Massive Waves Gravitationally Bound to Static Bodies
Erwin Schrödinger International Institute for Mathematics and Physics (ESI) via YouTube
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Overview
Syllabus
Introduction
Why the Clan Gordon equation
Decay rate
Grapevine
If this are true
Where does the mass go
asymptotically curved space times
nontrapping conditions
precise statement
faster decay
standing wave solutions
Constructing elements
Theory
Bump functions
Discrete spectrum
Taught by
Erwin Schrödinger International Institute for Mathematics and Physics (ESI)