Cosmological Expansion and Dark Energy

Slides:



Advertisements
Similar presentations
Cosmology Dr Katy Lancaster.
Advertisements

Pauline Gagnon Physicist and communicator at CERN The dark side of the Universe.
That other pesky 95% Dark Energy and Dark Matter Prof. Lawrence Wiencke Department of Physics Engineering Colorado School of Mines Nov
UNIVERSE CHAPTER BIG BANG The big bang theory is the main cosmological model for the earliest known time of the Universe. It shows us how the universe.
1 Approaching the Present Cosmic Times The Universe for Breakfast - Pancake or Oatmeal??  Which describes our Universe best?  1. Pancake:
Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance.
Cosmology : Cosmic Microwave Background & Large scale structure & Large scale structure Cosmology : Cosmic Microwave Background & Large scale structure.
Dark Matter, Dark Energy, and the Expansion of the Universe By Michael Howard
If the sequence above represents a range of stars that are close to us ( ) and at increasingly far distances, how do we interpret the changing positions.
2011 Nobel Prize in Physics Awarded to Saul Permutter Brian Schmidt Adam Riess "for the discovery of the accelerating expansion of the Universe through.
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.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 17.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 26 Cosmology Cosmology.
The Dawn of Creation and the Beauty of the Universe Wichita State University April 6, 2010 Steven Beckwith University of California.
Progress on Cosmology Sarah Bridle University College London.
Universe: Space-time, Matter, Energy Very little matter-energy is observable Critical matter-energy density balances expansion and gravitational collapse.
Dark Energy Bengt Gustafsson: Current problems in Astrophysics Lecture 3 Ångström Laboratory, Spring 2010.
Life in a Four percent Universe Dr. C.P. Girijavallabhan Professor Emeritus International School of Photonics CUSAT.
Expanding Universe 1)Hubble’s Law 2)Expanding Universe 3)Fate of the Universe November 20, 2002 Final Exam will be held in Ruby Diamond Auditorium NOTE.
Cosmology: The Study of the Universe as a Whole Physics 360 Geol 360 Astronomy John Swez.
Cosmology I & II Fall 2012 Cosmology Cosmology I & II  Cosmology I:  Cosmology II: 
COSMOLOGY SL - summary. STRUCTURES Structure  Solar system  Galaxy  Local group  Cluster  Super-cluster Cosmological principle  Homogeneity – no.
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.
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.
So, how’s it gonna end? The Big Bang started the universe expanding fast, but gravity should have put on the brakes. Expansion should slow down after.
THE UNIVERSE OR DECREASING ACCELERATION IS THE EXPANSION RATE PRESENTED BY: JAKE DOTTS & JESS MYERS.
Hubble’s Observations - Edwin Hubble, in the late 1920's, discovered that all galaxies are moving away from each other as he observed the red shift in.
Cosmology. We can simulate how a nearly smooth distribution of dark matter turns into our lumpy, grainy Universe with its hierarchy of structures -
Big Bang Theory – A History 1927: Belgian priest Georges Lemaître proposes that the universe began with the explosion of a "primeval atom". Einstein develops.
1 Curvature measures Topics The Runaway Universe Review of models Just what were they measuring? What did they expect? What did they find? Motivation Discover.
Prof Martin Hendry University of Glasgow. A long time ago, in a galaxy far, far away…
25-4: Galaxies Use the following PowerPoint to take notes on the final section of the chapter. Upon completion work with your partner to answer the Self.
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.
To do: Run through the ppt on Big Bang and Cosmology (resources.faulkes-telescope.com > GCSE Astronomy > Class Exercises > Cosmology Complete the following.
Cosmology -- the Origin and Structure of the Universe Cosmological Principle – the Universe appears the same from all directions. There is no preferred.
Universe Tenth Edition Chapter 25 Cosmology: The Origin and Evolution of the Universe Roger Freedman Robert Geller William Kaufmann III.
Cosmology -- the Origin and Structure of the Universe Cosmological Principle – the Universe appears the same from all directions. There is no preferred.
Nobel Prize in Physics 2011 Saul Perlmutter Supernova Cosmology Project Berkeley, USA Brian P. Schmidt High-z Supernova Search Team Weston Creek, Australia.
The Beginning of Time Review: evidence for dark matter evidence for dark matter comes from  motions of stars and gas in galaxies  motions of galaxies.
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.
COSMOLOGY The study of the origin, structure, and future of the universe.
Seeing the Invisible: Observing the Dark Side of the Universe Sarah Bridle University College London.
Constraining Dark Energy with Double Source Plane Strong Lenses Thomas Collett With: Matt Auger, Vasily Belokurov, Phil Marshall and Alex Hall ArXiv:
Cosmology -- the Origin and Structure of the Universe
Image of the day Turn in cosmology questions!.
The Origin of the Universe
Chapter 30 Section 4 Big Bang Theory.
Doesn’t that mean we are in the centre of the universe?
Ch. 14 Cosmology (or “The Whole Enchilada”)
Cosmology: SNC 1D.
WHAT KIND OF UNIVERSE DO YOU LIVE IN?
dark matter and the Fate of the Universe
Image of the day.
Expansion of the Universe
Cosmology Chapter 15 Great Idea:
Galaxies and the Universe
Lectures on galaxies and cosmology
A New Vision of the Cosmos
The omega problem There has always been a problem with the expanding universe. Will it go on expanding forever? The answer has depended on the balance.
The Big Bang and the Future of the Universe
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Cosmology: The Origin and Evolution of the Universe
Theories of Universe Formation
The Universe.
FORMATION OF THE UNIVERSE
Galaxies and the Universe
Presentation transcript:

Cosmological Expansion and Dark Energy

Spectroscopy and Redshift Everything known about the universe comes from what we can see. Spectroscopy tells about composition, among other things. The redshift, z, is Redshift tells about relative motion, rotation, etc. It turns out that nearly everything is redshifted.

Hubble Law In 1920s, Edwin Hubble finds that redshift is proportional to distance.

Hubble Law (phys.org)

Cosmological Expansion This redshift is not due to relative motion, but due to the universe itself expanding (cosmological redshift).

Expansion Rate is Increasing 2011 Nobel Prize in Physics awarded to Saul Perlmutter, Brian P. Schmidt, and Adam G. Riess (for their work from 1997) "for the discovery of the accelerating expansion of the Universe through observations of distant supernovae“ (nobelprize.org).

What is causing this? Dark Energy Term coined by Michael Turner in 1998. Doesn’t interact with light (dark) Pushes things apart. Does not clump together like matter (smooth). Very mysterious…How can we understand this?

Dark Energy Survey (DES) Over 120 scientists from 23 institutions in 5+ countries. Started 2013, ends 2018. Uses the Dark Energy Camera (DECam) in Chile. (darkenergysurvey.org)

Dark Energy Survey (DES) Mounted in Victor M. Blanco Telescope Looks at Type 1a Supernovae (cosmic acceleration) Baryon Acoustic Oscillations (cosmic acceleration) Galaxy Clusters (structure and expansion) Gravitational Lensing (dark matter) (darkenergysurvey.org)

The Q Continuum Simulation being performed on the Titan supercomputer at U.S. DOE’s Oak Ridge National Lab. (October 29, 2015) Models large scale structure of Universe. Involves half trillion particles; from 50 My after Big Bang to present. Over 90% of Titan’s Computational power used. (phys.org)

Associated with Dark Energy What is the geometry of the universe? Flat? (Euclidean) Closed? (spherical) Open? (hyperbolic) How did it start? (Did it start?) How will it end? (Will it end?) Big Rip Big Crunch Big Bounce