Derivation of parametric equations of the expansion of a closed universe with torsion. Prastik Mohanraj

Size: px
Start display at page:

Download "Derivation of parametric equations of the expansion of a closed universe with torsion. Prastik Mohanraj"

Transcription

1 Derivation of parametric equations of the expansion of a closed universe with torsion Prastik Mohanraj

2 Big Bang Cosmology We observe redshift, where galaxies become redder in color over time. This means that the galaxies are speeding away from us. So, we can see that the universe must be expanding. If the universe is expanding, it must have been smaller, denser, and hotter in the past. Thus, it is likely that the universe started from something extremely small, that being the Big Bang. Source: BBC iwonder

3 Models of the Universe The 3D plane of the universe is curved around the 4D hyperspace of the universe in one of these three different shapes. This is a result of matter-energy density on the largest scales in the universe. These images are of the Cosmic Microwave Background Radiation, which is a footprint left by the hot universe around 380,000 years after the Big Bang. The observed CMB fluctuations in temperature give information about the earliest moments of the universe.

4 Closed Universe Constant positive curvature (k = 1) A three-dimensional hypersurface of a fourdimensional hypersphere Analogous to two-dimensional surface of three-dimensional ball Scale factor a = Radius of fourdimensional hypersphere

5 Closed Universe Expansion The further two galaxies are from each other, the faster they recede from one another in an expanding universe: Hubble s Law If the universe is expanding, then it would be impossible to go around the universe since one would need to exceed the speed of light some parts of the universe appear to expand faster than other parts from an observer s view Source: One-Minute Astronomer

6 Friedmann Equations a = scale factor of universe k = curvature factor (-1, 0, or +1) ε = energy density of universe κ = constant value p = pressure f(a, ε) = 0 except for the immediate beginning of the universe

7 Friedmann Equations Model Period p-ε Relationship Second Friedmann Equation Model Relativistic (Radiation- Dominated) Nonrelativistic (Matter-Dominated) Second Friedmann Equation Result Revised First Friedmann Equation Model

8 Cycloid When a circle rolls along the plane, the curve connecting the position of one distinct point on the circle at different times produces a cycloid Geometric derivation of x, y coordinates yields parametric equations

9 Cycloid with the Nonrelativistic Friedmann Equations The result is equivalent to the nonrelativistic Friedmann Equation model, thus the cycloid function is a solution to the nonrelativistic universe expansion.

10 Dilemma In the diagram, there are points where the scale factor = a on the vertical axis is equal to 0 This means that the universe has become a point, with infinite density: a singularity This can be avoided with Einstein-Cartan Theory, which uses a torsion tensor to eliminate gravitational singularities

11 Trochoid The coefficients of the parametric functions for x, y are changed to: As long as A > B, the scale factor = a will always be a positive value Notice how the a = dt dθ here result from the cycloid function is preserved Another format for writing the scale factor = a in the trochoid function is

12 Revised Friedmann Equation Model with the Torsion Factor The Friedmann Equation will be revised to incorporate the added torsion factor, which is only present in the beginning of the universe, thus, the relativistic model will be revised The revised Friedmann Equation model is: Notice how the coefficient A 2 B 2 will be close to 0 with A > B, and only make an impact on the function when a is very small Instead of a singularity with the Big Bang, the non-singular bounce of the universe at the minimum scale factor, creating an alternate Big Bounce The torsion factor approaches 0 rapidly after the Big Bounce, so the 2A term a makes the only impact 2 Thus, the torsion factor can be removed from the model after the Big Bounce

13 Novel Solution to Revised Model A solution to the model is: Here, The E(θ, k) function an elliptic integral of the second kind

14 Proof of Solution The The result is equivalent to the Friedmann Equation with the added torsion factor, thus this is a working solution to the model.

15 As B A, torsion disappears Torsion fully disappears when torsion factor = 0 : This is when A = B This result gets substituted into the parametric equations to obtain: Substituting these functions a and t into the relativistic model without the torsion factor yields a true result. Thus, this solution is true.

