Uploaded January 2025 | Updated September 2026, 2 weeks ago
Development of the equations for the relativistic Doppler Effect and aberration of light (not to be confused with chromatic aberration on your graphics settings menu). Quick comment: I use k nought in the audio to refer to the wavevector magnitude in the R reference frame. What I actually mean is that k is the wavevector magnitude in R while k' is the magnitude in R'.
Questions/requests? Let me know in the comments!
Pre-reqs: previous videos in this playlist - youtube.com/playlist?list=PLdgVBOaXkb9CkdpdSWT9oPDSvQ8BjjNTq
Lecture Notes: drive.google.com/file/d/1KGSktebaRZtIMy2LpJAczMHYXMCefAI7/view?usp=drive_link
Special thanks to my Patrons:
Matthew
Patapom
Eugene Bulkin
Andy Johnston
Lina Stritt
Patrick Gibson
Joseph Dubeau
Development of the equations for the relativistic Doppler Effect and aberration of light (not to be confused with chromatic aberration on your graphics settings menu). Quick comment: I use k nought in the audio to refer to the wavevector magnitude in the R reference frame. What I actually mean is that k is the wavevector magnitude in R while k' is the magnitude in R'.
Questions/requests? Let me know in the comments!
Pre-reqs: previous videos in this playlist - youtube.com/playlist?list=PLdgVBOaXkb9CkdpdSWT9oPDSvQ8BjjNTq
Lecture Notes: drive.google.com/file/d/1KGSktebaRZtIMy2LpJAczMHYXMCefAI7/view?usp=drive_link
Special thanks to my Patrons:
Matthew
Patapom
Eugene Bulkin
Andy Johnston
Lina Stritt
Patrick Gibson
Joseph Dubeau










