General Relativity: Part II

Slides:



Advertisements
Similar presentations
Mr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path.
Advertisements

9A Black Holes and Neutron Stars Dead Stars Copyright – A. Hobart.
General Relativity is a surprisingly good fit for grade-9 Astronomy. It explains and gives depth to many standard topics like.... What causes orbits?
15.1Tenets of General Relativity 15.2Tests of General Relativity 15.3Gravitational Waves 15.4Black Holes General Relativity CHAPTER 15 General Relativity.
The Expanding Universe Except for a few nearby galaxies (like Andromeda), all the galaxies are seen to be moving away from us Generally, the recession.
13 Black Holes and Neutron Stars Dead Stars Copyright – A. Hobart.
The Hidden Lives of Galaxies Jim Lochner, USRA & NASA/GSFC.
Black Holes Dennis O’Malley. How is a Black Hole Created? A giant star (more than 25x the size of the sun) runs out of fuel –The outward pressure of the.
Chapter 12 Gravitation. Theories of Gravity Newton’s Einstein’s.
Black Holes By Irina Plaks. What is a black hole? A black hole is a region in spacetime where the gravitational field is so strong that nothing, not even.
Black Holes.
Please pick up problem set #3. Median score = 87. Recitation session: Today, 4:30 – 5:30 pm McPherson (Prof subbing for TA)
Stationary Elevator with gravity: Ball is accelerated down.
Unit 06 “Circular Motion, Gravitation and Black Holes” “Gravitation and Black Holes”
Nebulae A nebula is a cloud of dust, gas and plasma. The material clumps together to form larger masses that eventually are big enough to form a protostar.
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.
Chapter 13 Black Holes. What do you think? Are black holes just holes in space? What is at the surface of a black hole? What power or force enables black.
Remnant of a Type II supernova explosion Iron core collapses until neutrons are squeezed tightly together During the explosion core remains intact, outer.
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.
Bending Time Physics 201 Lecture 11. In relativity, perception is not reality Gravity affects the way we perceive distant events For example, although.
General Relativity and the Expanding Universe Allan Johnston 4/4/06.
Chapter 16 Dark Matter, Dark Energy, and the Fate of the Universe.
Lecture 27: Black Holes. Stellar Corpses: white dwarfs white dwarfs  collapsed cores of low-mass stars  supported by electron degeneracy  white dwarf.
Historical SN and their properties Total energy released ~10 54 erg in a few hours.
Black holes, Einstein, and space-time ripples
Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity.
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
Universe Tenth Edition
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.
A black hole: The ultimate space-time warp Ch. 5.4 A black hole is an accumulation of mass so dense that nothing can escape its gravitational force, not.
Exploring the Universe. Big Bang Theory The big bang theory is how the scientist say the universe began. How the Big Bang Started most people believe.
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.
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.
Prepared a presentation Teacher of English Anisova Julia Vladimirovna.
Neutron Stars & Black Holes (Chapter 11) APOD. Student Learning Objective Indentify properties of Neutron Stars & Black Holes NASA.
Chapter S3 Spacetime and Gravity
Supernovas Neutron Stars and Black Holes
Astrophysics and Cosmology
Einstein’s postulates
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.
Stars change over their life cycles.
Curvature in 2D… Imagine being an ant… living in 2D
Great Ideas in Science: Lecture 8 – Stars & Galaxies
Astronomy.
The Universe.
Relativity H7: General relativity.
The Sun, Formation of Elements, the Big Bang, and Black Holes
Interesting Stuff in Space
ORIGIN OF THE UNIVERSE UNIT 2 Big Bang.
8 Space physics Topic overview
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Galaxies and Stars Galaxies – billions of star groups
Black Holes and Neutron Stars
Earth Science 25.2B : Stellar Evolution
The Universe.
CHAPTER 15 General Relativity
Black Holes.
Exam 3 average: 65%. You will have all of class time on Thursday to do the group review. The response “Exams” will be on Learning Suite by Wed noon. They.
Intro to General Relativity
Chapter 13 Neutron Stars and Black Holes
The Death of a Star.
Key Areas covered Evidence for the expanding Universe
A theory of gravity, much more general than Newton’s theory.
Chapter 30-4 The Big Bang Theory
Dark Matter, Dark Energy, and the Fate of the Universe
What is it and how did it all begin?
The Death of a Star.
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Presentation transcript:

General Relativity: Part II Gravity is Curved Space

1) You walk 10 km south, 10 km west and then 10 km north and you are back where you started. What colour is the bear? a) brown b) black c) white Hint: There is only one place in the world where this would happen.