16 Dark Energy Universe Dark energy is present only in the nonrelativistic, matter-dominated era The dark energy factor is proportional to a 2, and will be added to the nonrelativistic model of the Friedmann equation, resulting in: Further into the universe s evolution, where a becomes extremely high, this model reaches the limit of: This is the exponential increase behavior of scale factor that we expect in a dark-energy dominated era, thus the model is valid

17 Conclusion Here, we have presented models of the Friedmann Equations incorporating different eras of the evolution of the universe The novel solution to the Big Bounce time period of a positively curved universe is presented here: and with These parametric equations are solutions to the Friedmann equations incorporating the Einstein-Cartan Theory torsion factor

18 Acknowledgements and References

Big Bounce and Inflation from Spin and Torsion Nikodem Popławski

Big Bounce and Inflation from Spin and Torsion Nikodem Popławski Big Bounce and Inflation from Spin and Torsion Nikodem Popławski Colloquium, Department of Physics Queens College, City University of New York, Queens, NY, USA November 12, 2018 Cosmic Microwave Background

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

Cosmology: The Origin and Evolution of the Universe Chapter Twenty-Eight. Guiding Questions

Cosmology: The Origin and Evolution of the Universe Chapter Twenty-Eight. Guiding Questions Cosmology: The Origin and Evolution of the Universe Chapter Twenty-Eight Guiding Questions 1. What does the darkness of the night sky tell us about the nature of the universe? 2. As the universe expands,

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

Black Hole Cosmology in Gravity with Torsion Nikodem Popławski

Black Hole Cosmology in Gravity with Torsion Nikodem Popławski Black Hole Cosmology in Gravity with Torsion Nikodem Popławski Department of Mathematics and Physics Seminar University of New Haven October 20, 2016 Cosmic Microwave Background Big Bang Licensed under

More information

Redshift-Distance Relationships

Redshift-Distance Relationships Redshift-Distance Relationships George Jones April 4, 0. Distances in Cosmology This note considers two conceptually important definitions of cosmological distances, look-back distance and proper distance.

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

Cosmology. Thornton and Rex, Ch. 16

Cosmology. Thornton and Rex, Ch. 16 Cosmology Thornton and Rex, Ch. 16 Expansion of the Universe 1923 - Edwin Hubble resolved Andromeda Nebula into separate stars. 1929 - Hubble compared radial velocity versus distance for 18 nearest galaxies.

More information

Olbers Paradox. Lecture 14: Cosmology. Resolutions of Olbers paradox. Cosmic redshift

Olbers Paradox. Lecture 14: Cosmology. Resolutions of Olbers paradox. Cosmic redshift Lecture 14: Cosmology Olbers paradox Redshift and the expansion of the Universe The Cosmological Principle Ω and the curvature of space The Big Bang model Primordial nucleosynthesis The Cosmic Microwave

More information

Cosmology ASTR 2120 Sarazin. Hubble Ultra-Deep Field

Cosmology ASTR 2120 Sarazin. Hubble Ultra-Deep Field Cosmology ASTR 2120 Sarazin Hubble Ultra-Deep Field Cosmology - Da Facts! 1) Big Universe of Galaxies 2) Sky is Dark at Night 3) Isotropy of Universe Cosmological Principle = Universe Homogeneous 4) Hubble

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

with Matter and Radiation By: Michael Solway

with Matter and Radiation By: Michael Solway Interactions of Dark Energy with Matter and Radiation By: Michael Solway Advisor: Professor Mike Berger What is Dark Energy? Dark energy is the energy needed to explain the observed accelerated expansion

More information

MIT Exploring Black Holes

MIT Exploring Black Holes THE UNIVERSE and Three Examples Alan Guth, MIT MIT 8.224 Exploring Black Holes EINSTEIN'S CONTRIBUTIONS March, 1916: The Foundation of the General Theory of Relativity Feb, 1917: Cosmological Considerations

More information

Hubble's Law. H o = 71 km/s / Mpc. The further a galaxy is away, the faster it s moving away from us. V = H 0 D. Modern Data.

