Lecture 10 Cosmological Concepts ASTR 340 Fall 2006 Dennis Papadopoulos.

Slides:



Advertisements
Similar presentations
How was Earth formed?. Big Bang Theory 13.7 billion years ago 13.7 billion years ago Creation of all matter Creation of all matter Hydrogen and Helium.
Advertisements

Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
Objectives: 1. relate the cosmological principle to isotropy and homgeneity of the universe. 2. understand how Hubble’s law is used to map the universe,
When Galaxies Collide. It is not uncommon for galaxies to gravitationally interact with each other, and even collide!
Chapter 28 Cosmology The Creation and Fate of the Universe.
The Fate of the Universe. The cosmological principle The simplest universes is: Homogenous – the same everywhere you go Isotropic – the same in all directions.
Lecture 20 Hubble Time – Scale Factor ASTR 340 Fall 2006 Dennis Papadopoulos.
THEORIES OF THE UNIVERSE. FLAT EARTH THEORY Date: Ancient Times Scientists: Babylonians, Egyptians Theory Description: The world is a flat disk, not.
A Brief Tour of the Universe Don’t Panic The Sun in UV.
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL 10. Inflation.
Expanding Universes Intro Cosmology Short Course Lecture 2 Paul Stankus, ORNL.
22-4 Coulomb’s Law q1 Unit q2 Only apply to point charges r
Our Place in the Universe Drew Smith. Important Principles The Cosmological Principle ▫The universe is isotropic and homogenous (it “looks” the same in.
AST101 Lecture 25 Why is the Night Sky Dark?. Olber’s Paradox Suppose the universe is infinite In whatever direction you look, you will see a star The.
The Uncertain Nature of Gravity An Illustration of Science as a Process of Investigating Nature.
Lecture 23 Models with Cosmological Constant ASTR 340 Fall 2006 Dennis Papadopoulos Chapter 11 Problems Due 12/5/06.
Cosmology Astronomy 315 Professor Lee Carkner Lecture 22 "In the beginning the Universe was created. This has made a lot of people very angry and been.
Lecture 21 Cosmological Models ASTR 340 Fall 2006 Dennis Papadopoulos.
Lecture 36: The Expanding Universe. Review the ‘zoo’ of observed galaxies and the Hubble Sequence the ‘zoo’ of observed galaxies and the Hubble Sequence.
Cosmology Physics466 Olbers Paradox Cosmological principle Expansion of the Universe Big Bang Theory Steady State Model Dark Matter Dark Energy Structure.
ASTR 1200 Announcements Website Homework not yet assigned Lecture Notes going up on the website.
Scientific Theory and Scientific Law
Scientific Theory and Scientific Law
New Core Curriculum week 4, class-2 Foundations of Scientific Process The Birth of the Universe.
Chapter 26: Cosmology How big is the universe? How long has it been around and how long will it last?
Natural Science 120 Prof. Andrew Reynolds CC219. Where are we in the universe?
Theory on the Formation of the Universe
Hubble’s Law Our goals for learning What is Hubble’s Law?
Exploring the Early Universe Chapter Twenty-Nine.
Standard Cosmology.
THE BIG BANG THEORY BY: JASMIN ELICEC S. DELEON. WHAT IS ABOUT THE BIG BANG THEORY The big bang theory is the prevailing cosmological model for the universe.
Ways of Knowing Philosophy of Thought
Expansion of the Universe Natural consequence of the basic field equations of the General Theory of Relativity (GTR) When GTR was first developed in the.
Astrophysics Cosmology - the study of the nature of the universe.
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL 3. Cosmological concepts and Olbers’ paradox.
Electricity and Magnetism Explore the second of the four fundamental forces in nature –Gravity –Electricity and Magnetism –Weak Nuclear Force –Strong Force.
Introduction to the Big Bang Theory
Kinematics and Dynamics Part 2 By: Nichole Raught.
The Tully-Fisher Relation A relation between the rotation speed of a spiral galaxy and its luminosity The more mass a galaxy has  the brighter it is 
10B The Big Bang Where do we come from, where are we going?
Origins Lecture 15; May Previously on Origins Time of history/humans vs. time of “god” –What was there before time? –Does this make sense? The.
Astronomy 1020 Stellar Astronomy Spring_2015 Day-2.
The Life of the Universe From Beginning to End.
Chapter 17 The Beginning of Time. Running the Expansion Backward Temperature of the Universe from the Big Bang to the present (10 10 years ~ 3 x
Large Scale Structure in the Universe We seem to be located at the edge of a Local Supercluster, which contains dozens of clusters and groups over a 40.
What forms the “texture” of the universe? Figure from book.
Our Place in the Universe. 1.1 Our Modern View of the Universe What is our place in the universe? How did we come to be? How can we know what the universe.
Life of a Star HOW DO STARS FORM?. Video Clip 2B7F65270DFF} “A Big.
The Meaning of Einstein’s Equation*
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
Cosmology (Chapter 14) NASA. Student Learning Objectives Describe the Big Bang theory Analyze possible fates of our universe.
The Uncertain Nature of Gravity An Illustration of Science as a Process of Investigating Nature  Using observed motions of objects to infer physics.
Dec 5, 2003Astronomy 100 Fall 2003 Last Homework is due next Friday– 11:50 am Honor credit– need to have those papers soon! THE FINAL IS DECEMBER 15 th.
The Expanding Universe
Lecture 38 – Cosmology II How do we describe (and understand) the expansion of the universe, what is happening now, what happened in the remote past, and.
Universe Tenth Edition Chapter 26 Exploring the Early Universe Roger Freedman Robert Geller William Kaufmann III.
The Shape and Fate of the Universe Assumptions in cosmology Olber’s paradox Expansion of the Universe Curvature of the Universe Fate of the Universe.
The Fate of the Universe. The fate depends on the rate of expansion and the density Density greater than critical value – gravity will halt expansion.
Chapter 20 Cosmology. Hubble Ultra Deep Field Galaxies and Cosmology A galaxy’s age, its distance, and the age of the universe are all closely related.
Discovering the Universe Eighth Edition Discovering the Universe Eighth Edition Neil F. Comins William J. Kaufmann III CHAPTER 18 Cosmology Cosmology.
The Science of Creation
Monday, November 12, 2007 Vilenkin Chs: 1-3.
How was Earth formed?.
Cosmology I Definition of Cosmology: The scientific study of the universe as a whole; how long ago it came into being, the nature of that beginning, the.
Cosmology.
Hypotheses, Models, Theories, and Laws
Did someone monkey with the laws of nature ? Unit 1.1
ASTR 1020 General Astronomy: Stars and Galaxies
A galaxy like the Milky Way contains about 10 billion stars.
Cosmology.
Presentation transcript:

Lecture 10 Cosmological Concepts ASTR 340 Fall 2006 Dennis Papadopoulos

The Universe The Physical Universe –Material objects, energy, space, time, forces Are space and time physical ? What is space, what time? Space is what keeps everything from happening at the same location Time is what prevents everything from happening at once Any physical model should include and explain space and time along with every other physical phenomenon. We cannot invoke a preexisting space and time into which we construct the universe. We cannot ask “what happened before the universe existed” or “what is outside the universe”. Space and time are not properties distinct from the universe. Time did not exist before the universe and space does not exist outside it. The universe is not expanding into space or spacetime.

Scientific Cosmology What is the universe now? How did it reach this state? If we trace the evolution of the universe backward in time we can ask whether or not there was a t=0 point. If there was we must arrive at the question of initial conditions, how things were at the earliest moment we can consider. Cosmology aims at describing these initial conditions and describing how it evolved from them Initial conditions must simple (Occam’s razor); e.g. big bang -> a certain amount of energy and matter, certain physical laws and certain fundamental constants. The complexity we observe existed as a potentiality and developed naturally in the subsequent evolution

Fundamental constants of nature G, c, h, e, m e, m p Values of fundamental constants and basic laws of physics determine what is possible in the universe If any of these changed even slightly the universe would be different than the one we observe e.g. if nuclear reactions were not possible at the densities and temperatures prevailing at the cores of gravitationally bound gaseous nebulae would they be stars? Life?

The Cosmological Principle Universe -> sum of all particles and energy, physical laws and spacetime Humans do not occupy a privileged position in universe Copernican principle ->Earth and solar system do not occupy special place in universe –Does not claim that there is no center –Is there a center somewhere? –Humans as observers Cosmological principle ->

Cosmological Principle (cont)

Isotropy and Homogeneity Homogeneous -> we see no difference when we change position; there is no preferred position in the universe (translational invariance) Isotropic -> no difference when we look at a different direction Examples: Surface of uniform cylinder is homogeneous but not isotropic- what about the surface of a sphere – or chessboard ? Cosmological Principle (CP)-> universe is homogeneous and isotropic (at a given cosmological time)

CP Cosmological principle means that physical laws are assumed to be the same everywhere, too The cosmological principle of isotropy and homogeneity, like other scientific hypotheses, is testable by confrontation with data. So far, observations support this hypothesis

Tests Galaxies arranged in superclusters that appear as long sheets surrounded by voids

Cosmological Principle Tested

The Perfect Cosmological Principle

The role of the observer Anthropic principle – weak and strong –We don’t know why the constants have these values or if it is possible to have other values but out of all possible universes ours is special because we exist Weak Anthropic Principle (WAP): The conditions we observe in the universe (constants, laws, etc) must be compatible with our existence.

Weak Anthropic Principle (WAP)

Against WAP

Other Anthropic Principles Non-Defendable

Cosmological Principles