CHAOS 5541 No. of Pages 5 ARTICLE IN PRESS UNCORRECTED PROOF

Size: px
Start display at page:

Download "CHAOS 5541 No. of Pages 5 ARTICLE IN PRESS UNCORRECTED PROOF"

Transcription

1 1 Chaos, Solitons and Fractals xxx (2007) xxx xxx 2 Hierarchical Cantor set in the large scale structure 3 with torus geometry 4 R. Murdzek 5 Physics Department, Al. I. Cuza University, Blvd. Carol I, Nr. 11, Iassy , Romania 6 Accepted 2 January Abstract 9 The formation of large scale structures is considered within a model with string on toroidal space-time. Firstly, the 10 space-time geometry is presented. In this geometry, the Universe is represented by a string describing a torus surface. 11 Thereafter, the large scale structure of the Universe is derived from the string oscillations. The results are in agreement 12 with the cellular structure of the large scale distribution and with the theory of a Cantorian space-time. 13 Ó 2007 Elsevier Ltd. All rights reserved Introduction 16 The recently completed galaxy surveys as such the Two Degree Field Galaxy Redshift Survey [1] have shown that, at 17 the largest scales, the distribution of galaxies exhibits structures that are not satisfactorily explained within the frame- 18 work of the standard cosmological model. The properties of the large scale structure are well characterized using the 19 fractal geometry language. Following this idea, it has been shown that the fractal dimension of the large scale galaxy 20 distribution is close to two and that there are no evidences for transition to homogeneity. A basic assumption of the 21 standard cosmological model is that, on some large enough scales, the universe presents a homogeneous distribution 22 of matter. But the last three decades proved that the observational data are consistent with Charlier s conception of 23 a hierarchical universe [2] and in agreement with El Naschie s E-infinity theory [3] rather than with the standard model 24 description. 25 In this respect, De Vaucouleurs [4] showed that, within wide limits, the available data satisfied a mass distribution 26 law MðrÞ /r 1;3. Since then, the issue has continued to take importance with the growth of the data. In 1995, Baryshev 27 et al. [5], showed that the scale of the largest inhomogeneities is given by the sizes of the sample s boundaries. In the last 28 two decades, several redshift surveys, such as those performed by Giovanelli and Haynes [6], De Lapparent et al. [7], 29 Broadhurst et al. [8], Da Costa et al. [9] and Vettolani et al. [10] have been emphasized massive structures such as sheets, 30 filaments, clusters and voids, and have shown that large structures are common features of the observable universe. The 31 pencil beam survey data gathered in ESO Slice Project has been analyzed by Pietronero and Sylos Labini [11]. Within 32 their work it has been shown that the distribution of galaxies confirms the law MðrÞ /r 2. The same result of fractal 33 distribution of dimension (D ¼ 2 0:2) has been found in the analysis performed by Guzzo et al. [12] and Moore address: rmurdzek@yahoo.com /$ - see front matter Ó 2007 Elsevier Ltd. All rights reserved. doi: /j.chaos

2 2 R. Murdzek / Chaos, Solitons and Fractals xxx (2007) xxx xxx 34 et al. [13]. Recently, it has been shown that this distribution looks more like a cellular structure among all scales rather 35 than a distribution which presents a cut-off to homogeneity [14]. 36 But such hierarchical structures are found in the Cantorian space-time. The Cantorian space-time [15] contains an 37 infinite number of sets E(i), where the index i means the topological dimension of the smooth space into which the 38 fractal set is contained. A representative example is the Cantor set, Eð0Þ, a fractal which is contained into a space of 39 topological dimension one, but whose Hausdorff dimension is equal to Similarly, the fractal dimension of the dis- 40 tribution of galaxies inside the smoothed space-time of integer dimension differs from the topological dimension of the 41 space into which is being contained. 42 Another problem of the standard cosmological model is the well-known singularity problem. One way to avoid it 43 but to keep the positive results of the expanding models is to consider a cyclic universe, without singularities, as it is 44 described within the ekpyrotic model [16]. 45 In this work, we shall show that the fractal structure of the large scale distribution of matter can be derived from a 46 brane-world scenario with toroidal space-time: in Section 2, we shall briefly discuss the geometry of the background 47 space-time. We also shall show that such a space-time supports the formation of standing waves. Then, our three- 48 dimensional space is represented by an oscillating closed string embedded into a higher dimensional space. In Section 49 3, we shall make the connection between the structure of the oscillating loop and the Cantor set. Some conclusions are 50 also discussed A string on a torus 52 In what follows we shall consider that: 53 By averaging, the Universe can be described as a smooth four-dimensional brane, embedded into an N-dimensional 54 space, as it is described in brane-world scenarios [16,17]. 55 The four-dimensional space-time is globally flat, isotropic and homogeneous, in respect with the Cosmological 56 Principle. 57 The Universe exhibits a cyclic behavior by following a succession of expanding and contracting stages. This state- 58 ment implies that our space-time is closed. 59 The formation of cosmic structures reflects the behavior of the space-time. 60 As the large scale distribution of galaxies proves, the fact that the Universe looks three-dimensional is due to the 61 smoothing (averaging) of the included structures In order to visualize such a space-time we shall consider the geometry of a torus. In this model our three-dimensional 64 space is represented as the great circle of the torus which evolves on torus surface. It means that from this point of view 65 the three-dimensional space is represented as a closed loop moving on the torus. 66 Toroidal geometry is presented in the literature through the work of Arfken, Moon and Spencer, Morse and Fesh- 67 bach [18]. 68 Using the notations from Fig. 1, we have for the torus surface the Riemannian metric [19] Fig. 1. Notations used for the torus parameters and coordinates.

