Relativity and Astrophysics
Syllabus, Handouts and PowerPoints for this unit: Syllabus | Handouts | Lectures
Labs for this unit: Stellar Evolution Flowchart .:. Hubble Lab
What you need to learn:
Chapter 26 - Special Relativity:
26A. Understand what ether is, and why the Michelson Morley experiment failed to find it. Understand Einstein's gedanken experiment, and the postulates of special relativity.
NoteGuide-01-01SpecialRelativity.docx
The Postulates of Special Relativity:
26B. Understand how the postulates lead to time dilation
NoteGuide-01-01SpecialRelativity.docx
Rationale for Time Dilation:
Deriving the Time Dilation Equation:
26C. Solve problems with Time Dilation, Length Contraction, and Mass Dilation
26H. Solve problems with relativistic Kinetic Energy.
NoteGuide-02-01SpecialRelativityII.docx
Relativistic Kinetic Energy:
26I. Solve relativistic addition of velocity problems.
NoteGuide-02-01SpecialRelativityII.docx
Relativistic Addition of Velocities:
26J. Use the energy-momentum formula.
Yeah - I don't have any video of this - read the book section 26-9.
General Relativity - Chapter 33
33A. Understand the Principle of Equivalence
NoteGuide-03-01GeneralRelativity.docx
Principle of Equivalence:
33B. Apply the curvature of space to observations
NoteGuide-03-01GeneralRelativity.docx
The Curvature of Space:
33C. Solve problems with black holes and Schwarzschild radius.
NoteGuide-03-01GeneralRelativity.docx
Black Holes:
33D. Understand gravitational time dilation using the approximate frequency shift equation.
NoteGuide-03-01GeneralRelativity.docx
Gravitational Frequency and Wavelength Shift:
33E. Solve problems with gravitational time dilation using the Schwarzschild radius.
NoteGuide-03-01GeneralRelativity.docx
Gravitational Time Dilation:
Chapter 33 - Astrophysics:
A. Use and understand the Wien displacement formula.
B. Calculate the total power output of a star.
C. Calculate the apparent brightness of a star.
D. Calculate the apparent magnitude of a star.
E. Calculate the absolute magnitude of a star.
F. Understand what an H-R diagram is, and what the main sequence is, and some common stars found off the main sequence.
G. Understand how to relate recession velocity to redshift using the approximate formula.
H. Use the Hubble law, and know what it means in terms of an expanding universe.