ELFT HÍRADÓ

[Biro Tamas <biro.tamas AT wigner.mta.hu>]

Tisztelt Kollégák,

a következő Wigner kollokviumot

2016. október 25.-én, kedden tartjuk 14:00 órai kezdettel.

Előadó:  Prof. Lars Andersson

Cím:   Geometry of Black Hole Spacetimes

Absztrakt:

Einstein's theory of general relativity admits solutions which describe 
black holes, regions of spacetime where the gravitational field is 
strong enough that light cannot escape. Observations indicate that black 
holes are common in the universe, and interactions of black holes 
provide an important source for gravitational radiation. The Kerr family 
of rotating black holes provides the only viable model these phenomena, 
and it is therefore of fundamental importance to prove that the Kerr 
solution to the Einstein equations is unique and stable. In this talk I 
will discuss some of the remarkable geometric properties of the Kerr 
black holes, which are expected to be important in proving the 
uniqueness and stability of the Kerr black hole.

Helyszín:  KFKI campus 1.épület tanácsterem.


Minden érdeklősőt szerettel várunk.

 Biró Tamás és Rácz István
 (szervezők)
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