3 R. Murdzek / Chaos, Solitons and Fractals xxx (2007) xxx xxx 3 70 ds 2 ¼ ðbþacos mþ 2 d/ 2 þ a 2 dm 2 : 71 After a short session in Maple, from this line element we obtain the connections coefficients. Then, we have C 1 12 ¼ a sin m ðb þ a cos mþ 73 C 2 ðb þ a cos mþ sin m 11 ¼ a 74 The geodesic equations are then derived and d 2 dt 2 /ðtþ d 2 dt mðtþ 2 2a sinðmþ d /ðtþ d mðtþ dt dt ¼ 0 b þ a cosðmþ ðb þ a cosðmþþ sinðmþ d /ðtþ 2 dt ¼ 0: a 82 Eqs. (3) and (4) as well as the visualization of the geodesics (Fig. 2) show that on the toroidal space-time the null- 83 geodesics are closed curves, which means that the formation of standing waves is allowed on the torus surface String oscillations and fractal space-time 85 In our model, the space-time is represented by the closed loop which describes the torus surface. We aim to have a 86 description of the string oscillations which ignores the details of the wiggles. Then, the most simple solution is 88 sðx; tþ ¼A sinðk n xþ cosðx n tþ; where x ¼ðbþacos mþu: ð5þ 89 Perturbations will appear because of the oscillations, in the effective density of the string. We compute the amplitude 90 of these perturbations as functions of x, starting from the energy distribution along the string. 91 If we require a length L of string to form a closed loop, from the periodicity condition it follows that 93 sðx; tþ ¼sðx þ L=2; tþ: ð6þ 94 We can compute the energy distribution of the oscillations along the string by averaging over a period and summing 95 over all oscillations modes. Then, we have V ðxþ ¼ A02 X 1 1 nxp L n 2 sin2 ; 97 L ð7þ n¼0 98 where A 0 ¼ const, and n an odd integer. 99 Let T 0 be the tension in the string in the absence of oscillations. Then, the effective tension along the string is then given through 103 ov ðxþ T eff ¼ T 0 : ð8þ ox 104 We must note here that the product of the effective density l eff and effective tension remains constant along the string 105 [20] ð1þ ð2þ ð3þ ð4þ Fig. 2. Geodesic on the torus surface: the torus is geodesically complete.

4 4 R. Murdzek / Chaos, Solitons and Fractals xxx (2007) xxx xxx T eff l eff ¼ l 2 ; 109 where l ¼ const. 110 From Eqs. (8) and (9), we have 112 l eff ðxþ ¼l 2 1 T 0 ov ðxþ ox Fig. 4. Cantor set D cantor ¼ 0:6309 (a) and Cantor cube D c ¼ 1:893 (b). : ð10þ 113 Fig. 3 illustrates the effective density of the string as a function of the position x on the string. The picture is that of a 114 cellular universe where clusters form by accumulating the matter in the regions of maximum densities on the string. 115 These regions correspond to the nodes which are formed by the standing waves. Because of the fact that every harmonic 116 participates in the distribution of the energy on the string, we will have different scales of clustering which correspond to 117 different energies. The distribution of the nodes on the string is perfectly analogous to Cantor set, meaning that the 118 fractal dimension of this distribution is equal to fractal dimension of the Cantor set which is D cantor ¼ 0:6309. The frac- 119 tal dimension of the distribution in the three-dimensional space will be that of a Cantor cube (Fig. 4), D c ¼ 1:893. This 120 result is concordant with the fractal dimension of the galaxy distribution. ð9þ Concluding remarks 122 Using the torus geometry, we have obtained a new representation of the Universe, in which the stationary waves on 123 the torus surface determine the appearance of the structures. These structures perfectly correspond to the Cantorian

5 R. Murdzek / Chaos, Solitons and Fractals xxx (2007) xxx xxx space-time. The fractal dimension given by the distribution of the nodes on the string and is in good concordance to the 125 fractal dimension of the galaxy distribution. 126 References 127 [1] also at: astro-ph/ [2] Charlier CVL. Wei Eine Unendliche Welt Aufgebaut Sein Kann. Astronomioch Fysik 1908;4:1; 129 Charlier CVL. How an infinite world may be built up. Arkiv Mat Astron Physik 1922;16:1 35; 130 Charlier CVL. Publ Astron Soc Pacific 1924;37: [3] El Naschie MS. A review of E infinity theory and the mass spectrum of high energy particle physics. Chaos Soliton Fract ;19: [4] De Vaucouleurs G. The case for a hierarchical cosmology. Science 1970;167: [5] Baryshev YuV, Sylos Labini F, Montuori M, Pietronero L. Facts and ideas in modern cosmology. Vistas Astron 1995;38: [6] Giovanelli R, Haynes MP. A 21 cm survey of the Pisces Perseus supercluster. 1: the declination zone to 33.5 degrees. Astron 136 J 1985;90: ; 137 Giovanelli R, Haynes MP, Chincarini GL. Morphological segregation in the Pisces Perseus supercluster. Astrophys J ;300: [7] De Lapparent V, Geller MJ, Huchra JP. The mean density and the two-point correlation function for the CfA1 redshift survey 140 slices. Astrophys J 1988;332: [8] Broadhurst TJ, Ellis RS, Koo DC, Szalay AS. Large scale distribution of galaxies at the galactic poles. Nature 1990;343: [9] Da Costa MJ et al. A complete southern sky redshift survey. Astrophys J 1994;424:L [10] Vettolani G, et al. Preliminary results from the ESO Slice Project (ESP). Proc of Schloss Rindberg Workshop: Studying the 144 Universe with Cluster of Galaxies. 145 [11] Pietronero L, Sylos Labini F. Comments on the CfA2 analysis, preprint; [12] Guzzo L, Iovino A, Chincarini G, Giovanelli R, Haynes MP. Scale invariant clustering in the large scale distribution of galaxies. 147 Astrophys J Lett 1992;382:L [13] Moore B, Frenk CS, Efstathiou G, Saunders W. The clustering of IRAS galaxies. Mon Not R Astron Soc 1994;269: [14] Einasto J. The structure of the universe on 100 Mpc scales preprint: arxiv.org/abs/astro-ph/ [15] El Naschie MS. Elementary prerequisites for E-infinity theory. Chaos Soliton Fract 2006;30: ; 151 El Naschie MS. Intermediate prerequisites for E-infinity theory. Chaos Soliton Fract 2006;30:622 8; 152 El Naschie MS. Advanced prerequisites for E-infinity theory. Chaos Soliton Fract 2006;30: [16] Khoury J, Ovrut BA, Steinhardt PJ, Turok N. Phys Rev D 2001;64; 154 Steinhardt Paul J, Turok Neil Available from: hep-th/ [17] Randall L, Sundrum R. Phys Rev Lett 1999;83:3370. Available from: hep-th/ [18] Arfken G. In: Mathematical method for physicists. Orlando, FL: Academic Press; p ; 157 Moon P, Spencer DE. Field theory handbook, including coordinate systems, differential equations, and their solutions. New York: 158 Springer-Verlag; p ; 159 Morse PM, Feshbach H. Methods of theoretical physics, part I. New York: McGraw-Hill; p [19] Murdzek R. The torus universe. Romanian J Phys 2006;51(9 10); 161 Murdzek R. The geometry of the torus universe. Int J Mod Phys 2007;16(3): [20] Vilenkin A. Phys. Rev. D 1990;41:

