of the asymmetric strings are not limited to an infinitely thin core alternate between positive and negative values as one circles the string they also lead to the same light paths as the disclinations in nematics C. Sátiro, A. M. de M. Carvalho and F. Moraes An asymmetric family of cosmic strings Int. J. Mod. Phys. D, under review UFCG p.14/17

15 conclusions the analogy between cosmic defects and defects in nematics goes beyond their formation, evolution and dynamics they are also analogous from the point of view of geometrical optics yet unknown cosmological defects have been proposed inspired by their nematic counterparts UFCG p.15/17

16 conclusions the geometrical approach is very handy when it comes to determine global properties like topological phases A. M. de M. Carvalho, C. Sátiro and F. Moraes Aharonov-Bohm-like effect for light propagating in nematics with disclinations Europhys. Lett. 80 (2007) UFCG p.16/17

17 acknowledgements Caio Sátiro (UFRPE, Brazil) Alexandre Carvalho (UEFS, Brazil) CNPq, CAPES/PROCAD, FAPESQ-PB, PRONEX (Brazilian agencies) UFCG p.17/17

arxiv: v1 [cond-mat.soft] 20 Sep 2007

arxiv: v1 [cond-mat.soft] 20 Sep 2007 epl draft Aharonov-Bohm-like effect for light propagating in nematics with disclinations arxiv:0709.3142v1 [cond-mat.soft] 20 Sep 2007 A. M. de M. Carvalho 1, C. Sátiro 2 and F. Moraes 2 1 Departamento

More information

Vacuum Polarization in the Presence of Magnetic Flux at Finite Temperature in the Cosmic String Background

Vacuum Polarization in the Presence of Magnetic Flux at Finite Temperature in the Cosmic String Background Vacuum Polarization in the Presence of Magnetic Flux at Finite Temperature in the Cosmic String Background Univ. Estadual da Paraíba (UEPB), Brazil E-mail: jeanspinelly@ig.com.br E. R. Bezerra de Mello

More information

Cosmic Strings. Joel Meyers

Cosmic Strings. Joel Meyers Cosmic Strings Joel Meyers Outline History and Motivations Topological Defects Formation of Cosmic String Networks Cosmic Strings from String Theory Observation and Implications Conclusion History In the

More information

Cosmic Strings. May 2, Safa Motesharrei University of Maryland

Cosmic Strings. May 2, Safa Motesharrei University of Maryland Safa Motesharrei University of Maryland May 2, 2007 String Theory!! Cosmology Outline Why? What is a Topological Defect? Examples of Cosmological Defects Brief History Importance to String Theory Geometry

More information

2.1 The metric and and coordinate transformations

2.1 The metric and and coordinate transformations 2 Cosmology and GR The first step toward a cosmological theory, following what we called the cosmological principle is to implement the assumptions of isotropy and homogeneity withing the context of general

More information

General Relativity and Differential

General Relativity and Differential Lecture Series on... General Relativity and Differential Geometry CHAD A. MIDDLETON Department of Physics Rhodes College November 1, 2005 OUTLINE Distance in 3D Euclidean Space Distance in 4D Minkowski

More information

arxiv: v1 [hep-th] 15 Jan 2014

arxiv: v1 [hep-th] 15 Jan 2014 Noninertial effects on the ground state energy of a massive scalar field in the cosmic string spacetime H. F. Mota Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH, UK. arxiv:1401.3728v1

More information

Uniformity of the Universe

Uniformity of the Universe Outline Universe is homogenous and isotropic Spacetime metrics Friedmann-Walker-Robertson metric Number of numbers needed to specify a physical quantity. Energy-momentum tensor Energy-momentum tensor of

More information

Colliding scalar pulses in the Einstein-Gauss-Bonnet gravity

Colliding scalar pulses in the Einstein-Gauss-Bonnet gravity Colliding scalar pulses in the Einstein-Gauss-Bonnet gravity Hisaaki Shinkai 1, and Takashi Torii 2, 1 Department of Information Systems, Osaka Institute of Technology, Hirakata City, Osaka 573-0196, Japan

More information

A5682: Introduction to Cosmology Course Notes. 2. General Relativity

A5682: Introduction to Cosmology Course Notes. 2. General Relativity 2. General Relativity Reading: Chapter 3 (sections 3.1 and 3.2) Special Relativity Postulates of theory: 1. There is no state of absolute rest. 2. The speed of light in vacuum is constant, independent

