Contact:  andrea.maselli[AT]gssi.itLocation:  L'Aquila, Italy
We are looking for a 2-year postdoc in the GW group of the Gran Sasso Science Institute
to work on source modelling of black hole binaries.
Candidates with experience in relativistic perturbation theory and semi-analytical approaches to describe astrophysical compact sources and their gravitational wave emission are strongly encouraged to apply.
We expect the candidate to work within an international network which includes different nodes in Europe, as the University of Pisa and the University of Nottingham.
Applications need to be submitted online:
(ref. Position 1.4)
Application deadline is on July 6.