THE GEOMETRY OF THE TORUS UNIVERSE

THE GEOMETRY OF THE TORUS UNIVERSE International Journal of Modern Physics D Vol. 16, No. 4 (2007) 681 686 c World Scientific Publishing Company THE GEOMETRY OF THE TORUS UNIVERSE R. MURDZEK Physics Department, Al. I. Cuza University, Iassy,

More information

THE SELF-ORGANIZING UNIVERSE

THE SELF-ORGANIZING UNIVERSE ASTROPHYSICS THE SELF-ORGANIZING UNIVERSE R. MURDZEK 1, O. IFTIMIE 2 1 Physics Department, Al. I. Cuza University, Iassy rmurdzek@yahoo.com 2 Phylosophy Department, Al. I. Cuza University, Iassy Received

More information

CYCLIC UNIVERSES FROM TORUS GEOMETRY

CYCLIC UNIVERSES FROM TORUS GEOMETRY COSMOLOGY CYCLIC UNIVERSES FROM TORUS GEOMETRY R. MURDZEK Physics Department, Al. I. Cuza University rmurdzek@yahoo.com Received April 27, 2006 The models of cyclic universes emerge in a natural way from

More information

The 2D Power Spectrum of the Las Campanas Redshift Survey: Detection of Excess Power on 100 h 1 Mpc Scales. and. Douglas Tucker ABSTRACT

The 2D Power Spectrum of the Las Campanas Redshift Survey: Detection of Excess Power on 100 h 1 Mpc Scales. and. Douglas Tucker ABSTRACT The 2D Power Spectrum of the Las Campanas Redshift Survey: Detection of Excess Power on 1 h 1 Mpc Scales Stephen D. Landy and Stephen A. Shectman Carnegie Observatories, 813 Santa Barbara Street, Pasadena,

More information

9.1 Large Scale Structure: Basic Observations and Redshift Surveys

9.1 Large Scale Structure: Basic Observations and Redshift Surveys 9.1 Large Scale Structure: Basic Observations and Redshift Surveys Large-Scale Structure Density fluctuations evolve into structures we observe: galaxies, clusters, etc. On scales > galaxies, we talk about

More information

Modelling the SPARC galaxies using a neo-mond formalism, and the subsequent derivation of a complete theory of the baryonic Tully-Fisher relation.

Modelling the SPARC galaxies using a neo-mond formalism, and the subsequent derivation of a complete theory of the baryonic Tully-Fisher relation. Modelling the SPARC galaxies using a neo-mond formalism, and the subsequent derivation of a complete theory of the baryonic Tully-Fisher relation. D. F. Roscoe (The Open University; D.Roscoe@open.ac.uk)

More information

Keywords: Fractal Cosmology, WiggleZ, Hubble s Law, General Relativity, Galaxy Distribution, Cosmological Principle

Keywords: Fractal Cosmology, WiggleZ, Hubble s Law, General Relativity, Galaxy Distribution, Cosmological Principle Observed Galaxy Distribution Transition with Increasing Redshift a Property of the Fractal Blair D. Macdonald First Published: November 20th 2014. Abstract Is the universe a fractal? This is one of the

More information

astro-ph/ Jan 1995

astro-ph/ Jan 1995 UTAP-96/95 January, 995 WEAKLY NONLINEAR EVOLUTION OF TOPOLOGY OF LARGE-SCALE STRUCTURE Takahiko Matsubara Department of Physics, The University of Tokyo Tokyo,, Japan and Department of Physics, Hiroshima

More information

On the Large-Scale Structure of the Universe as given by the Voronoi Diagrams

On the Large-Scale Structure of the Universe as given by the Voronoi Diagrams Chin. J. Astron. Astrophys. Vol. 6 (2006), No. 4, 387 395 (http://www.chjaa.org) Chinese Journal of Astronomy and Astrophysics On the Large-Scale Structure of the Universe as given by the Voronoi Diagrams

More information

The supercluster-void network V.