More information

General Relativity and Cosmology Mock exam

General Relativity and Cosmology Mock exam Physikalisches Institut Mock Exam Universität Bonn 29. June 2011 Theoretische Physik SS 2011 General Relativity and Cosmology Mock exam Priv. Doz. Dr. S. Förste Exercise 1: Overview Give short answers

More information

Geometric inequalities for black holes

Geometric inequalities for black holes Geometric inequalities for black holes Sergio Dain FaMAF-Universidad Nacional de Córdoba, CONICET, Argentina. 3 August, 2012 Einstein equations (vacuum) The spacetime is a four dimensional manifold M with

More information

New Blackhole Theorem and its Applications to Cosmology and Astrophysics

New Blackhole Theorem and its Applications to Cosmology and Astrophysics New Blackhole Theorem and its Applications to Cosmology and Astrophysics I. New Blackhole Theorem II. Structure of the Universe III. New Law of Gravity IV. PID-Cosmological Model Tian Ma, Shouhong Wang

More information

and Zoran Rakić Nonlocal modified gravity Ivan Dimitrijević, Branko Dragovich, Jelena Grujić

and Zoran Rakić Nonlocal modified gravity Ivan Dimitrijević, Branko Dragovich, Jelena Grujić Motivation Large cosmological observational findings: High orbital speeds of galaxies in clusters.( F.Zwicky, 1933) High orbital speeds of stars in spiral galaxies. ( Vera Rubin, at the end of 1960es )

More information

Geometrical models for spheroidal cosmological voids

Geometrical models for spheroidal cosmological voids Geometrical models for spheroidal cosmological voids talk by: Osvaldo M. Moreschi collaborator: Ezequiel Boero FaMAF, Universidad Nacional de Córdoba, Instituto de Física Enrique Gaviola (IFEG), CONICET,

More information

arxiv: v2 [gr-qc] 27 Apr 2013

arxiv: v2 [gr-qc] 27 Apr 2013 Free of centrifugal acceleration spacetime - Geodesics arxiv:1303.7376v2 [gr-qc] 27 Apr 2013 Hristu Culetu Ovidius University, Dept.of Physics and Electronics, B-dul Mamaia 124, 900527 Constanta, Romania

More information

Cosmic Strings in Dilaton Gravity and in Brans-Dicke Theory

Cosmic Strings in Dilaton Gravity and in Brans-Dicke Theory Bulg. J. Phys. 32 (2005) 257 262 Cosmic Strings in Dilaton Gravity and in Brans-Dicke Theory F. Rahaman, K. Gayen and A. Ghosh Dept. of Mathematics, Jadavpur University, Kolkata-700032, India Received

More information

arxiv:gr-qc/ v1 31 Dec 2005

arxiv:gr-qc/ v1 31 Dec 2005 On the differential geometry of curves in Minkowski space arxiv:gr-qc/0601002v1 31 Dec 2005 J. B. Formiga and C. Romero Departamento de Física, Universidade Federal da Paraíba, C.Postal 5008, 58051-970

More information

arxiv: v2 [gr-qc] 1 Oct 2009

arxiv: v2 [gr-qc] 1 Oct 2009 On the cosmological effects of the Weyssenhoff spinning fluid in the Einstein-Cartan framework Guilherme de Berredo-Peixoto arxiv:0907.1701v2 [gr-qc] 1 Oct 2009 Departamento de Física, ICE, Universidade

More information

arxiv: v1 [gr-qc] 7 Mar 2016

arxiv: v1 [gr-qc] 7 Mar 2016 Quantum effects in Reissner-Nordström black hole surrounded by magnetic field: the scalar wave case H. S. Vieira,2,a) and V. B. Bezerra,b) ) Departamento de Física, Universidade Federal da Paraíba, Caixa

More information

UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences

UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences Exam for AST5/94 Cosmology II Date: Thursday, June 11th, 15 Time: 9. 13. The exam set consists of 11 pages. Appendix: Equation summary Allowed

More information

The homogeneous and isotropic universe

The homogeneous and isotropic universe 1 The homogeneous and isotropic universe Notation In this book we denote the derivative with respect to physical time by a prime, and the derivative with respect to conformal time by a dot, dx τ = physical

More information

BRANE COSMOLOGY and Randall-Sundrum model

BRANE COSMOLOGY and Randall-Sundrum model BRANE COSMOLOGY and Randall-Sundrum model M. J. Guzmán June 16, 2009 Standard Model of Cosmology CMB and large-scale structure observations provide us a high-precision estimation of the cosmological parameters:

More information

Astr 2320 Tues. May 2, 2017 Today s Topics Chapter 23: Cosmology: The Big Bang and Beyond Introduction Newtonian Cosmology Solutions to Einstein s