Hubble's Law. H o = 71 km/s / Mpc. The further a galaxy is away, the faster it s moving away from us. V = H 0 D. Modern Data. Cosmology Cosmology is the study of the origin and evolution of the Universe, addressing the grandest issues: How "big" is the Universe? Does it have an "edge"? What is its large-scale structure? How did

More information

The Big Bang. Olber s Paradox. Hubble s Law. Why is the night sky dark? The Universe is expanding and We cannot see an infinite Universe

The Big Bang. Olber s Paradox. Hubble s Law. Why is the night sky dark? The Universe is expanding and We cannot see an infinite Universe The Big Bang Olber s Paradox Why is the night sky dark? The Universe is expanding and We cannot see an infinite Universe Hubble s Law v = H0 d v = recession velocity in km/sec d = distance in Mpc H 0 =

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

Early (Expanding) Universe. Average temperature decreases with expansion.

Early (Expanding) Universe. Average temperature decreases with expansion. Early (Expanding) Universe Average temperature decreases with expansion. Particles & Anti-Particles Very short wavelength photons collide and form electron-positron pairs. E=mc 2 electron=matter positron=antimatter

More information

Big Bounce and Inflation from Spin and Torsion Nikodem Popławski

Big Bounce and Inflation from Spin and Torsion Nikodem Popławski Big Bounce and Inflation from Spin and Torsion Nikodem Popławski Institute for Theory and Computation Luncheon Harvard-Smithsonian Center for Astrophysics September 29, 2016 Cosmic Microwave Background

More information

The Dawn of Time - II. A Cosmos is Born

The Dawn of Time - II. A Cosmos is Born The Dawn of Time - II. A Cosmos is Born Learning Objectives! Why does Olbers paradox show the Universe began?! How does Hubble s Law tell us the age of the Universe? If Hubble s Constant is large, is the

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

You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator.

You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator. MATHEMATICAL TRIPOS Part III Friday 8 June 2001 1.30 to 4.30 PAPER 41 PHYSICAL COSMOLOGY Answer any THREE questions. The questions carry equal weight. You may not start to read the questions printed on

More information

Cosmology Dark Energy Models ASTR 2120 Sarazin

Cosmology Dark Energy Models ASTR 2120 Sarazin Cosmology Dark Energy Models ASTR 2120 Sarazin Late Homeworks Last day Wednesday, May 1 My mail box in ASTR 204 Maximum credit 50% unless excused (but, better than nothing) Final Exam Thursday, May 2,

More information

Cosmology: Building the Universe.

Cosmology: Building the Universe. Cosmology: Building the Universe. The term has several different meanings. We are interested in physical cosmology - the study of the origin and development of the physical universe, and all the structure

More information

The Expanding Universe

The Expanding Universe Cosmology Expanding Universe History of the Universe Cosmic Background Radiation The Cosmological Principle Cosmology and General Relativity Dark Matter and Dark Energy Primitive Cosmology If the universe

More information

Is the Rate of Expansion of Our Universe. Really Accelerating?

Is the Rate of Expansion of Our Universe. Really Accelerating? Adv. Studies Theor. Phys., Vol. 5, 2011, no. 13, 633-638 Is the Rate of Expansion of Our Universe Really Accelerating? Nathalie Olivi-Tran 1,2 1 Laboratoire Charles Coulomb CNRS, UMR 5221, place Eugene

More information

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter. Olber s Paradox. Cosmology. Olber s Paradox. Assumptions 4/20/18

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter. Olber s Paradox. Cosmology. Olber s Paradox. Assumptions 4/20/18 Astronomy 113 Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter Cosmology ³The study of the origins, structure, and evolution of the universe ³Key moments: ²Einstein General Theory of Relativity ²Hubble

More information

Astronomy 113. Dr. Joseph E. Pesce, Ph.D Joseph E. Pesce, Ph.D.