The supercluster-void network V. (will be inserted by hand later) Your thesaurus codes are: 12 (12.3.3; 12.12.1) AND ASTROPHYSICS October 17, 2 The supercluster-void network V. Alternative evidence for its regularity O. Toomet 1, H. Andernach

More information

arxiv:astro-ph/ v1 19 Jan 2005

arxiv:astro-ph/ v1 19 Jan 2005 Europhysics Letters PREPRINT Fractals versus halos: asymptotic scaling without fractal properties arxiv:astro-ph/0501409v1 19 Jan 2005 M. Bottaccio 1,3, M.Montuori 1,3 and L. Pietronero 1,2,3 1 Center

More information

arxiv: v1 [astro-ph.co] 3 Feb 2018

arxiv: v1 [astro-ph.co] 3 Feb 2018 Spatial Distribution of Gamma-Ray Burst Sources S. I. Shirokov, 1 A. A. Raikov, 2 and Yu. V. Baryshev 1 1 St. Petersburg State University, Universitetskii pr. 28, St. Petersburg 198504, Russia 2 Main (Pulkovo)

More information

Twenty-six dimensional polytope and high energy spacetime physics

Twenty-six dimensional polytope and high energy spacetime physics From the SelectedWorks of Ji-Huan He 2007 Twenty-six dimensional polytope and high energy spacetime physics Ji-Huan He, Donghua University Lan Xu Li-Na Zhang Xu-Hong Wu Available at: https://works.bepress.com/ji_huan_he/40/

More information

Is the Universe Homogeneous on Large Scales?

Is the Universe Homogeneous on Large Scales? Is the Universe Homogeneous on Large Scales? arxiv:astro-ph/9610149v2 21 Oct 1996 Marc Davis Depts. of Astronomy and Physics University of California, Berkeley January 14, 2014 1 Two Competing Visions

More information

arxiv:hep-ph/ v1 21 Aug 1995

arxiv:hep-ph/ v1 21 Aug 1995 JHU-TIPAC 9503 Modifications of the Hubble Law in a Scale-Dependent Cosmology arxiv:hep-ph/9508336v1 1 Aug 1995 C. W. Kim a, T.H. Lee a,b and J. Song a a Department of Physics and Astronomy The Johns Hopkins

More information

FRACTAL SPACE-TIME THEORY AND SUPERCONDUCTIVITY

FRACTAL SPACE-TIME THEORY AND SUPERCONDUCTIVITY GENERAL PHYSICS RELATIVITY FRACTAL SPACE-TIME THEORY AND SUPERCONDUCTIVITY M. AGOP 1, V. ENACHE, M. BUZDUGAN 1 Department of Physics, Technical Gh. Asachi University, Iaºi 70009, România Faculty of Physics,

More information

FromBigCrunchToBigBang IsItPossible? Nathan Seiberg School of Natural Sciences Institute for Advanced Study Princeton, NJ 08540, USA.

FromBigCrunchToBigBang IsItPossible? Nathan Seiberg School of Natural Sciences Institute for Advanced Study Princeton, NJ 08540, USA. hep-th/0201039 FromBigCrunchToBigBang IsItPossible? Nathan Seiberg School of Natural Sciences Institute for Advanced Study Princeton, NJ 08540, USA seiberg@ias.edu ABSTRACT We discuss the possibility of

More information

Redshift survey with multiple pencil beams at the galactic poles

Redshift survey with multiple pencil beams at the galactic poles Proc. Natl. Acad. Sci. USA Vol. 90, pp. 4853-4858, June 1993 Colloquium Paper This paper was presented at a couoquium entitled "Physical Cosmology," organized by a committee chaired by David N. Schramm,

More information

Measures of Cosmic Structure

Measures of Cosmic Structure Measures of Cosmic Structure Lecture course LSS2009 University Groningen Apr. 2009-July 2009 If Standard you want to Reference: know more... Martinez & Saar 1 Ergodic Theorem Statistical Cosmological Principle

More information

LARGE QUASAR GROUPS. Kevin Rahill Astrophysics

LARGE QUASAR GROUPS. Kevin Rahill Astrophysics LARGE QUASAR GROUPS Kevin Rahill Astrophysics QUASARS Quasi-stellar Radio Sources Subset of Active Galactic Nuclei AGNs are compact and extremely luminous regions at the center of galaxies Identified as

More information

arxiv:astro-ph/ v1 22 Jun 2005

arxiv:astro-ph/ v1 22 Jun 2005 EPJ manuscript No. (will be inserted by the editor) Zipf s law for fractal voids and a new void-finder José Gaite arxiv:astro-ph/0506543v1 22 Jun 2005 Instituto de Matemáticas y Física Fundamental, CSIC,

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

Approaching a homogeneous galaxy distribution: results from the Stromlo-APM redshift survey

Approaching a homogeneous galaxy distribution: results from the Stromlo-APM redshift survey Mon. Not. R. Astron. Soc. 000, 000 000 (0000) Printed 31 August 1999 (MN LATEX style file v1.4) Approaching a homogeneous galaxy distribution: results from the Stromlo-APM redshift survey Steve Hatton

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

Ay 127. Large Scale Structure: Basic Observations, Redshift Surveys, Biasing

Ay 127. Large Scale Structure: Basic Observations, Redshift Surveys, Biasing Ay 127 Large Scale Structure: Basic Observations, Redshift Surveys, Biasing Structure Formation and Evolution From this (Δρ/ρ ~ 10-6 ) to this (Δρ/ρ ~ 10 +2 ) to this (Δρ/ρ ~ 10 +6 ) How Long Does It

More information

arxiv: v1 [physics.gen-ph] 29 May 2014

arxiv: v1 [physics.gen-ph] 29 May 2014 Noname manuscript No. will be inserted by the editor) Can negative mass be considered in General Relativity? Jean-Pierre Petit Gilles dagostini arxiv:1408.451v1 [physics.gen-ph] 9 May 014 Received: date