Astr 2320 Tues. May 2, 2017 Today s Topics Chapter 23: Cosmology: The Big Bang and Beyond Introduction Newtonian Cosmology Solutions to Einstein s Astr 0 Tues. May, 07 Today s Topics Chapter : Cosmology: The Big Bang and Beyond Introduction Newtonian Cosmology Solutions to Einstein s Field Equations The Primeval Fireball Standard Big Bang Model Chapter

More information

Dynamically generated embeddings of spacetime

Dynamically generated embeddings of spacetime arxiv:gr-qc/0503103v2 18 Oct 2005 Dynamically generated embeddings of spacetime F. Dahia 1 and C. Romero 2 1 Departamento de Física, UFCG, Campina Grande-PB, Brazil, 58109-970. 2 Departamento de Física,

More information

2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I

2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I 1 2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I 2 Special Relativity (1905) A fundamental change in viewing the physical space and time, now unified

More information

Law of Gravity and Gravitational Radiation

Law of Gravity and Gravitational Radiation Law of Gravity and Gravitational Radiation Tian Ma, Shouhong Wang Supported in part by NSF and ONR http://www.indiana.edu/ fluid Blog: https://physicalprinciples.wordpress.com I. Laws of Gravity, Dark

More information

A brain teaser: The anthropic principle! Last lecture I said Is cosmology a science given that we only have one Universe? Weak anthropic principle: "T

A brain teaser: The anthropic principle! Last lecture I said Is cosmology a science given that we only have one Universe? Weak anthropic principle: T Observational cosmology: The Friedman equations 1 Filipe B. Abdalla Kathleen Lonsdale Building G.22 http://zuserver2.star.ucl.ac.uk/~hiranya/phas3136/phas3136 A brain teaser: The anthropic principle! Last

More information

The volume growth of complete gradient shrinking Ricci solitons

The volume growth of complete gradient shrinking Ricci solitons arxiv:0904.0798v [math.dg] Apr 009 The volume growth of complete gradient shrinking Ricci solitons Ovidiu Munteanu Abstract We prove that any gradient shrinking Ricci soliton has at most Euclidean volume

More information

Lecture 8: Curved Spaces

Lecture 8: Curved Spaces EPGY Summer Institute Special and General Relativity 2012 Lecture 8: Curved Spaces With the necessity of curved geodesics within regions with significant energy or mass concentrations we need to understand

More information

General Relativity (225A) Fall 2013 Assignment 8 Solutions

General Relativity (225A) Fall 2013 Assignment 8 Solutions University of California at San Diego Department of Physics Prof. John McGreevy General Relativity (5A) Fall 013 Assignment 8 Solutions Posted November 13, 013 Due Monday, December, 013 In the first two

More information

Bianchi Type-VI Bulk Viscous Fluid String Cosmological Model in General Relativity

Bianchi Type-VI Bulk Viscous Fluid String Cosmological Model in General Relativity Bulg. J. Phys. 38 2011 14 14 Bianchi Type-VI Bulk Viscous Fluid String Cosmological Model in General Relativity S.P. Kandalkar 1, P.P. Khade 2, S.P. Gawande 1 1 Department of Mathematics, Government Vidarbha

More information

Hydrogen atom in the gravitational fields of topological defects. Abstract

Hydrogen atom in the gravitational fields of topological defects. Abstract Hydrogen atom in the gravitational fields of topological defects Geusa de A. Marques and Valdir B. Bezerra. Departamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58059-970, João Pessoa,

More information

Is there a magnification paradox in gravitational lensing?

Is there a magnification paradox in gravitational lensing? Is there a magnification paradox in gravitational lensing? Olaf Wucknitz wucknitz@astro.uni-bonn.de Astrophysics seminar/colloquium, Potsdam, 26 November 2007 Is there a magnification paradox in gravitational

More information

International Journal of Applied and Universal Research ISSN No: Volume III, Issue II, Mar-Apr Available online at:

International Journal of Applied and Universal Research ISSN No: Volume III, Issue II, Mar-Apr Available online at: BIANCHI TYPE III ELECTRO MAGNETIZED COSMOLOGICAL MODEL WITH NAMBU STRINGS IN GENERAL THEORY OF RELATIVITY R.K.Dubey 1, Anil Saini 2, Neelam Yadav 3 1 Department of Mathematics, Govt. SKN PG College Mauganj

More information

Bachelor Thesis. General Relativity: An alternative derivation of the Kruskal-Schwarzschild solution

