17–20 Aug 2016
Nordita, Stockholm
Europe/Stockholm timezone

Effective black hole degrees of freedom at low frequencies

17 Aug 2016, 14:30
30m
Wallenbergsalen (Nordita, Stockholm)

Wallenbergsalen

Nordita, Stockholm

Speaker

Barak Kol (Hebrew University)

Description

A black hole moving through a slowly varying background can be replaced by a point particle together with some effective interactions with the background by using the (non-quantum) effective field theory method. Some of the coefficients in the so-defined effective black hole (BH) action are known, and in particular 4d Schwarzschild black holes are known to have no induced gravitational polarization at the linearized response level. The BH effective action includes also certain well-defined degrees of freedom whose physical interpretation will be discussed.

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