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

brane world cosmology An introduction to Andreas Müller Theory group LSW Advanced seminar LSW Heidelberg 03/03/2004

brane world cosmology An introduction to Andreas Müller Theory group LSW Advanced seminar LSW Heidelberg 03/03/2004 An introduction to brane world cosmology Andreas Müller Theory group LSW http://www.lsw.uni-heidelberg.de/users/amueller Advanced seminar LSW Heidelberg 03/03/2004 Overview principles bulk and brane extradimensions

More information

The large-scale smoothness of the Universe

The large-scale smoothness of the Universe The large-scale smoothness of the Universe Kelvin K. S. Wu, Ofer Lahav & Martin J. Rees... The Universe is inhomogeneousðand essentially fractalðon the scale of galaxies and clusters of galaxies, but most

More information

The Multiplicity Function of groups of galaxies from CRoNaRio catalogues

The Multiplicity Function of groups of galaxies from CRoNaRio catalogues The Multiplicity Function of groups of galaxies from CRoNaRio catalogues E. DE FILIPPIS 1,G.LONGO 2, S. ANDREON 2, R. SCARAMELLA 3,TESTAV. 3,R.DE CARVALHO 4,G.DJORGOVSKI 5 1 Università Federico II, Naples,

More information

Galaxies 626. Lecture 3: From the CMBR to the first star

Galaxies 626. Lecture 3: From the CMBR to the first star Galaxies 626 Lecture 3: From the CMBR to the first star Galaxies 626 Firstly, some very brief cosmology for background and notation: Summary: Foundations of Cosmology 1. Universe is homogenous and isotropic

More information

The redshift periodicity of galaxies as a probe of the correctness of general relativity

The redshift periodicity of galaxies as a probe of the correctness of general relativity The redshift periodicity of galaxies as a probe of the correctness of general relativity Valerio Faraoni Department of Physics and Astronomy, University of Victoria P.O. Box 3055, Victoria, B.C. Canada

More information

arxiv:gr-qc/ v3 17 Jul 2003

arxiv:gr-qc/ v3 17 Jul 2003 REGULAR INFLATIONARY COSMOLOGY AND GAUGE THEORIES OF GRAVITATION A. V. Minkevich 1 Department of Theoretical Physics, Belarussian State University, av. F. Skoriny 4, 0050, Minsk, Belarus, phone: +37517095114,

More information

Fractals and the Large-Scale Structure in the Universe

Fractals and the Large-Scale Structure in the Universe Fractals and the Large-Scale Structure in the Universe 2. Is the Cosmological Principle Valid? A K Mittal and T R Seshadri In Part 1 of this article, we had introduced the reader to some basic concepts

More information

Structure Formation and Evolution"

Structure Formation and Evolution Structure Formation and Evolution" From this (Δρ/ρ ~ 10-6 )! to this! (Δρ/ρ ~ 10 +2 )! to this! (Δρ/ρ ~ 10 +6 )! How Long Does It Take?" The (dissipationless) gravitational collapse timescale is on the

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 ESO Slice Project (ESP) galaxy redshift survey

The ESO Slice Project (ESP) galaxy redshift survey Astron. Astrophys. 325, 954 960 (1997) ASTRONOMY AND ASTROPHYSICS The ESO Slice Project (ESP) galaxy redshift survey I. Description and first results G. Vettolani 1, E. Zucca 2,1, G. Zamorani 2,1, A. Cappi

More information

Cosmic Strings and Other Topological Defects. by A. Vilenkin and E. P. S. Shellard. Reviewed by John Preskill. 28 March 1996

Cosmic Strings and Other Topological Defects. by A. Vilenkin and E. P. S. Shellard. Reviewed by John Preskill. 28 March 1996 Cosmic Strings and Other Topological Defects by A. Vilenkin and E. P. S. Shellard Reviewed by John Preskill 28 March 1996 One of the most ironic twists of twentieth century science, and one of the most

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

Cylindrical Coordinates

Cylindrical Coordinates SEARCH MATHWORLD Algebra Applied Mathematics Calculus and Analysis Discrete Mathematics Foundations of Mathematics Geometry History and Terminology Number Theory Probability and Statistics Recreational

More information

arxiv:astro-ph/ v1 10 Mar 1998

arxiv:astro-ph/ v1 10 Mar 1998 Southern Sky Redshift Survey: Clustering of Local Galaxies C. N. A. Willmer Observatório Nacional, Rua General José Cristino 77, Rio de Janeiro, RJ 2092-030, Brazil electronic mail: cnaw@on.br arxiv:astro-ph/98038v

More information

arxiv:gr-qc/ v1 17 Mar 2005

arxiv:gr-qc/ v1 17 Mar 2005 A new time-machine model with compact vacuum core Amos Ori Department of Physics, Technion Israel Institute of Technology, Haifa, 32000, Israel (May 17, 2006) arxiv:gr-qc/0503077 v1 17 Mar 2005 Abstract

More information

Physics 133: Extragalactic Astronomy ad Cosmology

Physics 133: Extragalactic Astronomy ad Cosmology Physics 133: Extragalactic Astronomy ad Cosmology Lecture 4; January 15 2014 Previously The dominant force on the scale of the Universe is gravity Gravity is accurately described by the theory of general

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

The egg-carton Universe

The egg-carton Universe The egg-carton Universe E. Battaner and E. Florido February 4, 1998 The distribution of superclusters in the Local Supercluster neighbourhood presents such a remarkable periodicity that some kind of network

More information

Stability of the Einstein static universe in the presence of vacuum energy

Stability of the Einstein static universe in the presence of vacuum energy PHYSICAL REVIEW D 80, 043528 (2009) Stability of the Einstein static universe in the presence of vacuum energy Saulo Carneiro 1,2, * and Reza Tavakol 1, 1 Astronomy Unit, School of Mathematical Sciences,

More information

Article. Reference. Angular projections of fractal sets. DURRER, Ruth, et al.