Bachelor Thesis. General Relativity: An alternative derivation of the Kruskal-Schwarzschild solution Bachelor Thesis General Relativity: An alternative derivation of the Kruskal-Schwarzschild solution Author: Samo Jordan Supervisor: Prof. Markus Heusler Institute of Theoretical Physics, University of

More information

Cosmology. April 13, 2015

Cosmology. April 13, 2015 Cosmology April 3, 205 The cosmological principle Cosmology is based on the principle that on large scales, space (not spacetime) is homogeneous and isotropic that there is no preferred location or direction

More information

Kerr black hole and rotating wormhole

Kerr black hole and rotating wormhole Kerr Fest (Christchurch, August 26-28, 2004) Kerr black hole and rotating wormhole Sung-Won Kim(Ewha Womans Univ.) August 27, 2004 INTRODUCTION STATIC WORMHOLE ROTATING WORMHOLE KERR METRIC SUMMARY AND

More information

Geometrical Behaviuors of LRS Bianchi Type-I Cosmological Model

Geometrical Behaviuors of LRS Bianchi Type-I Cosmological Model EJTP 6, No. 22 (2009) 79 84 Electronic Journal of Theoretical Physics Geometrical Behaviuors of LRS Bianchi Type-I Cosmological Model Hassan Amirhashchi 1, Hishamuddin Zainuddin 2 and Hamid Nil Saz Dezfouli

More information

From An Apple To Black Holes Gravity in General Relativity

From An Apple To Black Holes Gravity in General Relativity From An Apple To Black Holes Gravity in General Relativity Gravity as Geometry Central Idea of General Relativity Gravitational field vs magnetic field Uniqueness of trajectory in space and time Uniqueness

More information

مقاله نامه بیست و دومین کنفرانس بهاره فیزیک )30-31 اردیبهشت ) Acoustic vortex in media with screw dislocation using Katanaev-Volovich approach

مقاله نامه بیست و دومین کنفرانس بهاره فیزیک )30-31 اردیبهشت ) Acoustic vortex in media with screw dislocation using Katanaev-Volovich approach Acoustic vortex in media with screw dislocation using Katanaev-Volovich approach Reza Torabi Department of Physics, Tafresh University, P.O.Box: 39518-79611, Tafresh, Iran Abstract We study acoustic vortex

More information

Notes on General Relativity Linearized Gravity and Gravitational waves

Notes on General Relativity Linearized Gravity and Gravitational waves Notes on General Relativity Linearized Gravity and Gravitational waves August Geelmuyden Universitetet i Oslo I. Perturbation theory Solving the Einstein equation for the spacetime metric is tremendously

More information

On Isotropic Coordinates and Einstein s Gravitational Field

On Isotropic Coordinates and Einstein s Gravitational Field July 006 PROGRESS IN PHYSICS Volume 3 On Isotropic Coordinates and Einstein s Gravitational Field Stephen J. Crothers Queensland Australia E-mail: thenarmis@yahoo.com It is proved herein that the metric

More information

Cosmic Strings and Closed time-like curves in teleparallel gravity

Cosmic Strings and Closed time-like curves in teleparallel gravity Cosmic Strings and Closed time-like curves in teleparallel gravity arxiv:gr-qc/0102094v1 22 Feb 2001 L.C. Garcia de Andrade 1 Abstract Closed Time-like curves (CTC) in Cosmic strings in teleparallel T

More information

Einstein Double Field Equations

Einstein Double Field Equations Einstein Double Field Equations Stephen Angus Ewha Woman s University based on arxiv:1804.00964 in collaboration with Kyoungho Cho and Jeong-Hyuck Park (Sogang Univ.) KIAS Workshop on Fields, Strings and

More information

Übungen zu RT2 SS (4) Show that (any) contraction of a (p, q) - tensor results in a (p 1, q 1) - tensor.

