Download presentation

Presentation is loading. Please wait.

Published bySydney Patterson Modified over 3 years ago

1
**Trip to a Black Hole I by Robert J. Nemiroff Michigan Tech**

Extraordinary Concepts in Physics Lecture 4 Trip to a Black Hole I by Robert J. Nemiroff Michigan Tech

2
**Physics X: About This Course**

Officially "Extraordinary Concepts in Physics" Being taught for credit at Michigan Tech Light on math, heavy on concepts Anyone anywhere is welcome No textbook required Wikipedia, web links, and lectures only Find all the lectures with Google at: "Starship Asterisk" then "Physics X"

3
**Trip to a Black Hole: Overview**

Schwarzschild black hole only It's the easiest It's what I know best Based partly on my paper: "Visual distortions near a neutron star and black hole" American Journal of Physics 1993, 61, 619 And my web page: Virtual Trips to Black Holes and Neutron Stars

4
**Trip to a Black Hole: Key Distances**

r = infinity: space is flat: aN = GM/r2 Near the black hole: a = aN / (1 - rs/r)1/2 r = 3 rs: last stable orbit r = 1.5 rs: photon sphere r = rs: event horizon r = rc: Compton radius r = 0: GR singularity

5
**Trip to a Black Hole: Far Away**

r -> infinity: space is "flat" all (1 - rs/r) terms go to 1. gravity is Newtonian: aN = GM/r2 black holes attract the same as normal matter curved universe NOT flat as r -> infinity can see lensing effects with a telescope orbiting the same as spinning in place

6
**Trip to a Black Hole: Approaching**

black hole appears black excludes evaporation effects blackness everywhere inside photon sphere cannot see to the event horizon outside, average surface brightness unchanged appears fuzzy as star images merge distant universe speeds up appears bluer

8
**Background: Gravitational Lensing**

gravity bends light: "null geodesics"

9
**Gravitational Lensing: Einstein Ring**

Actual Einstein ring: APOD 2008 July 28

10
**Gravitational Lensing: Einstein Ring**

Detailed image of Einstein ring from AJP paper

11
**Trip to a Black Hole: Orbiting Nearby**

12
**Trip to a Black Hole: Orbiting at 10 rs **

Stars CANNOT cross the Einstein ring Einstein ring mapped point behind BH center Einstein ring divides complete image sets Angular speeds diverge at the Einstein ring One can see oneself All stars have two discernible images One outside the ER, one inside Observers also have two images Actually, an infinite number of images exist

13
**Trip to a Black Hole: Orbiting at 10 rs **

Distant stars appear slightly bluer Distant clocks appear to run faster This also occurs for stars that appear next to the black hole Objects ACTUALLY nearer to the black hole Appear redder Clocks appear to run slower

14
**Trip to a Black Hole: Orbiting at the Photon Sphere**

15
**Trip to a Black Hole: Orbiting at the Photon Sphere**

Everything below you is black because those light paths fall into the BH The whole sky appear above you because those light paths escape the BH The Einstein ring appears above the horizon Stars still CANNOT cross the Einstein ring Stars still speed up near the Einstein ring

16
**Trip to a Black Hole: Orbiting at the Photon Sphere**

Other image sets between other Einstein rings "The" Einstein ring actually "First Sky Einstein ring" There are infinitely many Sky Einstein rings Every radius from the BH has its own infinite set of Einstein rings its own redshift (or blueshift)

17
**Gravitational Lensing: Einstein Ring**

Einstein rings near a black hole

Similar presentations

© 2017 SlidePlayer.com Inc.

All rights reserved.

Ads by Google