Article. Reference. Angular projections of fractal sets. DURRER, Ruth, et al. Article Angular projections of fractal sets DURRER, Ruth, et al Abstract We discuss various questions which arise when one considers the central projection of three-dimensional fractal sets (galaxy catalogs)

More information

International Journal of Applied and Universal Research E-ISSN No: Volume III, Issue V, Sept-Oct Available online at:

International Journal of Applied and Universal Research E-ISSN No: Volume III, Issue V, Sept-Oct Available online at: COSMOLOGICAL MODELS BIANCHI TYPE II WITH BULK VISCOSITY IN GENERAL THEORY OF RELATIVITY R.K. Dubey 1, Shishir Kumar Srivastava 2, Dhirendra Tripathi 3 1 Department of Mathematics Govt. S.K.N.P.G. College,

More information

On the synchronization of a class of electronic circuits that exhibit chaos

On the synchronization of a class of electronic circuits that exhibit chaos Chaos, Solitons and Fractals 13 2002) 1515±1521 www.elsevier.com/locate/chaos On the synchronization of a class of electronic circuits that exhibit chaos Er-Wei Bai a, *, Karl E. Lonngren a, J.C. Sprott

More information

Quantum golden field theory Ten theorems and various conjectures

Quantum golden field theory Ten theorems and various conjectures Available online at www.sciencedirect.com Chaos, Solitons and Fractals 36 (2008) 2 25 www.elsevier.com/locate/chaos Quantum golden field theory Ten theorems and various conjectures M.S. El Naschie * Department

More information

Variational Iteration Method for Solving Nonlinear Coupled Equations in 2-Dimensional Space in Fluid Mechanics

Variational Iteration Method for Solving Nonlinear Coupled Equations in 2-Dimensional Space in Fluid Mechanics Int J Contemp Math Sciences Vol 7 212 no 37 1839-1852 Variational Iteration Method for Solving Nonlinear Coupled Equations in 2-Dimensional Space in Fluid Mechanics A A Hemeda Department of Mathematics

More information

SOLVING THE HORIZON PROBLEM WITH A DELAYED BIG-BANG SINGULARITY

SOLVING THE HORIZON PROBLEM WITH A DELAYED BIG-BANG SINGULARITY SOLVING THE HORIZON PROBLEM WITH A DELAYED BIG-BANG SINGULARITY Marie-Noëlle CÉLÉRIER Département d Astrophysique Relativiste et de Cosmologie Observatoire de Paris Meudon 5 Place Jules Janssen 92195 Meudon

More information

The supercluster void network

The supercluster void network ASTRONOMY & ASTROPHYSICS MAY II 1997, PAGE 119 SUPPLEMENT SERIES Astron. Astrophys. Suppl. Ser. 123, 119-133 (1997) The supercluster void network I. The supercluster catalogue and large-scale distribution

More information

arxiv:astro-ph/ v1 14 Dec 1998

arxiv:astro-ph/ v1 14 Dec 1998 Proceedings: Evolution of Large Scale Structure Garching, August 1998 GALAXY REDSHIFT SURVEYS: 20 YEARS LATER Luiz da Costa 1 1 ESO, Karl-Schwarzschildstr. 2, D 85748 Garching arxiv:astro-ph/9812258v1

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

EKPYROTIC SCENARIO IN STRING THEORY. Kunihito Uzawa Kwansei Gakuin University

EKPYROTIC SCENARIO IN STRING THEORY. Kunihito Uzawa Kwansei Gakuin University EKPYROTIC SCENARIO IN STRING THEORY Kunihito Uzawa Kwansei Gakuin University [1] Introduction The Ekpyrosis inspired by string theory and brane world model suggests alternative solutions to the early universe

More information

Superclusters...what are they? They are Superfun!

Superclusters...what are they? They are Superfun! Superclusters...what are they? They are Superfun! General background The Local Supercluster Observations Structure at high z Formation theory Current research General background Groups and clusters: Galactic

More information

EVALUATING THE EXACT INFINITESIMAL

EVALUATING THE EXACT INFINITESIMAL EVALUATING THE EXACT INFINITESIMAL VALUES OF AREA OF SIERPINSKI S CARPET AND VOLUME OF MENGER S SPONGE Yaroslav D. Sergeyev Dipartimento di Elettronica, Informatica e Sistemistica, Università della Calabria,

More information

Proceedings of the Workshop

Proceedings of the Workshop Proceedings of the Workshop Astro-particle physics Ringberg Castle 15.10-19.10 1996 F. Sylos Labini, L. Pietronero and M. Montuori INFM Sezione di Roma1, and Dipartimento di Fisica, Università di Roma

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

Spherical Coordinates

Spherical Coordinates SEARCH MATHWORLD Algebra Applied Mathematics Calculus and Analysis Discrete Mathematics Foundations of Mathematics Geometry History and Terminology Number Theory Probability and Statistics Recreational

More information

Parametric convergence and control of chaotic system using adaptive feedback linearization

Parametric convergence and control of chaotic system using adaptive feedback linearization Available online at www.sciencedirect.com Chaos, Solitons and Fractals 4 (29) 1475 1483 www.elsevier.com/locate/chaos Parametric convergence and control of chaotic system using adaptive feedback linearization

More information

Alternatives To Inflation. Jean-Luc Lehners MPI for Gravitational Physics Albert-Einstein-Institute

Alternatives To Inflation. Jean-Luc Lehners MPI for Gravitational Physics Albert-Einstein-Institute Alternatives To Inflation Jean-Luc Lehners MPI for Gravitational Physics Albert-Einstein-Institute PLANCK data A simple universe: approximately homogeneous, isotropic, flat With, in addition, nearly scale-invariant,