Übungen zu RT2 SS (4) Show that (any) contraction of a (p, q) - tensor results in a (p 1, q 1) - tensor. Übungen zu RT2 SS 2010 (1) Show that the tensor field g µν (x) = η µν is invariant under Poincaré transformations, i.e. x µ x µ = L µ νx ν + c µ, where L µ ν is a constant matrix subject to L µ ρl ν ση

More information

The Schwarzschild Metric

The Schwarzschild Metric The Schwarzschild Metric The Schwarzschild metric describes the distortion of spacetime in a vacuum around a spherically symmetric massive body with both zero angular momentum and electric charge. It is

More information

5 Topological defects and textures in ordered media

5 Topological defects and textures in ordered media 5 Topological defects and textures in ordered media In this chapter we consider how to classify topological defects and textures in ordered media. We give here only a very short account of the method following

More information

2 General Relativity. 2.1 Curved 2D and 3D space

2 General Relativity. 2.1 Curved 2D and 3D space 22 2 General Relativity The general theory of relativity (Einstein 1915) is the theory of gravity. General relativity ( Einstein s theory ) replaced the previous theory of gravity, Newton s theory. The

More information

UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences

UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences Exam for AST5220 Cosmology II Date: Tuesday, June 4th, 2013 Time: 09.00 13.00 The exam set consists of 13 pages. Appendix: Equation summary

More information

Black Hole Universe with Rotation Chan Park KAIST

Black Hole Universe with Rotation Chan Park KAIST Black Hole Universe with Rotation 2016.01.02. Chan Park KAIST Motivation FLRW cosmology Highly symmetric assumption : spatial homogeneity and isotropy Metric ds 2 = dt 2 + a 2 t a t : scale factor Friedmann

More information

An introduction to General Relativity and the positive mass theorem

An introduction to General Relativity and the positive mass theorem An introduction to General Relativity and the positive mass theorem National Center for Theoretical Sciences, Mathematics Division March 2 nd, 2007 Wen-ling Huang Department of Mathematics University of

More information

General Relativity I

General Relativity I General Relativity I presented by John T. Whelan The University of Texas at Brownsville whelan@phys.utb.edu LIGO Livingston SURF Lecture 2002 July 5 General Relativity Lectures I. Today (JTW): Special

More information

Time-Periodic Solutions of the Einstein s Field Equations II: Geometric Singularities

Time-Periodic Solutions of the Einstein s Field Equations II: Geometric Singularities Science in China Series A: Mathematics 2009 Vol. 52 No. 11 1 16 www.scichina.com www.springerlink.com Time-Periodic Solutions of the Einstein s Field Equations II: Geometric Singularities KONG DeXing 1,

More information

Write your CANDIDATE NUMBER clearly on each of the THREE answer books provided. Hand in THREE answer books even if they have not all been used.

Write your CANDIDATE NUMBER clearly on each of the THREE answer books provided. Hand in THREE answer books even if they have not all been used. UNIVERSITY OF LONDON BSc/MSci EXAMINATION May 2007 for Internal Students of Imperial College of Science, Technology and Medicine This paper is also taken for the relevant Examination for the Associateship

More information

General Relativity and Cosmology. The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang

General Relativity and Cosmology. The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang The End of Absolute Space (AS) Special Relativity (SR) abolished AS only for the special

More information

Non-static local string in Brans Dicke theory

Non-static local string in Brans Dicke theory PRAMANA cfl Indian Academy of Sciences Vol. 55, No. 3 journal of September 2 physics pp. 369 374 Non-static local string in Brans Dicke theory AASEN Λ Relativity and Cosmology Research Centre, Department

More information

Properties of Traversable Wormholes in Spacetime

Properties of Traversable Wormholes in Spacetime Properties of Traversable Wormholes in Spacetime Vincent Hui Department of Physics, The College of Wooster, Wooster, Ohio 44691, USA. (Dated: May 16, 2018) In this project, the Morris-Thorne metric of

More information

Some Quantum Aspects of D=3 Space-Time Massive Gravity.

Some Quantum Aspects of D=3 Space-Time Massive Gravity. Some Quantum Aspects of D=3 Space-Time Massive Gravity. arxiv:gr-qc/96049v 0 Nov 996 Carlos Pinheiro, Universidade Federal do Espírito Santo, Departamento de Física, Vitória-ES, Brazil, Gentil O. Pires,

More information

The magnification theorem

The magnification theorem The magnification theorem Olaf Wucknitz wucknitz@astro.uni-bonn.de Three decades of gravitational lenses, JENAM, 21 April 2009 2.5 decades of the magnification theorem General theorems in lensing odd image

More information

The Aharonov-Bohm effect around a rotating black hole analogue

The Aharonov-Bohm effect around a rotating black hole analogue The Aharonov-Bohm effect around a rotating black hole analogue Cássio I. S. Marinho Supervisor: Prof. Dr. Ednilton S. de Oliveira Universidade Federal do Pará IV AWBHAMG, May 11 th, 2015. Outline 1 Introduction

More information

8.821/8.871 Holographic duality

8.821/8.871 Holographic duality Lecture 3 8.81/8.871 Holographic duality Fall 014 8.81/8.871 Holographic duality MIT OpenCourseWare Lecture Notes Hong Liu, Fall 014 Lecture 3 Rindler spacetime and causal structure To understand the spacetime