Astronomy 113. Dr. Joseph E. Pesce, Ph.D Joseph E. Pesce, Ph.D. Astronomy 113 Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter 17-2 Cosmology ³ The study of the origins, structure, and evolution of the universe ³ Key moments: ² Einstein General Theory of Relativity

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

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

CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence

CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence that the Universe began with a Big Bang? How has the Universe

More information

The expansion of the Universe, and the big bang

The expansion of the Universe, and the big bang The expansion of the Universe, and the big bang Q: What is Hubble s law? A. The larger the galaxy, the faster it is moving way from us. B. The farther away the galaxy, the faster it is moving away from

More information

The Universe: What We Know and What we Don t. Fundamental Physics Cosmology Elementary Particle Physics

The Universe: What We Know and What we Don t. Fundamental Physics Cosmology Elementary Particle Physics The Universe: What We Know and What we Don t Fundamental Physics Cosmology Elementary Particle Physics 1 Cosmology Study of the universe at the largest scale How big is the universe? Where What Are did

More information

II. The Universe Around Us. ASTR378 Cosmology : II. The Universe Around Us 23

II. The Universe Around Us. ASTR378 Cosmology : II. The Universe Around Us 23 II. The Universe Around Us ASTR378 Cosmology : II. The Universe Around Us 23 Some Units Used in Astronomy 1 parsec distance at which parallax angle is 1 ; 1 pc = 3.086 10 16 m ( 3.26 light years; 1 kpc

More information

12. Relativistic Cosmology I. Simple Solutions to the Einstein Equations

12. Relativistic Cosmology I. Simple Solutions to the Einstein Equations 12. Relativistic Cosmology I. Simple Solutions to the Einstein Equations 1. Minkowski space Initial assumptions:! no matter (T µν = 0)! no gravitation (R σ µνρ = 0; i.e., zero curvature) Not realistic!

More information

Lecture 34: The Big Bang Readings: Sections 28-3 and 28-6

Lecture 34: The Big Bang Readings: Sections 28-3 and 28-6 Lecture 34: The Big Bang Readings: Sections 28-3 and 28-6 Key Ideas: Big Bang Model of the Universe Universe starts in a hot, dense state in the past Universe expands & cools with time Cosmological Redshift

More information

Chapter 29. The Hubble Expansion

Chapter 29. The Hubble Expansion Chapter 29 The Hubble Expansion The observational characteristics of the Universe coupled with theoretical interpretation to be discussed further in subsequent chapters, allow us to formulate a standard

More information

Astrophysics Lecture Notes

Astrophysics Lecture Notes Astrophysics Lecture Notes by: Eric Deir April 11, 2017 Pop Quiz!! Is the universe homogeneous? Roughly! If averaged over scales of 10 9 pc. Is the universe isotropic? Roughly! If you average over large

More information

3.1 Cosmological Parameters

3.1 Cosmological Parameters 3.1 Cosmological Parameters 1 Cosmological Parameters Cosmological models are typically defined through several handy key parameters: Hubble Constant Defines the Scale of the Universe R 0 H 0 = slope at

More information

The Concept of Inflation

The Concept of Inflation The Concept of Inflation Introduced by Alan Guth, circa 1980, to provide answers to the following 5 enigmas: 1. horizon problem. How come the cosmic microwave background radiation is so uniform in very

More information

Formation of the Universe. What evidence supports current scientific theory?

Formation of the Universe. What evidence supports current scientific theory? Formation of the Universe What evidence supports current scientific theory? Cosmology Cosmology is the study of the Nature, Structure, Origin, And fate of the universe. How did it all begin? Astronomers

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 7 Oct. 30, 2015 Today Relativistic Cosmology Dark Side of the Universe I: Dark Matter Assignments This week: read Hawley and

More information

FXA ρ 0 = 3(H 0 ) 2. UNIT G485 Module Universe Evolution. Candidates should be able to : age of the universe 1/H 0

FXA ρ 0 = 3(H 0 ) 2. UNIT G485 Module Universe Evolution. Candidates should be able to : age of the universe 1/H 0 1 Candidates should be able to : Explain that the standard (hot big bang) model of the universe implies a finite age for the universe. Select and use the expression : age of the universe 1/H 0 Describe