More information

The Endless Universe: A Brief Introduction 1

The Endless Universe: A Brief Introduction 1 The Endless Universe: A Brief Introduction 1 PAUL J. STEINHARDT Professor of Physics, Princeton University The cyclic model of the universe is a radical alternative to standard big bang/inflationary theory

More information

Introduction to Cosmology

Introduction to Cosmology Introduction to Cosmology João G. Rosa joao.rosa@ua.pt http://gravitation.web.ua.pt/cosmo LECTURE 2 - Newtonian cosmology I As a first approach to the Hot Big Bang model, in this lecture we will consider

More information

Gravitational lensing constraint on the cosmic equation of state

Gravitational lensing constraint on the cosmic equation of state Gravitational lensing constraint on the cosmic equation of state arxiv:astro-ph/0105551v1 31 May 2001 Deepak Jain, Abha Dev, N. Panchapakesan S. Mahajan and V. B. Bhatia Department of Physics and Astrophysics

More information

From General Relativity to A Simple-Harmonically Oscillating Universe, and Vice-Versa: A Review

From General Relativity to A Simple-Harmonically Oscillating Universe, and Vice-Versa: A Review Applied Physics Research; Vol. 9, No. 1; 2017 ISSN 1916-969 E-ISSN 1916-9647 Published by Canadian Center of Science and Education From General Relativity to A Simple-Harmonically Oscillating Universe,

More information

Nonarchimedean Cantor set and string

Nonarchimedean Cantor set and string J fixed point theory appl Online First c 2008 Birkhäuser Verlag Basel/Switzerland DOI 101007/s11784-008-0062-9 Journal of Fixed Point Theory and Applications Nonarchimedean Cantor set and string Michel

More information

METHOD FOR ANALYZING THE SPATIAL DISTRIBUTION OF GALAXIES ON GIGAPARSEC SCALES. II. APPLICATION TO A GRID OF THE HUDF-FDF-COSMOS-HDF SURVEYS

METHOD FOR ANALYZING THE SPATIAL DISTRIBUTION OF GALAXIES ON GIGAPARSEC SCALES. II. APPLICATION TO A GRID OF THE HUDF-FDF-COSMOS-HDF SURVEYS METHOD FOR ANALYZING THE SPATIAL DISTRIBUTION OF GALAXIES ON GIGAPARSEC SCALES. II. APPLICATION TO A GRID OF THE HUDF-FDF-COSMOS-HDF SURVEYS N.V.NABOKOV and Yu.V.BARYSHEV 1 Using the deep fields of COSMOS,

More information

Return to cosmology. Is inflation in trouble? Are we cycling back to cycles? And then what happens to the 2 nd law?

Return to cosmology. Is inflation in trouble? Are we cycling back to cycles? And then what happens to the 2 nd law? Return to cosmology Is inflation in trouble? Are we cycling back to cycles? And then what happens to the 2 nd law? We saw inflation correctly predict: 1. Flatness of universe 2. Homogeneity of universe

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

Cosmology with Clusters of Galaxies

Cosmology with Clusters of Galaxies Cosmology with Clusters of Galaxies arxiv:astro-ph/9901076v1 8 Jan 1999 Neta A. Bahcall Princeton University Observatory Princeton, NJ 08544 December 31, 1998 Abstract Rich clusters of galaxies, the largest

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

A5682: Introduction to Cosmology Course Notes. 11. CMB Anisotropy

A5682: Introduction to Cosmology Course Notes. 11. CMB Anisotropy Reading: Chapter 9, sections 9.4 and 9.5 11. CMB Anisotropy Gravitational instability and structure formation Today s universe shows structure on scales from individual galaxies to galaxy groups and clusters

More information

The angular homogeneity scale of the Universe

The angular homogeneity scale of the Universe The angular homogeneity scale of the Universe Alicia Bueno Belloso ITP, Heidelberg Work in collaboration with: David Alonso, Juan García-Bellido, Eusebio Sánchez and Javier Sánchez in preparation 2 nd

More information

Dynamical compactification from higher dimensional de Sitter space

Dynamical compactification from higher dimensional de Sitter space Dynamical compactification from higher dimensional de Sitter space Matthew C. Johnson Caltech In collaboration with: Sean Carroll Lisa Randall 0904.3115 Landscapes and extra dimensions Extra dimensions

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

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

The angular homogeneity scale of the Universe

The angular homogeneity scale of the Universe The angular homogeneity scale of the Universe Alicia Bueno Belloso Work in collaboration with: David Alonso, Juan García-Bellido, Eusebio Sánchez and Javier Sánchez in preparation 12 th of September 2013

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

Lecture 14: Cosmological Principles

Lecture 14: Cosmological Principles Lecture 14: Cosmological Principles The basic Cosmological Principles The geometry of the Universe The scale factor R and curvature constant k Comoving coordinates Einstein s initial solutions 3/28/11

More information

The Tolman-Bondi Model in the Ruban-Chernin Coordinates. 1. Equations and Solutions.

The Tolman-Bondi Model in the Ruban-Chernin Coordinates. 1. Equations and Solutions. The Tolman-Bondi Model in the Ruban-Chernin Coordinates.. Equations and Solutions. arxiv:gr-qc/9638v 5 Dec 996 Alexander Gromov March, 8 Abstract It is demonstrated that the system of coordinates {M, t}

More information

A multiple Riccati equations rational expansion method and novel solutions of the Broer Kaup Kupershmidt system

A multiple Riccati equations rational expansion method and novel solutions of the Broer Kaup Kupershmidt system Chaos, Solitons and Fractals 30 (006) 197 03 www.elsevier.com/locate/chaos A multiple Riccati equations rational expansion method and novel solutions of the Broer Kaup Kupershmidt system Qi Wang a,c, *,

More information

astro-ph/ Jul 94

astro-ph/ Jul 94 Mon. Not. R. Astron. Soc. 000, 000{000 (1994) The Two-Point Correlation Function of Rich Clusters of Galaxies: Results From An Extended APM Cluster Redshift Survey G. B. Dalton 1, R. A. C. Croft 1, G.

