LECTURE 8 GENERAL THEORY OF RELATIVITY PHYS 420-SPRING 2006 Dennis Papadopoulos.

Slides:



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

Mr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path.
Chapter 18: Relativity and Black Holes
15.1Tenets of General Relativity 15.2Tests of General Relativity 15.3Gravitational Waves 15.4Black Holes General Relativity CHAPTER 15 General Relativity.
Special and General Relativity
Black Holes. Outline Escape velocity Definition of a black hole Sizes of black holes Effects on space and time Tidal forces Making black holes Evaporation.
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.
1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If.
Review for Test #3 April 16 Topics: Measuring the Stars The Interstellar medium Stellar Evolution and Stellar Death Gamma Ray Bursts Neutron stars, pulsars.
Spacetime: just when you thought it was it throws you a.
Review for Test #3 Sunday 3-5 PM Topics: The Sun Stars (including our Sun) The Interstellar medium Stellar Evolution and Stellar Death for Low mass, medium.
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.
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.
Entanglement of cats |   =  |  +  |  Teleportation: making an exact replica of an arbitrary quantum state (while destroying the original...)
Gravitation Applications Lecturer: Professor Stephen T. Thornton
Chapter 13: Neutron Stars and Black Holes Einstein’s theories of Relativity Albert Einstein (Al) is best known for his two theories of relativity Special.
GRAVITY.
13.3 Black Holes: Gravity’s Ultimate Victory Our Goals for Learning What is a black hole? What would it be like to visit a black hole? Do black holes really.
Special Relativity Speed of light is constant Time dilation Simultaneity Length Contraction Spacetime diagrams.
Stationary Elevator with gravity: Ball is accelerated down.
© 2010 Pearson Education, Inc. Chapter S3 Spacetime and Gravity.
General Relativity.
GR Part 1: The Equivalence Principle is in Unit B: Dynamics “distinguish between reference systems (inertial and non-inertial) with respect to real and.
Chapter 26 Relativity. General Physics Relativity II Sections 5–7.
The Theory of Relativity. What is it? Why do we need it? In science, when a good theory becomes inadequate to describe certain situations, it is replaced.
Lecture 4: General Relativity. Einstein’s Progress in General Relativity Einstein knew Special Relativity could only treat situations where gravity was.
Einstein’s postulates 1.The laws of nature are the same for everyone. 2. The speed of light in a vacuum is constant for all observers.
Gravity, Energy, and Light Einstein and Newton 1.
General Relativity Principle of equivalence: There is no experiment that will discern the difference between the effect of gravity and the effect of.
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.
Relatively Einstein 2005 has been chosen as the World Year of Physics to celebrate the 100th anniversary of Einstein’s Miraculous Year. In this presentation,
Fundamental Principles of General Relativity  general principle: laws of physics must be the same for all observers (accelerated or not)  general covariance:
Black Holes Formation Spacetime Curved spacetime Event horizon Seeing black holes Demo: 1L Gravity Well - Black Hole.
Extragalactic Astronomy & Cosmology Lecture GR Jane Turner Joint Center for Astrophysics UMBC & NASA/GSFC 2003 Spring [4246] Physics 316.
Principle of Equivalence: Einstein 1907 Box stationary in gravity field Box falling freely Box accelerates in empty space Box moves through space at constant.
Space Warps. Light is believed to travel the shortest distance between two points But…… the path of light is curved in the presence of a gravitational.
Astronomy 1143 – Spring 2014 Lecture 19: General Relativity.
Physics 55 Monday, December 5, Course evaluations. 2.General relativity with applications to black holes, dark matter, and cosmology. 3.Hubble’s.
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
Unit 13 Relativity.
It was discovered in the early 1990’s that the pulse period of a millisecond pulsar 500 parsecs from earth varies in a regular way.
General Theory of Relativity (Part 2). STOR vs GTOR Recall Special Theory looked at only inertial frames. General theory looks at accelerated frames of.
Gravity, Energy, and Light Einstein and Newton 1.
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.
Phy107 Fall Exam Hour Exam 2: Wednesday, October 25th In-class, covering waves, electromagnetism, and relativity Twenty multiple-choice questions.
ASTR 113 – 003 Spring 2006 Lecture 08 March 22, 2006 Review (Ch4-5): the Foundation Galaxy (Ch 25-27) Cosmology (Ch28-29) Introduction To Modern Astronomy.
Testing General Relativity Hyperspace, Wormholes, and Warp Drives.
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.
Einstein’s Second Revolution. Movement on the surface of the Earth is limited to two dimensions: forward-backward and left-right (or N-S and E-W) However,
Black Holes. Escape Velocity The minimum velocity needed to leave the vicinity of a body without ever being pulled back by the body’s gravity is the escape.
The quest for Gravitation Waves By Benjamin Thayer.
Black Holes and Gravity 1)Type II Supernova 2)Neutron Stars 3)Black Holes 4)More Gravity April 7, 2003
Astronomy 1020 Stellar Astronomy Spring_2016 Day-34.
Black Holes A stellar mass black hole accreting material from a companion star 1.
General Relativity.
Chapter S3 Spacetime and Gravity
A neutron star over the Sandias?
Einstein’s postulates
Relativity H7: General relativity.
Special Relativity Speed of light is constant Time dilation
CHAPTER 15 General Relativity
David Berman Queen Mary College University of London
Special Relativity Speed of light is constant Time dilation
Intro to General Relativity
General relativity Special relativity applies only to observers moving with constant velocity. Can we generalize relativity to accelerated observers.
A theory of gravity, much more general than Newton’s theory.
Special Relativity Speed of light is constant Time dilation
Presentation transcript:

LECTURE 8 GENERAL THEORY OF RELATIVITY PHYS 420-SPRING 2006 Dennis Papadopoulos

General Relativity I The need for a more general theory of relativity… Einstein’s tower experiment The equivalence principle

O: RECAP OF SPECIAL RELATIVITY Einstein’s postulates –Laws of physics look the same in any inertial frame of reference. –The speed of light is the same in any inertial frame of reference Strange consequences –Time dilation and length contraction –Relativity of simultaneity and ordering of events –Equivalence and conversion of mass and energy Why have we been so carefully avoiding gravity until now?

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

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.

Floating Astronauts

ARTIFICIAL GRAVITY

WHAT ABOUT LIGHT

The Eddington Test 1919 – the first “accessible” total Solar eclipse since Einstein postulated SEP Arthur Eddington –Famous British Astronomer –Lead expedition to South America to observe eclipse –Was looking for effects of gravitational light bending by searching for shifts in positions of stars just next to the Sun.

GEN RELAT PREDICTION: Light bends when it passes by massive objects. The more the mass the larger it bends. Observation: During solar eclipse stars along the same line of sight with the Sun are seen on a shifted position. GR gives accurate prediction. SR half of the observed shift. Newton no shift

Galaxies between the earth and a quasar can produce multiple images. From bending one can estimate the mass of galaxy

“The Einstein Cross”

This picture, released to commemorate Hubble's sixth anniversary, shows several blue, loop-shaped objects that are actually multiple images of the same galaxy. The duplicate images were produced by a cosmic lens in space: the massive cluster of yellow elliptical and spiral galaxies near the photograph's center. This cosmic lens, called a gravitational lens, is created by the cluster's tremendous gravitational field, which bends light from a distant object and magnifies, brightens, and distorts it. How distorted the image becomes and how many copies are made depends on the alignment between the foreground cluster and the more distant galaxy.

THE BENDING OF LIGHT (GRAVITATIONAL LENSING)

GRAVITATIONAL TIME DILATION Recap of waves: Waves characterized by –Wavelength ( ) = distance between crests –Frequency (f ) = number of crests passing a given point per second Speed of a crest; c= Energy of a wave is proportional to frequency f  E=hf.

EINSTEIN’S TOWER Another thought experiment… suppose that light is not affected by gravity. Consider a tower on Earth –Shine a light ray from bottom to top –When light gets to top, turn its energy into mass. –Then drop mass to bottom of tower. –Then turn it back into energy

If we can do this, we can get make energy from nothing… –Original energy in light beam = E start –Thus, mass created at top is m=E/c 2 –Then drop mass… at bottom of tower it has picked up speed (and energy) due to the effects of gravitational field (E grav =mgh) –When we turn it back into energy, we have E end =E start +E grav –But, we started off with E start – we have made energy! We’re rich!

Clearly, our assumption is wrong… –light must be affected by gravity. –But gravity does not appear in Maxwell’s equations –Thus, Maxwell’s equations are not valid in the reference frame of Earth’s surface. –The Earth’s surface must not be an inertial frame of reference.

Fig. 3-25, p. 95

Fig. 3-26, p. 96

GRAVITATIONAL REDSHIFT

Prediction: time should run ``slower'' near a large mass. This effect is called time dilation. For example, if someone on a massive object (call her person A) sends a light signal to someone far away from any gravity source (call him person B) every second according to her clock on the massive object, person B will receive the signals in time intervals further apart than one second. According to person B, the clock on the massive object is running slow. Observation: a) Clocks on planes high above the ground run faster than those on the ground. The effect is small since the Earth's mass is small, so atomic clocks must be used to detect the difference. b) The Global Positioning Satellite (GPS) system must compensate for General Relativity effects or the positions it gives for locations would be significantly off. Clock A Clock B

How to live for a 1000 years! Observer on Earth would see astronauts clock running very slowly when close to black hole – astronaut would age very slowly.

