Lecture 16: Spinning Black Holes and the No-Hair Theorem

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Lecture 16: Spinning Black Holes and the No-Hair Theorem. S. Chandrasekhar – “Shattering Experience”. Roy Kerr – Discoverer of Black-Hole Spin. Spinning Stars and Gyroscopic Effect. Spin Gives Preferred Axis for Jets. Disk-to-Hole Transfer of Angular Momentum. - PowerPoint PPT Presentation

Transcript of Lecture 16: Spinning Black Holes and the No-Hair Theorem

Lecture 16:Spinning Black Holes

and the No-Hair Theorem

S. Chandrasekhar – “Shattering Experience”

Roy Kerr – Discoverer of Black-Hole Spin

Spinning Stars and Gyroscopic Effect

Spin Gives Preferred Axis for Jets

Disk-to-Hole Transfer of Angular Momentum

Trajectories Near Spinning Black Hole

Horizon Shape of Spinning Black Hole

Equatorial Bulges of Planets

Spinning Black-Hole Accretion is Efficient

Implosion of Real vs. Idealized Stars

Stars Have Magnetic Fields

A Black Hole Radiating a Magnetic Field

A Black Hole Radiating a “Mountain”

Black Holes Have No Hair

Validating the Oppenheimer-Snyder Study