Dark matter and black holes over cosmic time TOMMASO TREU.

Slides:



Advertisements
Similar presentations
The Large Scale Structure of the Universe Clusters of galaxies X-rays from clusters of galaxies Sheets and voids.
Advertisements

Our Galaxy `. Interstellar dust obscures our view at visible wavelengths along lines of sight that lie in the plane of the galactic disk.
The W i d e s p r e a d Influence of Supermassive Black Holes Christopher Onken Herzberg Institute of Astrophysics Christopher Onken Herzberg Institute.
Galaxies The Universe is filled with these star systems which themselves cluster together into larger systems.
Slide 1 Andromeda galaxy M31Milky Way galaxy similar to M31.
Copyright © 2010 Pearson Education, Inc. Chapter 16 Galaxies and Dark Matter.
Chapter 16 Dark Matter And The Fate Of The Universe.
H.-W. Rix, Vatican 2003 Gravitational Lensing as a Tool in Cosmology A Brief History of Lensing 1704 Newton (in Optics): „Do not bodies act upon light.
Astro-2: History of the Universe Lecture 4; April
QUASARS Monsters of the ancient Universe Professor Jill Bechtold Steward Observatory Tucson Amateur Astronomers, Dec. 6, 2002.
Baking a universe Or, how we came looking like this out of the Big Bang.
Galaxy Evolution Astronomy 315 Professor Lee Carkner Lecture 22.
Chapter 23: Our Galaxy Our location in the galaxy Structure of the galaxy Dark matter Spiral arm formation Our own supermassive black hole.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 12; February
Galaxy collisions & galaxy formation Collisions of galaxies Formation of galaxies Dark Matter.
Class 23 : The mass of galaxies and the need for dark matter How do you measure the mass of a galaxy? What is “dark matter” and why do we need it?
ASTR100 (Spring 2008) Introduction to Astronomy The Case for Dark Matter Prof. D.C. Richardson Sections
GALAXY FORMATION AND EVOLUTION - 2. DISCOVER Magazine’s 2007 Scientist of the Year David Charbonneau, of the Harvard-Smithsonian Canter for Astrophysics.
PRESIDENCY UNIVERSITY
Susan CartwrightOur Evolving Universe1 Galaxy evolution n Why do galaxies come in such a wide variety of shapes and sizes? n How are they formed? n How.
Chapter 31 Galaxies & the Universe Review & Recap It does this by precisely measuring the speed of gas and stars around a black hole. This provides clues.
The Milky Way Galaxy.
Virtually all galaxies show a flat rotation curve.
Christopher | Vlad | David | Nino SUPERMASSIVE BLACK HOLES.
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
Astro-2: History of the Universe Lecture 5; April
Overview of Astronomy AST 200. Astronomy Nature designs the Experiment Nature designs the Experiment Tools Tools 1) Imaging 2) Spectroscopy 3) Computational.
Dark Matter begin. Definition Dark Matter is matter that we cannot see. It neither emits nor reflects any light. If we can’t see it, how do we know it.
This Set of Slides This set of material starts “the big(gest) picture”. Cosmology – the study of the structure and evolution of the universe. This set.
Galaxies Read Your Textbook: Foundations of Astronomy
Components of the Milky Way The light from galaxies is centrally concentrated. But is the mass also centrally concentrated? Does Mass follow Light in Galaxies?
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.
Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe
Dark Matter, Dark Energy, How Come Some People Think We Need It and Others Don’t and the Fate of the Universe.
Dark Matter in Galaxies and Clusters AST 112. Matter Galaxies appear to be made up of stars, gas and dust Reasonable to think that’s the end of the story…
GRAVITATIONAL LENSING
Intro to Cosmology! OR What is our Universe?. The Latest High Resolution Image of the Cosmic Microwave Background Radiation Low Energy RegionHigh Energy.
A black hole is a region of space with such a strong gravitational field that not even light can escape.
Chapter 25 Galaxies and Dark Matter Dark Matter in the Universe We use the rotation speeds of galaxies to measure their mass:
North America at night from space. Light can be: broken up into component colors broken up into component colors absorbed absorbed reflected reflected.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 25.
Dark Matter. Zwicky’s Coma In 1933 Fred Zwicky measured the speed of Coma cluster galaxies. –Too fast for the visible stars –Cluster would fly apart Either.
Exploring Dark Matter through Gravitational Lensing Exploring the Dark Universe Indiana University June 2007.
Quasars Chapter 17. Topics Quasars –characteristics –what are they? –what is their energy source? –where are they? –how old are they? –interactions of.
Chapter 16 Dark Matter, Dark Energy, and the Fate of the Universe.
Lecture Outline Chapter 18: Dark Matter, Dark Energy, and the Fate of the Universe © 2015 Pearson Education, Inc.
Gravitational Lensing: How to See the Dark J. E. Bjorkman University of Toledo Department of Physics & Astronomy.
1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped.
© 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
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.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
More to the universe than meets the eye
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.
Norma, scuitum-crux, Sagittarius, Orion, Perseus, cygruus.
Quiz #10 What would really happen to you if you were to fall all the way into the Event Horizon of a black hole? We know the gravity is unbelievably strong.
Copyright © 2010 Pearson Education, Inc. Chapter 16 Galaxies and Dark Matter Lecture Outline.
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.
General Relativity and Grade-9 Astronomy. 0) Gravity causes time to slow down. Everyday Einstein: The GPS and Relativity OAPT Conference May 12 – 14 McMaster.
Chapter 25 Galaxies and Dark Matter. 25.1Dark Matter in the Universe 25.2Galaxy Collisions 25.3Galaxy Formation and Evolution 25.4Black Holes in Galaxies.
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.
Chapter 14: Chapter 14: Black Holes: Matters of Gravity.
Astronomy 1020 Stellar Astronomy Spring_2016 Day-38.
ASTR112 The Galaxy Lecture 5 Prof. John Hearnshaw 8. Galactic rotation 8.3 Rotation from HI and CO clouds 8.4 Best rotation curve from combined data 9.
Dark Matter, Dark Energy
Chapter 16 Active Galaxy.
Announcements Final exam is Monday, May 9, at 7:30 am.
© 2017 Pearson Education, Inc.
The invisibles of the Universe
Astronomy Mr. Thompson THE MILKY WAY Galaxy.
Enormous black holes in galaxies
Presentation transcript:

Dark matter and black holes over cosmic time TOMMASO TREU

Our view of the Universe (2009) Now… wear your dark matter goggles!!

Elliptical Galaxies. Simple? MOVIE

A big dark surprise They contain supermassive black holes at their centers. The mass of the black hole is proportional to that of the stars in the galaxy and that of the dark matter around it! –M BH = 0.2% M * = 0.001% M DM

The local Universe

… are thought to form by mergers of spirals…

Questions and puzzles 1.Do elliptical galaxies live in dark matter halos consistent with those predicted by the model? 2.Why is the mass of the black hole proportional to the mass of the stars and that of dark matter? 3.How do (stars) black holes and dark matter evolve over cosmic time?

Telescopes as time machines

Into the invisible How do we “see” dark matter? –Gravitational lensing How do we “weigh” black holes? –Reverberation mapping

What is Gravitational Lensing? Matter curves space…

What is Gravitational Lensing? …and can create multiple images Image separation is a direct measurement of mass, luminous or dark!

Why is it called Lensing?

A DOUBLE EINSTEIN RING

A DOUBLE EINSTEIN RING: GEOMETRY OBSERVER MAIN LENS (2 billion light yrs) INNER RING (6 billion light yrs) OUTER RING (11 billion light yrs)

How likely? More unlikely than winning two consecutive bets on a single number at roulette!

The most precise mass density profile measurement Dark matter halo! (Atoms)

Really? Is there dark matter?

Cosmic collisions and dark matter

Black holes on a “scale”?

Reverberation Mapping Ring of gas with radius r Gas along line of sight to observer will appear to respond with no delay Gas that is furthest from observer will appear to have response delayed by 2r/c Mean lag time is r/c, I.e radius / speed of light

Example: Arp 151 SDSS

The local Universe

Summary Our standard cosmological model is undergoing rigorous testing –We need to understand how galaxies and black holes form Things that appear to work include: –Galaxies live in dark matter halos. –Dark matter appears to be real although it would be good to know what particle it is made of Things that we do not understand include: –Why are galaxies “isothermal”? –How do black holes know of their host galaxy and viceversa? –The most massive galaxies and their black holes appear to have completed their evolution before the lower mass systems. In the model we naively expect the opposite. Is the model fundamentally wrong or is this because we do not understand the “gastrophysics”?

The end