Gravitational time dilation has practical importance! Global Positioning System (GPS) –System of satellites that emit timing signals –Detector on Earth receives signals –Can figure out position on Earth’s surface by measuring time delay between signals from different satellite. –Need to measuring timing signal from satellite very well! If GR effects were not included, GPS positions would drift from true position by kilometers per day!

ACCELERATION AND WARPING OF SPACE/TIME Measure radius and circumference with no spin you find their ratio equal circumf/radius=  Do it again when the wheel is spinning. Radius the same but circumference longer Ratio> 6.28

ACCELERATION AND TIME Slim and Jim compare their watches while Jim crawls slowly along the radius. Slim’s clock runs slower since he was always moving faster than Jim. Example of warped time, rate of passage differs from location to location

THE GENERAL THEORY OF RELATIVITY Within a free-falling frame, the Special Theory of Relativity applies. Free-falling particles/observers move on geodesics through curved space-time The distribution of matter and energy determines how space-time is curved. “Space-time curvature tells matter/energy how to move. Matter/energy tells space-time how to curve.”

Notes: –The Einstein curvature tensor “G” is mathematical object describing curvature of 4-D space-time. –The Stress-Energy tensor “T” is mathematical object describing distribution of mass/energy. –Newton’s constant of gravitation “G” and the speed of light “c” appear as fundamental constants in this equation. –This is actually a horrendous set of 10 coupled non-linear partial differential equations!! For weak gravitational fields, this gives Newton’s law of gravitation.

CURVED SPACE-TIME Einstein pondered several things… –Success of Special Relativity showed that space & time were closely linked –The “tower thought experiment” suggested that free-fall observers are (locally) free of effects of gravity –He wanted to say that gravity was an illusion caused by the fact that we live in an accelerating frame… –… but there is no single accelerating frame that works! Somehow, you need to stick together frames of reference that are accelerating in different directions

Einstein’s suggestion –4-dimensional space-time is curved –Free-falling objects move on “geodesics” (generalizations of straight lines) through curved space- time. –Matter and energy causes space-time to bend. What is a geodesic? –Shortest path between two points on a surface –E.g. path flown by aircraft –Geodesics that start parallel can converge or diverge (or even cross).

EUCLIDEAN AND NON EUCLIDEAN GEOMETRIES Ratio of circumference to radius depends on curvature 22 < 2  > 2 

GEOMETRY REPLACES FORCES The presence of mass distorts space/time, bodies move in geodesics in space/time – no forces Mechanism that transmits force is warping of space by mass No two dimensional membrane being pulled down.

GEODESICS Short paths (in space time) between two points. Flat space – straight line Sphere great circle. Paths of least resistance.

Earth does not orbit Sun because the Sun forces it. It simply follows the geodesic (shortest path in four dimensional space time) Shadow of plane flying on a straight line over hilly terrain. Low masses Einst and Nt same.

Curved space around the Earth looks something like this… From web site of UCSD

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.

Direct detection of gravitational waves… How do you search for gravitational waves? Look for tidal forces as gravitational wave passes Pioneered by Joseph Weber (UMd Professor) –Estimated wave frequency (10000Hz) –Looked for “ringing” in a metal bar caused by passage of gravitational wave. –Weber claimed detection of waves in early 1970s –Never verified – but Weber held out to the end…

Fig. 2-7, p. 57

Fig. 2-8, p. 57

Fig. 2-9, p. 57

The binary pulsar (PSR ) Russell Hulse & Joseph Taylor (1974) –Discovered remarkable double star system –Nobel prize in 1993 From Nobel Prize website

Fig. 2-11, p. 58

Fig. 2-10a, p. 58

Modern experiments : LIGO Laser Interferometer Gravitational Wave Observatory Two L-shaped 4km components –Hanford, Washington –Livington, Louisiana

Will become operational very soon! Can detect gravitational waves with frequencies of about Hz. VERY sensitive… need to account for –Earthquakes and Geological movement –Traffic and people! What will it see? –Stellar mass black holes spiraling together –Neutron stars spiraling together

LISA Laser Interferometer Space Antenna Space-based version of LIGO Sensitive to lower-frequency waves ( – 0.1Hz) Can see –Normal binary stars in the Galaxy –Stars spiraling into large black holes in the nearby Universe. –Massive black holes spiraling together anywhere in the universe!

Fig. 2-10b, p. 58

Fig. 3-27, p. 97

Fig. 3-28, p. 98