More information

Controlling chaos in Colpitts oscillator

Controlling chaos in Colpitts oscillator Chaos, Solitons and Fractals 33 (2007) 582 587 www.elsevier.com/locate/chaos Controlling chaos in Colpitts oscillator Guo Hui Li a, *, Shi Ping Zhou b, Kui Yang b a Department of Communication Engineering,

More information

COSMOLOGY PHYS 30392 OBSERVING THE UNIVERSE Part I Giampaolo Pisano - Jodrell Bank Centre for Astrophysics The University of Manchester - January 2013 http://www.jb.man.ac.uk/~gp/ giampaolo.pisano@manchester.ac.uk

More information

LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS.

LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS. LOCALIZATION OF FIELDS ON A BRANE IN SIX DIMENSIONS Merab Gogberashvili a and Paul Midodashvili b a Andronikashvili Institute of Physics, 6 Tamarashvili Str., Tbilisi 3877, Georgia E-mail: gogber@hotmail.com

More information

Cosmology. Clusters of galaxies. Redshift. Late 1920 s: Hubble plots distances versus velocities of galaxies. λ λ. redshift =

Cosmology. Clusters of galaxies. Redshift. Late 1920 s: Hubble plots distances versus velocities of galaxies. λ λ. redshift = Cosmology Study of the structure and origin of the universe Observational science The large-scale distribution of galaxies Looking out to extremely large distances The motions of galaxies Clusters of galaxies

More information

Synchronization of an uncertain unified chaotic system via adaptive control

Synchronization of an uncertain unified chaotic system via adaptive control Chaos, Solitons and Fractals 14 (22) 643 647 www.elsevier.com/locate/chaos Synchronization of an uncertain unified chaotic system via adaptive control Shihua Chen a, Jinhu L u b, * a School of Mathematical

More information

1 h 23 h. 2 h. 3 h. 22 h. 4 h 21 h. -39 o -42 o -45 o Dec. 30 cz (1000 km/s) South galaxies

1 h 23 h. 2 h. 3 h. 22 h. 4 h 21 h. -39 o -42 o -45 o Dec. 30 cz (1000 km/s) South galaxies LARGE SCALE STRUCTURE OF THE UNIVERSE NETA A. BAHCALL Princeton University Observatory Princeton, NJ Abstract How is the universe organized on large scales? How did this structure evolve from the unknown

More information

A5682: Introduction to Cosmology Course Notes. 11. CMB Anisotropy

A5682: Introduction to Cosmology Course Notes. 11. CMB Anisotropy Reading: Chapter 8, sections 8.4 and 8.5 11. CMB Anisotropy Gravitational instability and structure formation Today s universe shows structure on scales from individual galaxies to galaxy groups and clusters

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

PHY 475/375. Lecture 5. (April 9, 2012)

PHY 475/375. Lecture 5. (April 9, 2012) PHY 475/375 Lecture 5 (April 9, 2012) Describing Curvature (contd.) So far, we have studied homogenous and isotropic surfaces in 2-dimensions. The results can be extended easily to three dimensions. As

More information

Advanced Study, 9 Adela Court, Mulgrave, Victoria 3170, Australia

Advanced Study, 9 Adela Court, Mulgrave, Victoria 3170, Australia ON OLBERS PARADOX Vu B Ho Advanced Study, 9 Adela Court, Mulgrave, Victoria 3170, Australia Email: vubho@bigpond.net.au Abstract: In this work we discuss a possibility to resolve Olbers paradox that states

More information

Class 5 Cosmology Large-Scale Structure of the Universe What do we see? Big Bang Cosmology What model explains what we see?

Class 5 Cosmology Large-Scale Structure of the Universe What do we see? Big Bang Cosmology What model explains what we see? Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System

More information

Computers and Mathematics with Applications. Chaos suppression via periodic pulses in a class of piece-wise continuous systems

Computers and Mathematics with Applications. Chaos suppression via periodic pulses in a class of piece-wise continuous systems Computers and Mathematics with Applications 64 (2012) 849 855 Contents lists available at SciVerse ScienceDirect Computers and Mathematics with Applications journal homepage: www.elsevier.com/locate/camwa

More information

arxiv: v1 [astro-ph.co] 25 Sep 2012

arxiv: v1 [astro-ph.co] 25 Sep 2012 Draft version May 23, 2018 Preprint typeset using L A TEX style emulateapj v. 5/2/11 THE CHALLENGE OF THE LARGEST STRUCTURES IN THE UNIVERSE TO COSMOLOGY arxiv:1209.5659v1 [astro-ph.co] 25 Sep 2012 Changbom

More information

p-adic AND ADELIC GRAVITY AND COSMOLOGY

p-adic AND ADELIC GRAVITY AND COSMOLOGY p-adic AND ADELIC GRAVITY AND COSMOLOGY Branko Dragovich http://www.phy.bg.ac.yu/ dragovich dragovich@ipb.ac.rs Institute of Physics University of Belgrade Belgrade, Serbia ISAAC2013: 9th International

More information

Inflationary Cosmology: Progress and Problems

Inflationary Cosmology: Progress and Problems 1 / 95 ary Cosmology: Progress and Robert McGill University, Canada and Institute for Theoretical Studies, ETH Zuerich, Switzerland NAO Colloquium, Sept. 23, 2015 2 / 95 Outline 1 2 Review of ary Cosmology

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