Spacetime: just when you thought it was it throws you a.

Slides:



Advertisements
Similar presentations
Lecture 15 General Theory of Relativity ASTR 340 Fall 2006 Dennis Papadopoulos.
Advertisements

LIGO-G v1 Black holes, Einstein, and gravitational waves Peter R. Saulson Syracuse University.
Relativity Theories. The Principle of Relativity Although motion often appears relative, it’s logical to identify a “background” reference frame from.
PHY306 1 Relativity Principle of relativity  not a new idea! Basic concepts of special relativity  …an idea whose time had come… Basic concepts of general.
15.1Tenets of General Relativity 15.2Tests of General Relativity 15.3Gravitational Waves 15.4Black Holes General Relativity CHAPTER 15 General Relativity.
Extragalactic Astronomy & Cosmology First-Half Review [4246] Physics 316.
Developing a Theory of Gravity Does the Sun go around the Earth or Earth around Sun? Why does this happen? Plato } Artistotle } Philosophy Ptolemy }& Models.
How do we transform between accelerated frames? Consider Newton’s first and second laws: m i is the measure of the inertia of an object – its resistance.
LIGO-G W Measuring Ripples in the Geometry of Space Fred Raab LIGO Hanford Observatory.
This set of slides This set of slides continues the late-in-life evolution and death of massive stars, stars > 8 solar masses. It starts with Special and.
Friday: review (HERE - A110) Monday: Final Exam 2:30 – 4:20 pm A110 (here again) Closed book, may bring 2 double- sided sheets of hand-written notes, and.
General Relativity I The need for a more general theory of relativity… Einstein’s tower experiment The strong equivalence principle.
Lecture 16 GR – Curved Spaces ASTR 340 Fall 2006 Dennis Papadopoulos.
J. Goodman – May 2003 Quarknet Symposium May 2003 Neutrinos, Dark Matter and the Cosmological Constant The Dark Side of the Universe Jordan Goodman University.
Entanglement of cats |   =  |  +  |  Teleportation: making an exact replica of an arbitrary quantum state (while destroying the original...)
LECTURE 8 GENERAL THEORY OF RELATIVITY PHYS 420-SPRING 2006 Dennis Papadopoulos.
LIGO-G W Measuring Ripples in the Geometry of Space Fred Raab LIGO Hanford Observatory.
PH 103 Dr. Cecilia Vogel Lecture 13 Review Outline  Einstein’s postulates  inertial frames indistinguishable  constancy of speed of light  principle.
GRAVITY.
Hubble Diagram: Distribution of Galaxies. Hubble’s Law: v = H o d Velocity increases with distance.
Friday, October 24 Next planetarium show: Thurs, Nov. 6
5 Gravitation. The Milky Way galaxy and the black hole.
1 CDT403 Research Methods in Natural Sciences and Engineering Theory of Science GOLEM ANALYSIS OF SCIENTIFIC CONFIRMATION: THEORY OF RELATIVITY Gordana.
Objectives Solve orbital motion problems. Relate weightlessness to objects in free fall. Describe gravitational fields. Compare views on gravitation.
SPS8.c Relate falling objects to gravitational force.
Gravity: Newton to Einstein
Wormholes and space warps Topics Ripples in space Wormholes Time warps Space warps Motivation A few spacetime oddities. 1.
LIGO-G Black holes, Einstein, and space-time ripples Peter R. Saulson Syracuse University.
According to Isaac Newton, gravity is a force which acts everywhere in the Universe, attracting massive bodies – including planets, stars, galaxies – towards.
NS 1300 Dr. Hoge.  Can we slow light down?  Can we make things invisible?  Is it possible to travel faster than the speed of light?  Is faster than.
Physics Mrs. Coyle -Gravitational Field -Satellites -Einstein’s View of Gravity.
1 Discussion on Chapters Einstein’s Universe Gravity at work and play.
General Relativity (1915) A theory of gravity, much more general than Newton’s theory. Newtonian gravity is a “special case”; applies when gravity is very.
E = mc 2 Yeah So What?. Outstanding Science Issues in 1900.
 Newtonian relativity  Michelson-Morley Experiment  Einstein ’ s principle of relativity  Special relativity  Lorentz transformation  Relativistic.
Fundamental Principles of General Relativity  general principle: laws of physics must be the same for all observers (accelerated or not)  general covariance:
Extragalactic Astronomy & Cosmology Lecture GR Jane Turner Joint Center for Astrophysics UMBC & NASA/GSFC 2003 Spring [4246] Physics 316.
Spacetime diagrams A useful way of making spacetime maps Similar to normal map (north-south & east-west)......but with one axis being time instead of a.
18/04/2004New Windows on the Universe Jan Kuijpers Part 1: Gravitation & relativityPart 1: Gravitation & relativity J.A. Peacock, Cosmological Physics,
Principle of Equivalence: Einstein 1907 Box stationary in gravity field Box falling freely Box accelerates in empty space Box moves through space at constant.
Relativity Jennifer Keehn. “I want to know how God created this world. I am not interested in this or that phenomena, in the spectrum of this or that.
Black holes, Einstein, and space-time ripples
Unit 1 Lesson 4 Gravity and Motion
Astronomy 1143 – Spring 2014 Lecture 19: General Relativity.
Dark Matter Inquiring Minds Want to Know Prof. David Toback Texas A&M University.
General Relativity. Einstein’s Theory of General Relativity -deals with accelerated frames of reference and provides a new theory of gravity. -(Special.
The Expanding Universe
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.
Testing General Relativity Hyperspace, Wormholes, and Warp Drives.
Life on Earth Without the Theories of Relativity How would our lives be different on Earth if we did not have any knowledge of the theory of relativity?
A recap of the main points so far… Observers moving uniformly with respect to each other do not agree on time intervals or distance intervals do not agree.
The quest for Gravitation Waves By Benjamin Thayer.
Astronomy 1020 Stellar Astronomy Spring_2016 Day-34.
PHY 151: Lecture Newton’s Law of Universal Gravitation 11.2 Structural Models 11.3 Kepler’s Laws 11.4 Energy Considerations in Planetary and Satellite.
Black Hole. Special Relativity Einstein’s special theory of relativity has two parts. –All objects moving at constant velocity have the same laws of physics.
Gravity and Motion. Kepler’s Theory of Planetary Motion 1. Paths are ellipses and sun at the focus 2. Planets move faster when closer 3. Relationship.
Astrophysics and Cosmology
A neutron star over the Sandias?
Einstein’s postulates
2017 Nobel Prize in Physics: Discovery of Gravitational Waves
Physics for Scientists and Engineers, 3rd edition
CHAPTER 15 General Relativity
Intro to General Relativity
Gravity and Motion.
A theory of gravity, much more general than Newton’s theory.
Newton, Einstein, and Gravity
General Relativity: Part II
The First Ever Detection of Gravity Waves
Principle of Equivalence: Einstein 1907
Gravity Chapter 12.2.
Presentation transcript:

Spacetime: just when you thought it was it throws you a

On one hand mass seems to encourage acceleration. On the other hand, it resists it. Another conundrum Einstein just could not ignore.

PRINCIPLE OF EQUIVALENCE No experiment in an isolated space can distinguish between a gravitational field and an equivalent uniform acceleration.

No experiment would help you distinguish between being weightless far out in space and being in free-fall in a gravitational field.

GR POSTULATES PRINCIPLE OF EQUIVALENCE: IN THE VICINITY OF ANY POINT, A GRAVITATTIONAL FIELD IS EQUIVALENT TO AN ACCELERATED FRAME OF REFERENCE IN THE ABSENCE OF GRAVITTATIONAL EFFECTS THE LAWS OF NATURE HAVE THE SAME FORM IN ANY FRAME OF REFERENCE, WHETHER ACCELERATED OR NOT

A new way to look at why the Earth rotates around the Sun.

Two people are walking in parallel lines at the equator. They continue along lines of constant longitude, until, much to their surprise, they meet. They conclude they must have been attracted by a force. You see that they were actually walking on a curved surface.

Lensing

Gravitational Lensing

Why do we think there is dark matter? Isn’t obvious that most of the matter in the Universe is in Stars?Isn’t obvious that most of the matter in the Universe is in Stars? Spiral Galaxy

Clusters produce distinctive tangential patterns

Distortions of our view of the sky

Gravitational Lensing

Measuring the energy in the Universe We can measure the mass of clusters of galaxies with gravitational lensingWe can measure the mass of clusters of galaxies with gravitational lensing These measurements give  mass ~0.3These measurements give  mass ~0.3 We also know (from the primordial deuterium abundance) that only a small fraction is nucleons  nucleons < ~0.04We also know (from the primordial deuterium abundance) that only a small fraction is nucleons  nucleons < ~0.04 Gravitational lensing

Dark Matter

Another Consequence: GRAVITATIONAL WAVES Particular kind of phenomena (e.g. orbiting stars) produce ripples in the space-time curvature… Ripples travel at speed of light through space These are called gravitational waves.

Early instrumentation to detect gravity waves,, “Weber bars”, were pioneered by UMD professor, Joseph Weber! Go Terps!

LIGO - Laser Interferometer Gravitational Wave Observatory Like Michelson Morley, but each arm is kilometers long!