More information

FURTHER COSMOLOGY Book page T H E M A K E U P O F T H E U N I V E R S E

FURTHER COSMOLOGY Book page T H E M A K E U P O F T H E U N I V E R S E FURTHER COSMOLOGY Book page 675-683 T H E M A K E U P O F T H E U N I V E R S E COSMOLOGICAL PRINCIPLE Is the Universe isotropic or homogeneous? There is no place in the Universe that would be considered

More information

Module 3: Astronomy The Universe Topic 1 Content: Cosmology Presentation Notes

Module 3: Astronomy The Universe Topic 1 Content: Cosmology Presentation Notes Pretend that you have been given the opportunity to travel through time to explore cosmology. Cosmology is the study of how the universe formed and what will happen to it. Watch through your viewport as

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

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

Astronomy 150: Killer Skies Lecture 35, April 23

Astronomy 150: Killer Skies Lecture 35, April 23 Assignments: ICES available online Astronomy 150: Killer Skies Lecture 35, April 23 HW11 due next Friday: last homework! note: lowest HW score dropped but: HW11 material will be on Exam 3, so be sure to

More information

A A + B. ra + A + 1. We now want to solve the Einstein equations in the following cases:

A A + B. ra + A + 1. We now want to solve the Einstein equations in the following cases: Lecture 29: Cosmology Cosmology Reading: Weinberg, Ch A metric tensor appropriate to infalling matter In general (see, eg, Weinberg, Ch ) we may write a spherically symmetric, time-dependent metric in

More information

Chapter 21 Evidence of the Big Bang. Expansion of the Universe. Big Bang Theory. Age of the Universe. Hubble s Law. Hubble s Law

Chapter 21 Evidence of the Big Bang. Expansion of the Universe. Big Bang Theory. Age of the Universe. Hubble s Law. Hubble s Law Chapter 21 Evidence of the Big Bang Hubble s Law Universal recession: Slipher (1912) and Hubble found that all galaxies seem to be moving away from us: the greater the distance, the higher the redshift

More information

Cosmology. Chapter 18. Cosmology. Observations of the Universe. Observations of the Universe. Motion of Galaxies. Cosmology

Cosmology. Chapter 18. Cosmology. Observations of the Universe. Observations of the Universe. Motion of Galaxies. Cosmology Cosmology Chapter 18 Cosmology Cosmology is the study of the structure and evolution of the Universe as a whole How big is the Universe? What shape is it? How old is it? How did it form? What will happen

More information

Implications of the Hubble Law: - it is not static, unchanging - Universe had a beginning!! - could not have been expanding forever HUBBLE LAW:

Implications of the Hubble Law: - it is not static, unchanging - Universe had a beginning!! - could not have been expanding forever HUBBLE LAW: Cosmology and the Evolution of the Universe Edwin Hubble, 1929: -almost all galaxies have a redshift -moving away from us -greater distance greater redshift Implications of the Hubble Law: - Universe is

More information

Cosmology and the Evolution of the Universe. Implications of the Hubble Law: - Universe is changing (getting bigger!) - it is not static, unchanging

Cosmology and the Evolution of the Universe. Implications of the Hubble Law: - Universe is changing (getting bigger!) - it is not static, unchanging Cosmology and the Evolution of the Edwin Hubble, 1929: -almost all galaxies have a redshift -moving away from us -exceptions in Local Group -with distance measurements - found a relationship greater distance

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

The Early Universe: A Journey into the Past

The Early Universe: A Journey into the Past Gravity: Einstein s General Theory of Relativity The Early Universe A Journey into the Past Texas A&M University March 16, 2006 Outline Gravity: Einstein s General Theory of Relativity Galileo and falling

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

The Early Universe: A Journey into the Past

The Early Universe: A Journey into the Past The Early Universe A Journey into the Past Texas A&M University March 16, 2006 Outline Galileo and falling bodies Galileo Galilei: all bodies fall at the same speed force needed to accelerate a body is

More information

Was the Universe Born Inside a Black Hole? Charles Peterson BS Mechanical Engineering Faculty Mentors: Dr. Nikodem Poplawski and Dr.