More information

New cosmological solutions in Nonlocal Modified Gravity. Jelena Stanković

New cosmological solutions in Nonlocal Modified Gravity. Jelena Stanković Motivation Large observational findings: High orbital speeds of galaxies in clusters. (F.Zwicky, 1933) High orbital speeds of stars in spiral galaxies. (Vera Rubin, at the end of 1960es) Big Bang Accelerated

More information

General Relativity ASTR 2110 Sarazin. Einstein s Equation

General Relativity ASTR 2110 Sarazin. Einstein s Equation General Relativity ASTR 2110 Sarazin Einstein s Equation Curvature of Spacetime 1. Principle of Equvalence: gravity acceleration locally 2. Acceleration curved path in spacetime In gravitational field,

More information

Are spacetime horizons higher dimensional sources of energy fields? (The black hole case).

Are spacetime horizons higher dimensional sources of energy fields? (The black hole case). Are spacetime horizons higher dimensional sources of energy fields? (The black hole case). Manasse R. Mbonye Michigan Center for Theoretical Physics Physics Department, University of Michigan, Ann Arbor,

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

Analogue non-riemannian black holes in vortical moving plasmas

Analogue non-riemannian black holes in vortical moving plasmas Analogue non-riemannian black holes in vortical moving plasmas arxiv:gr-qc/0509034v1 11 Sep 2005 L.C. Garcia de Andrade 1 Abstract Analogue black holes in non-riemannian effective spacetime of moving vortical

More information

Singularity formation in black hole interiors

Singularity formation in black hole interiors Singularity formation in black hole interiors Grigorios Fournodavlos DPMMS, University of Cambridge Heraklion, Crete, 16 May 2018 Outline The Einstein equations Examples Initial value problem Large time

More information

A practical look at Regge calculus

A practical look at Regge calculus A practical look at Regge calculus Dimitri Marinelli Physics Department - Università degli Studi di Pavia and I.N.F.N. - Pavia in collaboration with Prof. G. Immirzi Karl Schwarzschild Meeting 2013, Frankfurt

More information

Fifth force from fifth dimension: a comparison between two. different approaches

Fifth force from fifth dimension: a comparison between two. different approaches Fifth force from fifth dimension: a comparison between two different approaches F. Dahia a,e.m.monte b and C. Romero b a Departamento de Física, Universidade Federal de Campina Grande, 58109-970, Campina

More information

Classical and Quantum Bianchi type I cosmology in K-essence theory

Classical and Quantum Bianchi type I cosmology in K-essence theory Classical and Quantum Bianchi type I cosmology in K-essence theory Luis O. Pimentel 1, J. Socorro 1,2, Abraham Espinoza-García 2 1 Departamento de Fisica de la Universidad Autonoma Metropolitana Iztapalapa,

More information

Dynamical Domain Wall and Localization

Dynamical Domain Wall and Localization Dynamical Domain Wall and Localization Shin ichi Nojiri Department of Physics & Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI), Nagoya Univ. Typeset by FoilTEX 1 Based on

More information

Cosmology & CMB. Set2: Linear Perturbation Theory. Davide Maino

Cosmology & CMB. Set2: Linear Perturbation Theory. Davide Maino Cosmology & CMB Set2: Linear Perturbation Theory Davide Maino Covariant Perturbation Theory Covariant = takes same form in all coordinate systems Invariant = takes the same value in all coordinate systems

More information

A GENERALLY COVARIANT FIELD EQUATION FOR GRAVITATION AND ELECTROMAGNETISM. Institute for Advanced Study Alpha Foundation

A GENERALLY COVARIANT FIELD EQUATION FOR GRAVITATION AND ELECTROMAGNETISM. Institute for Advanced Study Alpha Foundation A GENERALLY COVARIANT FIELD EQUATION FOR GRAVITATION AND ELECTROMAGNETISM Myron W. Evans Institute for Advanced Study Alpha Foundation E-mail: emyrone@aol.com Received 17 April 2003; revised 1 May 2003

More information

arxiv: v1 [gr-qc] 19 Jun 2009

arxiv: v1 [gr-qc] 19 Jun 2009 SURFACE DENSITIES IN GENERAL RELATIVITY arxiv:0906.3690v1 [gr-qc] 19 Jun 2009 L. FERNÁNDEZ-JAMBRINA and F. J. CHINEA Departamento de Física Teórica II, Facultad de Ciencias Físicas Ciudad Universitaria,