We live in a 4-dimensional curved space which we cannot see or experience directly. We can get a sense of how it works by using an analogy with fewer dimensions.

Imagine that you are a smart blind ant moving about on the surface of a balloon. Draw the path of the polar explorer from the the riddle on your balloon.  

2) Suppose that there is a light at the North Pole 2) Suppose that there is a light at the North Pole. The light radiates in all directions and follows the straightest lines in this space. What will an ant at the South Pole notice? a)      Nothing. b)      A bright spot. c)      A bright ring.  

The curved arcs that you see in this photograph are coming from a distant light. Between it and the Earth there is a large mass that warps the space, so that light appears to come from many directions.

3) Try to get a planet to orbit for more We can detect how mass distorts the three dimensions of space but we can’t picture it. 3) Try to get a planet to orbit for more than a dozen times on your fabric. How do you do this? 4) How would an ant explain this motion?

When Einstein first calculated the curvature of light he got it wrong by a factor of two. Half the curvature is from the equivalence principle and the second half is from the curvature of space.

Mass curves spacetime into gravitational lenses.

Gravitational lenses are used by astronomers to measure the mass of regular matter and dark matter.

Draw a 15-cm line on your balloon Draw a 15-cm line on your balloon. At right angles to that, draw another 15-cm line. Draw two more of them. What do you get?

Planetary orbits don’t form simple ellipses either Planetary orbits don’t form simple ellipses either. They form patterns like Daisy petals - this is called the precession of the equinoxes. This was a known problem with Newtonian Gravitation that General Relativity was able to solve.

a) Jupiter because it is biggest b) Mercury because it is smallest 5) The planet with the greatest precession will be a)      Jupiter because it is biggest b)      Mercury because it is smallest c)      Mercury because it is closest to the sun d)      Neptune because it is farthest

Suppose, the balloon was expanding. What would the ant notice?

The galaxies are all moving away from us and the more distant ones are moving faster.

There is a simple relationship between velocity and distance There is a simple relationship between velocity and distance. This suggests that everything in the universe was once gathered in one point that exploded around 14 billion years ago – the Big Bang.

6) Gravity should cause this expansion to Recent evidence suggests that it speeding up! The cause of this is not understood, but it has a name - Dark Energy. 6) Gravity should cause this expansion to a) slow down b) speed up c) remain constant. Best-fit Constant velocity

7)As a star’s life ends, it collapses and gets much denser 7)As a star’s life ends, it collapses and gets much denser. What would you see if you got close to dense star whose escape velocity was almost c? a) Light rising and falling b) Faint radio waves c) Faint gamma rays Particles can rise and slow down, but not light. Light gets red-shifted.

8) What happens if the escape velocity is greater than c? a) only gamma rays escape b) only radio waves escape c) nothing escapes d) nothing escapes so it can’t be detected No light can escape. This is called a Black Hole.

You can detect one by the way it warps light.

You can detect black holes that have matter spiraling into them You can detect black holes that have matter spiraling into them. This matter will form hot disks that give off x-rays.

Black Holes often produce jets spewing matter out at speeds close to c Black Holes often produce jets spewing matter out at speeds close to c. Many of these have been found.

Black holes can also be detected by measuring the speeds of orbiting bodies. This data can be used to calculate the mass and density of the central body. M = v2 r /G

What is it like inside a Black Hole What is it like inside a Black Hole? All light and matter will be driven by the extremely curved spacetime into a singularity of infinite density.

Rapidly orbiting massive objects should generate gravitational waves, ripples in the fabric of space. These waves take energy away, so the objects should spiral into the center.

Taylor and Hulse have measured a binary pulsar doing exactly that.

Large detectors are being built around the world to detect gravitational waves directly. This is LIGO.

An even larger gravity detector called LISA, is being built An even larger gravity detector called LISA, is being built. It is made of three satellites in a huge triangle. It may be able to measure the curvature near a Black Hole.