Cosmology. We can simulate how a nearly smooth distribution of dark matter turns into our lumpy, grainy Universe with its hierarchy of structures -

Slides:



Advertisements
Similar presentations
Cosmology GREAT WEB RESOURCE: Contains a cosmological calculator
Advertisements

Formation of Stars and Galaxies.
EXTREME ENERGY COSMIC RAYS AND THE UNIVERSE General scope: a new universe Cosmic rays: facts and puzzles.
Chapter 28 Cosmology The Creation and Fate of the Universe.
Dark Matter, Dark Energy, and the Fate of the Universe.
Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance.
BIG BANG. EVIDENCE FOR BIG BANG Hot Big Bang Model: The universe began expanding a finite time ago from a very dense, very hot initial state. Dense Dense.
Dark Energy Observations of distant supernovae and fluctuations in the cosmic microwave background indicate that the expansion of the universe is accelerating.
Cosmological Structure Formation A Short Course
PRESENTATION TOPIC  DARK MATTER &DARK ENERGY.  We know about only normal matter which is only 5% of the composition of universe and the rest is  DARK.
Cosmology Equipped with his five senses, man explores the universe around him, and calls the adventure "science". -- Edwin Powell Hubble.
Prof. Eric Gawiser Galaxy Formation Seminar 2: Cosmological Structure Formation as Initial Conditions for Galaxy Formation.
Probing The Dark Universe Josh Frieman Fermilab & The University of Chicago Link to Learn, May, 2011.
Cosmology Physics CSG Day at Southampton University 5/6/7 13.7Gyr ABB Steve King.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 14; March
Inflation, Expansion, Acceleration Two observed properties of the Universe, homogeneity and isotropy, constitute the Cosmological Principle Manifest in.
The Dawn of Creation and the Beauty of the Universe Wichita State University April 6, 2010 Steven Beckwith University of California.
Scales in Space and Time in the Cosmos By Dr. Harold Williams of Montgomery College Planetarium
Chapter 30 Section 4 Handout
Cosmic Microwave Background (CMB) Peter Holrick and Roman Werpachowski.
1 Misao Sasaki. 2 Message of this lecture Bing Bang Universe Bing Bang Universe ・・・ confirmed ・・・ probably correct ・・・ in progress Inflationary Universe.
The Evolution of the Universe Nicola Loaring. The Big Bang According to scientists the Universe began ~15 billion years ago in a hot Big Bang. At creation.
1 Galaxies The Andromeda Galaxy - nearest galaxy similar to our own. Only 2 million light years away! Galaxies are clouds of millions to hundreds of billions.
Birth of a Theory Chapter 30.4.
Lecture 5: Matter Dominated Universe: CMB Anisotropies and Large Scale Structure Today, matter is assembled into structures: filaments, clusters, galaxies,
The Universe - 2. Inflation When the strong force began separating from the electroweak force at the end of the GUT era, theorists hypothize that.
MAPping the Universe ►Introduction: the birth of a new cosmology ►The cosmic microwave background ►Measuring the CMB ►Results from WMAP ►The future of.
Our Evolving Universe1 Vital Statistics of the Universe Today… l l Observational evidence for the Big Bang l l Vital statistics of the Universe   Hubble’s.
the National Radio Astronomy Observatory – Socorro, NM
The Cosmic Web The Large Scale Structure of the Universe Szydagis University of Oregon 1 / 17.
Announcements The final exam will be at Noon on Monday, December 13 in Van Allen Hall LR1. Practice questions for unit #5 are available on the class web.
Copyright © 2010 Pearson Education, Inc. Chapter 17 Cosmology Lecture Outline.
Composition Until 30 years ago, we thought all matter was “baryonic” matter (protons, neutrons, electrons). Now: 4.6% is baryonic matter 95% is non-baryonic.
Fate of the Universe 1)Fate of the Universe 2)Shape of the Universe 3)Large Scale Structure November 25, 2002 Final Exam will be held in Ruby Diamond Auditorium.