More information

Astro 596/496 PC Lecture 9 Feb. 8, 2010

Astro 596/496 PC Lecture 9 Feb. 8, 2010 Astro 596/496 PC Lecture 9 Feb. 8, 2010 Announcements: PF2 due next Friday noon High-Energy Seminar right after class, Loomis 464: Dan Bauer (Fermilab) Recent Results from the Cryogenic Dark Matter Search

More information

Brane-World Black Holes

Brane-World Black Holes Brane-World Black Holes A. Chamblin, S.W. Hawking and H.S. Reall DAMTP University of Cambridge Silver Street, Cambridge CB3 9EW, United Kingdom. Preprint DAMTP-1999-133 arxiv:hep-th/990905v 1 Oct 1999

More information

Problem 1, Lorentz transformations of electric and magnetic

Problem 1, Lorentz transformations of electric and magnetic Problem 1, Lorentz transformations of electric and magnetic fields We have that where, F µν = F µ ν = L µ µ Lν ν F µν, 0 B 3 B 2 ie 1 B 3 0 B 1 ie 2 B 2 B 1 0 ie 3 ie 2 ie 2 ie 3 0. Note that we use the

More information

Static Hydrodynamic Equation in 4d BSBM Theory

Static Hydrodynamic Equation in 4d BSBM Theory Advanced Studies in Theoretical Physics Vol. 8, 2014, no. 23, 1015-1020 HIKARI Ltd, www.m-hikari.com http://dx.doi.org/10.12988/astp.2014.49120 Static Hydrodynamic Equation in 4d BSBM Theory Azrul S. K.

More information

Compact Stars in the Braneworld

Compact Stars in the Braneworld Compact Stars in the Braneworld Mike Georg Bernhardt Zentrum für Astronomie Heidelberg Landessternwarte 28 January 29 Outline Review: Relativistic Stars TOV equations Solutions of the TOV equations Neutron

More information

Lecture 1 General relativity and cosmology. Kerson Huang MIT & IAS, NTU

Lecture 1 General relativity and cosmology. Kerson Huang MIT & IAS, NTU A Superfluid Universe Lecture 1 General relativity and cosmology Kerson Huang MIT & IAS, NTU Lecture 1. General relativity and cosmology Mathematics and physics Big bang Dark energy Dark matter Robertson-Walker

More information

Non Linear Dynamics in Einstein-Friedman Equations

Non Linear Dynamics in Einstein-Friedman Equations Non Linear Dynamics in Einstein-Friedman Equations Usman Naseer 2012-10-0054 May 15, 2011 Abstract Einstein-Friedman equations for the dynamics of a spatially homogenous and isotropic universe are rederived

More information

The Aharonov-Bohm Effect: Mathematical Aspects of the Quantum Flow

The Aharonov-Bohm Effect: Mathematical Aspects of the Quantum Flow Applied athematical Sciences, Vol. 1, 2007, no. 8, 383-394 The Aharonov-Bohm Effect: athematical Aspects of the Quantum Flow Luis Fernando ello Instituto de Ciências Exatas, Universidade Federal de Itajubá

More information

Gravitational Waves. Basic theory and applications for core-collapse supernovae. Moritz Greif. 1. Nov Stockholm University 1 / 21

Gravitational Waves. Basic theory and applications for core-collapse supernovae. Moritz Greif. 1. Nov Stockholm University 1 / 21 Gravitational Waves Basic theory and applications for core-collapse supernovae Moritz Greif Stockholm University 1. Nov 2012 1 / 21 General Relativity Outline 1 General Relativity Basic GR Gravitational

More information

A Brief Introduction to Mathematical Relativity

A Brief Introduction to Mathematical Relativity A Brief Introduction to Mathematical Relativity Arick Shao Imperial College London Arick Shao (Imperial College London) Mathematical Relativity 1 / 31 Special Relativity Postulates and Definitions Einstein

More information

PHYM432 Relativity and Cosmology 17. Cosmology Robertson Walker Metric

PHYM432 Relativity and Cosmology 17. Cosmology Robertson Walker Metric PHYM432 Relativity and Cosmology 17. Cosmology Robertson Walker Metric Cosmology applies physics to the universe as a whole, describing it s origin, nature evolution and ultimate fate. While these questions

More information

Theoretical Aspects of Black Hole Physics

Theoretical Aspects of Black Hole Physics Les Chercheurs Luxembourgeois à l Etranger, Luxembourg-Ville, October 24, 2011 Hawking & Ellis Theoretical Aspects of Black Hole Physics Glenn Barnich Physique théorique et mathématique Université Libre

More information

Kerr-Schild Method and Geodesic Structure in Codimension-2 BBH

Kerr-Schild Method and Geodesic Structure in Codimension-2 BBH 1 Kerr-Schild Method and Geodesic Structure in Codimension-2 Brane Black Holes B. Cuadros-Melgar Departamento de Ciencias Físicas, Universidad Nacional Andrés Bello, Santiago, Chile Abstract We consider

More information

PROBLEM SET 10 (The Last!)

