The Brightness Discrepancy and Magnetic Fields

This chapter explores how the brightness of an object is affected by mass inflow and luminosity, and how a strong magnetic field in neutron stars can influence particle movement. It also discusses the limitations of using eddyton luminosity as an indicator of an object's maximum luminosity, and criticizes a misleading headline about defying the laws of physics.

Transcript

Play full episode

The AI-powered Podcast Player

Save insights by tapping your headphones, chat with episodes, discover the best highlights - and more!

Get the app