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PHY483/1483F
Pre-class reading and digitised lecture notes

This work is licensed under a Creative
Commons Attribution-NonCommercial-ShareAlike 2.0 Canada License.
(CC) awpeet 2006
| Wk |
Date |
Reading (C=Carroll) |
Lecture notes / topic |
| 1 |
w14sep |
[none] |
Introduction
to the course and the prof. |
|
f16sep |
my OSC lecture |
Review
of Lorentz transformations, rapidity;
xμ and the Minkowski metric
ημν
|
| 2 |
w21sep |
[C online pp1-12]
| Invariant interval, causality; vectors |
| |
f23sep |
[C online pp8-19]
| Tensors;
vectors and dual vectors; Coordinate bases;
Kronecker δμν
|
| 3 |
w28sep |
[C online pp14-21 and
OSC lecture pp12-14] |
Manipulating tensors;
4-momentum pμ ;
Levi-Civita εμναβ ,
EM field Fμν;
Constant acceleration & Twin Paradox |
|
f30sep |
Carroll book sec. 3.1 |
Equivalence
principle; gravity as geometry; Tensors in curved space
|
| 4 |
w05oct |
3.2-3.3 |
Parallel transport and
covariant derivative ∇μ ;
Christoffel connection
Γμνλ |
|
f07oct |
3.3-3.4 |
Parallel transport and the geodesic
equation; affine parameter; an explicit example
|
| 5 |
w12oct |
2.3, 3.8 & Appendix B |
Vector field
commutators and Lie derivatives; role
of symmetries and Killing vectors; examples |
|
f14oct* |
Appendix J |
Orthormal frames and non-coordinate
bases eA; spin connection one-form
ωAB
|
| 6 |
w19oct |
3.6-3.7 |
Riemann
two-form RAB ,
Riemann curvature
Rλσμν
|
|
f21oct |
3.9 |
Geodesic deviation;
Riemann curvature example from 2004 exam |
| 7 |
w26oct |
3.10 |
Ricci
tensor Rμν and scalar R ;
how symmetries reduce complexity |
|
f28oct |
1.9-1.10,3.5 |
Energy-momentum
tensor Tμν
, e.g. perfect fluid; covariant conservation |
| 8 |
w02nov |
4.1,4.2 |
Newtonian
limit; Why a tensor theory of gravity? |
|
f04nov* |
4.3 |
Action
for gravity and obtaining Einstein's equations |
| 9 |
w09nov |
4.4 |
Einstein field equations |
|
f11nov |
4.4,4.5 |
Finding
energy-momentum tensor in general; e.g.s
spin-0 & spin-1 fields, cosmological constant, particle |
| 10 |
w16nov |
4.6, Appendix F |
Bending of
geodesics by gravity: Raychaudhuri equation;
energy conditions |
|
f18nov |
5.1,5.2,5.8 |
Birkhoffs's theorem;
hydrostatic equilibrium and
Tolman-Oppenheimer-Volkoff (TOV) equations |
| 11 |
w23nov |
5.1-5.3,5.8 |
Schwarzschild black hole solution;
Event Horizon and
Singularity; matching to TOV |
|
f25nov |
5.4-5.5 |
Singularities and Geodesics
in Schwarzschild |
| 12 |
w30nov |
5.6-5.7, Appendix G |
Precession of perihelion of
Mercury; Causal structure of Schwarzschild |
|
f02dec* |
6 |
Causal structure of
black holes; Surface gravity;
charged/rotating black holes |
| 13 |
w07dec |
[none] |
Hawking
radiation, black hole entropy, extra dimensions
and string theory
|
|
f09dec |
all lecture notes & HW solutions |
Solving exam-type problems |
* = homework assignment due by 1:10pm
Advice
To view PDF files, you should have Adobe
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Here is a table of the Greek alphabet
for your reference.
Please make sure you read the assigned sections of Carroll (the
course textbook) before turning up to each class. Doing the
assigned reading will make each lecture more comprehensible and much
more valuable for you. Assigned reading will be posted no less than
two days before a lecture.
I number important equations in my lecture notes, to help you synchronize
with auxiliary notes you may take during class.
Digitised lecture notes will be uplinked soon after each
lecture. Since important in-lecture annotations to prepared notes
will be made, uplinking of course lecture notes prior to lecture would
be inconsistent with causality and hence will not be done. I also have
other sound educational reasons for loading lecture notes
after the fact - not to mention the common phenomenon of
last-minute titivations. Please also remember that I am providing
lecture notes as a service, primarily to be welcoming to
students with disabilities. So please don't argue with me about
my post-lecture uploading policy... Thanks.
Important deadlines and dates can be found on the Arts
and Science Calendar Sessional Dates page .

This work is licensed under a Creative
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