Key: Thorne = the required textbook, Kip Thornes
Black holes and time warps; Seeds = Mike Seeds's Foundations of astronomy;
Hawking = Stephen Hawking's A brief history of time; Silk = Joe Silk's
The Big Bang.
à = night-time class meeting, Hoyt Auditorium, 7-11 PM.
N = on-line examination, 12-6 PM.
|
Date |
Subject |
Required/recommended reading |
---|---|---|---|
Preliminaries, including our first meetings with the odd properties of black holes, which we will spend the rest of the semester explaining. |
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1 |
|
How big is that? An introduction to the sizes, masses, distances, ages and speeds commonly encountered in astronomy. |
Seeds, chapter 1 |
2 |
3 |
Prologue in outer space: what it’s like to be in the neighborhood of some typical black holes. |
Thorne, pp. 23-59. |
3 |
8 |
||
Relativity: a non-mathematical introduction to the special and general theories of relativity. | |||
|
|
Einstein’s theories: special relativity; the warping of space and time; the Lorentz transformation and velocity-addition formulas; general relativity; experimental verifications of relativity. | Thorne, pp. 59-120. Seeds, chapter 5. |
5 |
|
||
6 |
|
||
7 |
2 |
||
8 |
2 |
Gravitational radiation, general relativity’s analogue of light. | Thorne, pp. 357-396.. |
9 |
2 |
General relativity predicts the existence of black holes | Thorne, pp. 121-139. Hawking, chapter 6 |
à | 30 September 2009 | Review session for Exam #1, with Jae Song presiding. | |
N |
1 October 2009 |
Exam #1, covering all subjects discussed to date. | |
Quantum mechanics: important microscopic properties of the very dense progenitors of black holes and their relatives, the degenerate stars. | |||
10 |
|
Material strength and the uncertainty principle: can quantum mechanics keep black holes from forming? | Thorne, pp. 140-163. Hawking, pp. 57-85. |
11 |
8 |
Degenerate stars. White dwarf stars and the Chandrasekhar maximum mass; neutron stars and the Oppenheimer maximum mass; supernovae; the inevitable formation of black holes. | Thorne, pp. 164-257. Seeds, pp. 265-268, 285-295. |
12 |
1 |
||
Observations of black holes. They really do exist in nature, and here's how we know. | |||
13 |
1 |
Properties of real black holes. | Thorne, pp. 258-299. |
14 |
2 |
Energetics of black holes, and the discovery of quasars. | Thorne, pp. 300-321. |
15 |
2 |
Black holes unveiled. Astronomical objects thought, or known, to involve black holes: X-ray binary stars, active galaxy nuclei, the center of the Milky Way, and gamma-ray bursters. | Thorne, pp. 322-356. Seeds, pp. 295-303, 356-376; Silk, pp. 259-284. |
16 |
2 |
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17 |
2 |
||
18 |
3 |
||
à | 4 November 2009 | Review session for Exam #2, with Brian DiCesare presiding. | |
N |
5 November 2009 |
Exam #2, emphasizing subjects introduced since Exam #1. | |
The outsides and insides of horizons: black holes and their relation to thermodynamics, Hawking radiation, and odd relativistic objects that can be considered to be combinations of black holes. | |||
19 |
10 November 2009 |
Black holes aren’t quite black: quantum fluctuations near the horizon, and black-hole evaporation. | Thorne, pp. 412-448. Hawking, pp. 105-120. |
20 |
12 November 2009 |
Inside black holes: physics beyond the black-hole horizon; or is it metaphysics? | Thorne, pp. 397-411, 449-482. |
21 |
17 November 2009 |
Wormholes and space travel: How (potentially) to use black holes to travel very long distances in a short time. | Thorne, pp. 483-522. |
à | 17 November 2009 | AST 102 Film Festival: Star Trek (2009) and Contact (1997). | |
à | 18 November 2009 | AST 102 Film Festival: Contact (1997) and Star Trek (2009). | |
22 | 19 November 2009 | Wormhole time machines: Time travel may indeed be possible, if only in a limited sense, using wormholes. | Thorne, pp. 483-522. |
Cosmology: the Big Bang and the large-scale structure of the Universe, which turns out to be very black-hole-like. | |||
23 |
24 November 2009 |
The homogeneous, isotropic, expanding Universe: According to GR it begins and/or ends in a singularity. | Hawking, pp. 1-36; Silk, pp. 105-158. |
24 |
1 December 2009 |
The Big Bang, its observation, and Big Bang cosmology: The present expansion and large-scale structure of the universe, dark matter, and the history and fate of matter-dominated universes. | Seeds, pp. 378-400; Hawking, pp. 37-84 and 121-150; Silk, pp. 29-104 and 149-186. |
25 |
3 December 2009 |
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26 | 8 December 2009 | The new flat universe: Acceleration of the expansion, dark energy, and other potential implications of the latest generation of cosmic microwave background observations. | |
à | 9 December 2009 | Review session for Exam #3, with Brian DiCesare presiding. | |
N |
10 December 2009 |
Exam #3, emphasizing subjects introduced since Exam #2. |