Was the Universe Born Inside a Black Hole? Charles Peterson BS Mechanical Engineering Faculty Mentors: Dr. Nikodem Poplawski and Dr. Was the Universe Born Inside a Black Hole? Charles Peterson BS Mechanical Engineering Faculty Mentors: Dr. Nikodem Poplawski and Dr. Chris Haynes Abstract Black-Hole Cosmology (BHC) proposes that every

More information

Unication models of dark matter and dark energy

Unication models of dark matter and dark energy Unication models of dark matter and dark energy Neven ƒaplar March 14, 2012 Neven ƒaplar () Unication models March 14, 2012 1 / 25 Index of topics Some basic cosmology Unication models Chaplygin gas Generalized

More information

What is the evidence that Big Bang really occurred

What is the evidence that Big Bang really occurred What is the evidence that Big Bang really occurred Hubble expansion of galaxies Microwave Background Abundance of light elements but perhaps most fundamentally... Darkness of the night sky!! The very darkness

More information

Eternal Inflation Theory, the Multiverse, and Cosmology. Inflation and inflationary cosmology have become a big part of the popular

Eternal Inflation Theory, the Multiverse, and Cosmology. Inflation and inflationary cosmology have become a big part of the popular Scientific Paper I wrote this paper about inflation theory for Astronomy 317: Our Universe, the Final Frontier (Galaxies and Cosmology). I researched a cosmological model and presented the evidence that

More information

Cosmology. What is Cosmology?

Cosmology. What is Cosmology? Cosmology What is Cosmology? The study of the structure and evolution of the entire universe The idea is to form picture of the entire Universe: origin, size, and future We will make assumptions that what

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

Cosmology. Assumptions in cosmology Olber s paradox Cosmology à la Newton Cosmology à la Einstein Cosmological constant Evolution of the Universe

Cosmology. Assumptions in cosmology Olber s paradox Cosmology à la Newton Cosmology à la Einstein Cosmological constant Evolution of the Universe Cosmology Assumptions in cosmology Olber s paradox Cosmology à la Newton Cosmology à la Einstein Cosmological constant Evolution of the Universe Assumptions in Cosmology Copernican principle: We do not

More information

PAPER 73 PHYSICAL COSMOLOGY

PAPER 73 PHYSICAL COSMOLOGY MATHEMATICAL TRIPOS Part III Wednesday 4 June 2008 1.30 to 4.30 PAPER 73 PHYSICAL COSMOLOGY Attempt no more than THREE questions. There are FOUR questions in total. The questions carry equal weight. STATIONERY

More information

Outline. Covers chapter 2 + half of chapter 3 in Ryden

Outline. Covers chapter 2 + half of chapter 3 in Ryden Outline Covers chapter + half of chapter 3 in Ryden The Cosmological Principle I The cosmological principle The Cosmological Principle II Voids typically 70 Mpc across The Perfect Cosmological Principle

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 Contents of the Universe (or/ what do we mean by dark matter and dark energy?)

The Contents of the Universe (or/ what do we mean by dark matter and dark energy?) The Contents of the Universe (or/ what do we mean by dark matter and dark energy?) Unseen Influences Dark Matter: An undetected form of mass that emits little or no light but whose existence we infer from

More information

Relativity and Black Holes

Relativity and Black Holes Relativity and Black Holes Post-MS Evolution of Very High Mass (>15 M Θ ) Stars similar to high mass except more rapid lives end in Type II supernova explosions main difference: mass of iron core at end

More information

Cosmology. An Analogy 11/28/2010. Cosmology Study of the origin, evolution and future of the Universe

Cosmology. An Analogy 11/28/2010. Cosmology Study of the origin, evolution and future of the Universe Cosmology Cosmology Study of the origin, evolution and future of the Universe Obler s Paradox If the Universe is infinite why is the sky dark at night? Newtonian Universe The Universe is infinite and unchanging

More information

The Big Bang Theory was first proposed in the late 1920 s. This singularity was incredibly dense and hot.