PROBLEM SET 10 (The Last!) MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.286: The Early Universe December 8, 2016 Prof. Alan Guth PROBLEM SET 10 (The Last!) DUE DATE: Wednesday, December 14, 2016, at 4:00 pm.

More information

A Generally Covariant Field Equation For Gravitation And Electromagnetism

A Generally Covariant Field Equation For Gravitation And Electromagnetism 3 A Generally Covariant Field Equation For Gravitation And Electromagnetism Summary. A generally covariant field equation is developed for gravitation and electromagnetism by considering the metric vector

More information

Third Year: General Relativity and Cosmology. 1 Problem Sheet 1 - Newtonian Gravity and the Equivalence Principle

Third Year: General Relativity and Cosmology. 1 Problem Sheet 1 - Newtonian Gravity and the Equivalence Principle Third Year: General Relativity and Cosmology 2011/2012 Problem Sheets (Version 2) Prof. Pedro Ferreira: p.ferreira1@physics.ox.ac.uk 1 Problem Sheet 1 - Newtonian Gravity and the Equivalence Principle

More information

FRW cosmology: an application of Einstein s equations to universe. 1. The metric of a FRW cosmology is given by (without proof)

FRW cosmology: an application of Einstein s equations to universe. 1. The metric of a FRW cosmology is given by (without proof) FRW cosmology: an application of Einstein s equations to universe 1. The metric of a FRW cosmology is given by (without proof) [ ] dr = d(ct) R(t) 1 kr + r (dθ + sin θdφ ),. For generalized coordinates

More information

A873: Cosmology Course Notes. II. General Relativity

A873: Cosmology Course Notes. II. General Relativity II. General Relativity Suggested Readings on this Section (All Optional) For a quick mathematical introduction to GR, try Chapter 1 of Peacock. For a brilliant historical treatment of relativity (special

More information

Chapter 7 Curved Spacetime and General Covariance

Chapter 7 Curved Spacetime and General Covariance Chapter 7 Curved Spacetime and General Covariance In this chapter we generalize the discussion of preceding chapters to extend covariance to more general curved spacetimes. 145 146 CHAPTER 7. CURVED SPACETIME

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

Escape velocity and Schwarzschild s Solution for Black Holes

Escape velocity and Schwarzschild s Solution for Black Holes Escape velocity and Schwarzschild s Solution for Black Holes Amir Ali Tavajoh 1 1 Amir_ali3640@yahoo.com Introduction Scape velocity for every star or planet is different. As a star starts to collapse

More information

Anisotropic Interior Solutions in Hořava Gravity and Einstein-Æther Theory

Anisotropic Interior Solutions in Hořava Gravity and Einstein-Æther Theory Anisotropic Interior Solutions in and Einstein-Æther Theory CENTRA, Instituto Superior Técnico based on DV and S. Carloni, arxiv:1706.06608 [gr-qc] Gravity and Cosmology 2018 Yukawa Institute for Theoretical

More information

A rotating charged black hole solution in f (R) gravity

A rotating charged black hole solution in f (R) gravity PRAMANA c Indian Academy of Sciences Vol. 78, No. 5 journal of May 01 physics pp. 697 703 A rotating charged black hole solution in f R) gravity ALEXIS LARRAÑAGA National Astronomical Observatory, National

More information

Some Results about the Classification of Totally Real Minimal Surfaces in S 5

Some Results about the Classification of Totally Real Minimal Surfaces in S 5 Int. J. Contemp. Math. Sciences, Vol. 2, 2007, no. 24, 1175-1181 Some Results about the Classification of Totally Real Minimal Surfaces in S 5 Rodrigo Ristow Montes Departamento de Matemática Universidade

More information

The Geometry of Relativity

The Geometry of Relativity The Geometry of Relativity Tevian Dray Department of Mathematics Oregon State University http://www.math.oregonstate.edu/~tevian OSU 4/27/15 Tevian Dray The Geometry of Relativity 1/27 Books The Geometry

More information