The Big Bang Theory Earth and Space Ms. Lizette Gutierrez Austin High School.
Cosmology and Dark Matter III: The Formation of Galaxies Jerry Sellwood.
Copyright © 2010 Pearson Education, Inc. Chapter 16 Galaxies and Dark Matter Lecture Outline.
Cosmology (Chapter 14) NASA. Student Learning Objectives Describe the Big Bang theory Analyze possible fates of our universe.
Lec2 Mapping Structure (Frieman)
Chapter 16-17: Cosmology  Hubble’s law Expansion of Universe 1  Galaxy spectra Optical spectra of remote galaxies show redshift (galaxies appear to move.
Announcements Final exam is Monday, May 9, at 7:30 am. –Students with last names A-K go to 225 CB. –Students with last names L-Z go to 300 CB. –All students.
Salient Features of the Universe Homogeneity and isotropy for 6000 Mpc > x > 100 Mpc Universe expanding uniformly ordinary matter is more abundant than.
Homework for today was WORKBOOK EXERCISE: “Expansion of the Universe” (pg in workbook)
The Planck Satellite Matthew Trimble 10/1/12. Useful Physics Observing at a redshift = looking at light from a very distant object that was emitted a.
Birth of a Theory Chapter The Universe & Beyond -Cosmology – study of origin, structure, & future of the universe. Why? -to study how the universe.
Probing Dark Energy with Cosmological Observations Fan, Zuhui ( 范祖辉 ) Dept. of Astronomy Peking University.
Study of Proto-clusters by Cosmological Simulation Tamon SUWA, Asao HABE (Hokkaido Univ.) Kohji YOSHIKAWA (Tokyo Univ.)
The Mass of the Galaxy Can be determined using Kepler’s 3 rd Law –Solar System: the orbital velocities of planets determined by mass of Sun –Galaxy: orbital.
Dark Energy By Chris Malafis & Amit Sheth. Discovery Two competing groups from different observatories were trying to prove the deceleration of the expansion.
Lecture 23: The Acceleration of the Universe Astronomy 1143 – Spring 2014.
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.
Seeing the Invisible: Observing the Dark Side of the Universe Sarah Bridle University College London.
The Dark Side of the Universe
Harrison B. Prosper Florida State University YSP
Chapter 30 Section 4 Big Bang Theory.
The Big Bang The Big Bang
Announcements Final exam is Monday, May 9, at 7:30 am.
CMBR Kinematic Dipole Anisotropy (~300 km/s velocity toward Leo); map of the temperature fluctuation relative to the MEAN (black body with T=2.728 Kelvin)
dark matter and the Fate of the Universe
Olber’s Paradox The universe is expanding! Hubbles Law.
Lecture 20-21: The Formation of Structure---Galaxies, Clusters, Voids
Cosmology The study of the structure and evolution of the Universe as a whole. Seeks to answer questions such as: How big is the Universe? What shape is.
Cosmological Expansion and Dark Energy
Graduate Course: Cosmology
Lecture 5: Matter Dominated Universe
The Big Bang The Big Bang
COSMOLOGY Prospects in Theoretical Physics Institute for Advance Study
Measurements of Cosmological Parameters
Kinematic Dipole Anisotropy from COBE
Presentation transcript:

Cosmology

We can simulate how a nearly smooth distribution of dark matter turns into our lumpy, grainy Universe with its hierarchy of structures - from galaxies to superclusters, great walls and voids New results also indicate that we have dark energy in addition to dark matter, accelerating the expansion of the universe We can “see” some of the dark matter through gravitational lensing

“Acoustic” spectrum of CMB Temperature Power   Angular scale

Large Scale Structure of Universe The Universe is expanding… –Hubble Constant H 0 = 70 km/s/Mpc = 1/14Gyr …initially it was filled with a smooth distribution of dark matter –and a smaller amount of nucleons + electrons –very small initial density fluctuations… …which began to clump to create the seeds of filaments, superclusters, walls, …, galaxies (central black holes?)

Detailed map of dark matter

Geometry of Universe?

What is the Universe made of? Universe is 70% dark energy!