The Big Bang Theory was first proposed in the late 1920 s. This singularity was incredibly dense and hot. The Big Bang Theory was first proposed in the late 1920 s. It states that there was an infinitely small, infinitely dense point that contained everything that is the universe. This singularity was incredibly

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

Lecture 37 Cosmology [not on exam] January 16b, 2014

Lecture 37 Cosmology [not on exam] January 16b, 2014 1 Lecture 37 Cosmology [not on exam] January 16b, 2014 2 Structure of the Universe Does clustering of galaxies go on forever? Looked at very narrow regions of space to far distances. On large scales the

More information

Abstracts of Powerpoint Talks - newmanlib.ibri.org - The Cosmos. Robert C. Newman

Abstracts of Powerpoint Talks - newmanlib.ibri.org - The Cosmos. Robert C. Newman The Cosmos Robert C. Newman The Cosmos Carl Sagan said: "The cosmos is all that is, or ever was, or ever will be." If Christianity is true, Sagan is mistaken. But we can perhaps define the cosmos as "All

More information

The Formation of the Solar System

The Formation of the Solar System Earth and the Solar System The Formation of the Solar System Write a number beside each picture to rank each from the oldest (1) to the youngest (4). The universe includes everything that exists: all matter,

More information

Ay1 Lecture 17. The Expanding Universe Introduction to Cosmology

Ay1 Lecture 17. The Expanding Universe Introduction to Cosmology Ay1 Lecture 17 The Expanding Universe Introduction to Cosmology 17.1 The Expanding Universe General Relativity (1915) A fundamental change in viewing the physical space and time, and matter/energy Postulates

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

Homework 6 Name: Due Date: June 9, 2008

Homework 6 Name: Due Date: June 9, 2008 Homework 6 Name: Due Date: June 9, 2008 1. Where in the universe does the general expansion occur? A) everywhere in the universe, including our local space upon Earth, the solar system, our galaxy and

More information

26. Cosmology. Significance of a dark night sky. The Universe Is Expanding

26. Cosmology. Significance of a dark night sky. The Universe Is Expanding 26. Cosmology Significance of a dark night sky The Universe is expanding The Big Bang initiated the expanding Universe Microwave radiation evidence of the Big Bang The Universe was initially hot & opaque

More information

Modern Cosmology Solutions 4: LCDM Universe

Modern Cosmology Solutions 4: LCDM Universe Modern Cosmology Solutions 4: LCDM Universe Max Camenzind October 29, 200. LCDM Models The ansatz solves the Friedmann equation, since ȧ = C cosh() Ωm sinh /3 H 0 () () ȧ 2 = C 2 cosh2 () sinh 2/3 () (

More information

What forms AGN Jets? Magnetic fields are ferociously twisted in the disk.

What forms AGN Jets? Magnetic fields are ferociously twisted in the disk. What forms AGN Jets? Magnetic fields are ferociously twisted in the disk. Charged particles are pulled out of the disk and accelerated like a sling-shot. Particles are bound to the magnetic fields, focussed

More information

Cosmic Confusion. common misconceptions about the big bang, the expansion of the universe and cosmic horizons.

Cosmic Confusion. common misconceptions about the big bang, the expansion of the universe and cosmic horizons. The basics Cosmic Confusion common misconceptions about the big bang, the expansion of the universe and cosmic horizons. What is the expansion of space? Is there an edge to space? What is the universe

More information

Cosmology Distinction Course

Cosmology Distinction Course 2006 HIGHER SCHOOL CERTIFICATE EXAMINATION Cosmology Distinction Course Modules 1, 2 and 3 (including Residential 1) Total marks 60 Section I Page 2 General Instructions Reading time 5 minutes Working

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

Model Universe Including Pressure

Model Universe Including Pressure Model Universe Including Pressure The conservation of mass within the expanding shell was described by R 3 ( t ) ρ ( t ) = ρ 0 We now assume an Universe filled with a fluid (dust) of uniform density ρ,

