ASTR 1020 – March 9 Homework 5 due today .

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ASTR 1020 – March 9 Homework 5 due today . Second mid-term exam next Tuesday March 14 Note: I will be out of town on Monday and Tuesday so there will be no last minute help from me. Contact David or your LA or the help center for that. . Website http://casa.colorado.edu/~wcash/APS1020/APS1020.html

A Newtonian Black Hole Energy Falling To Surface Kinetic Energy OR if v=c

Schwarzschild Radius Two errors cancel. This is the radius of the “Event Horizon” The event horizon is a true singularity in space-time. It is a place where time and space cease to exist.

Geometry of Black Hole Can you boost the signal? No, that doesn’t help. Space Curves in on itself There’s no path out!

Curved Space

Rubber Sheet Analogy

Properties - Size The radius of a black hole is 3km per solar mass There is no limit on size or mass. Note: Volume rises as the cube of the mass. Implies the larger the black hole gets, the lower is its density. A sphere of water the size of Saturn’s orbit would be a black hole!

Properties – Escape Velocity No way. Not even light can escape. No signal can escape No particle Nothing

Properties – Orbital Period Material orbiting a black hole will have milli-second periods

Properties - Basic Mass (Schwarzschild Black Hole) Electric Charge (doesn’t happen) Angular Momentum (Kerr Black Hole) No “Surface” Features No Magnetic Fields No Pulsing “No Hair”

Jump on In You won’t make it, but it would be quite a ride!

Properties – Energy Emitted Energy Released from accretion about 0.1mc2

Time Dilation Now it gets weird! Time does not run at the same rate everywhere in the universe. Twins are not always the same age. Clocks run a little bit faster in Colorado than in Washington DC. Folks in DC are actually a little slower than us. About one part in a trillion. That’s a millisecond over a lifetime.

Time Dilation Some event takes dt∞ out in free space. Same event takes place at radius r from center of a black hole. Now view it from free space. Takes dt instead. Longer. It looks like things are moving slower. If you are near the black hole, the rest of the universe appears to be moving faster.

Time Dilation As r approaches Rs dt gets longer and longer. When r reaches the event horizon, time stops. We know how to make a time machine with a forward switch only! Just fly to a black hole and orbit above the surface. But you can fall in really fast as viewed from outside.

A “frozen star” If time stops above the surface, it can’t go in. How does the hole form? Is the material still stuck in temporal limbo just above the surface? What’s inside? If nothing can get out, then how can gravity?

Hawking Radiation The vacuum makes pairs of electrons and positrons that pop into existence and then annihilate without any net effect. Above a black hole, one can get sucked in. The other annihilates above the surface to cause radiation. Since its close to the surface, the light gets redshifted escaping, but it carries energy with it!

Temperature Hawking derived that the temperature of a black hole is thermal. Energy for the radiation comes from the mass of the hole. The black hole shrinks with time. That’s a really long time unless the black hole is tiny. A 1kg black hole would last only 10-16s.

Artist’s impression of Cyg X-1 (NASA) 6M0 BH orbiting an O9 star. 2000pc away in Cygnus

Active Galactic Nuclei Some Galaxies have Giant Black Holes in the middle, spewing relativistic jets into intergalactic space