More information

baryons+dm radiation+neutrinos vacuum curvature

baryons+dm radiation+neutrinos vacuum curvature baryons+dm radiation+neutrinos vacuum curvature DENSITY ISN T DESTINY! The cosmologist T-shirt (if Λ>0): ΩM,0=0.9 ΩΛ,0=1.6 ΩR=0 ΩM,0=2.5 ΩM,0=2.0 ΩΛ,0=0.1 ΩM,0=2.0 TODAY Baryons 10 t0 68% Dark Energy 5%

More information

Doppler Effect. Sound moving TOWARDS. Sound moving AWAY 9/22/2017. Occurs when the source of sound waves moves towards or away

Doppler Effect. Sound moving TOWARDS. Sound moving AWAY 9/22/2017. Occurs when the source of sound waves moves towards or away Burkey- ESS QUIZ Thursday At the instant of the Big Bang, all the matter, energy, time, & space in the Universe was condensed into a single, tiny point. We call this Singularity. Doppler Effect Occurs

More information

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

BLACKHOLE WORMHOLE THEORY

BLACKHOLE WORMHOLE THEORY BLACKHOLE WORMHOLE THEORY By - ASHU PRAKASH Black hole, a name which has infinite knowledge to define, but very difficult to define. What is a black hole? In general, a black hole is a gravitationally

More information

In the expanding Universe, a comoving volume element expands along with the cosmological flow, getting physically larger over time.

In the expanding Universe, a comoving volume element expands along with the cosmological flow, getting physically larger over time. Cosmological models In the expanding Universe, a comoving volume element expands along with the cosmological flow, getting physically larger over time. The expansion is described by the scale factor R(t).

More information

Chapter 18. Cosmology. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Chapter 18. Cosmology. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 18 Cosmology Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Cosmology Cosmology is the study of the structure and evolution of the Universe as a whole

More information

Cosmology & the CMB - Cosmology: Overview - Cosmic Microwave Background - Large Scale Structure (Wed) - CMB Fluctuations (Wed)

Cosmology & the CMB - Cosmology: Overview - Cosmic Microwave Background - Large Scale Structure (Wed) - CMB Fluctuations (Wed) Oct 16, 2017 Cosmology & the CMB - Cosmology: Overview - Cosmic Microwave Background - Large Scale Structure (Wed) - CMB Fluctuations (Wed) Wednesday: HW#5 due History of the universe Discovery of Quasars

More information

Brief Introduction to Cosmology

Brief Introduction to Cosmology Brief Introduction to Cosmology Matias Zaldarriaga Harvard University August 2006 Basic Questions in Cosmology: How does the Universe evolve? What is the universe made off? How is matter distributed? How

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

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

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

Dynamics of the Universe

Dynamics of the Universe Dynamics of the Universe 1 Contents 1 A Brief Summary of Observational Facts 3 2 The Friedmann-Robertson-Walker Universe 3 3 Critical Density 7 4 Dark Matter and Dark Energy 8 5 Early Universe and Critical

More information

Lecture Outlines. Chapter 26. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 26. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 26 Astronomy Today 8th Edition Chaisson/McMillan Chapter 26 Cosmology Units of Chapter 26 26.1 The Universe on the Largest Scales 26.2 The Expanding Universe 26.3 The Fate of the

More information

Lecture 16 : Cosmological Models I

Lecture 16 : Cosmological Models I Lecture 16 : Cosmological Models I Hubble s law and redshift in the new picture Standard cosmological models - 3 cases Hubble time and other terminology The Friedmann equation The Critical Density and

More information

Kinetic Theory of Dark Energy within General Relativity

Kinetic Theory of Dark Energy within General Relativity Kinetic Theory of Dark Energy within General Relativity Author: Nikola Perkovic* percestyler@gmail.com University of Novi Sad, Faculty of Sciences, Institute of Physics and Mathematics Abstract: This paper

More information

Big Bang Theory PowerPoint

Big Bang Theory PowerPoint Big Bang Theory PowerPoint Name: # Period: 1 2 3 4 5 6 Recombination Photon Epoch Big Bang Nucleosynthesis Hadron Epoch Hadron Epoch Quark Epoch The Primordial Era Electroweak Epoch Inflationary Epoch

More information