19-23 June 2017
Dept. of Physics & Astronomy and the CoSMS Institute, University of North Carolina at Chapel Hill
US/Eastern timezone

Progress at second order

21 Jun 2017, 09:00
50m
Sitterson 011 (UNC)

Sitterson 011

UNC

Speaker

Adam Pound (University of Southampton)

Description

I discuss the status of second-order self-force formulations and computations, which will be necessary for accurate models of EMRIs. In the first part of the talk, I describe recent progress on the foundations of the theory. A principal feature of the second-order field equations is that the retarded field does not have a distributionally well-defined source, instead having a free boundary value in a region around the small object. This challenge has historically been addressed using a puncture scheme. However, it can also be eliminated entirely with a judicious choice of gauge, which may radically simplify future numerical work. In the second part of the talk, I describe ongoing work to numerically implement a second-order, two-timescale puncture scheme for quasicircular orbits in Schwarzschild spacetime. This will lead into the talk by Wardell.

Primary author

Adam Pound (University of Southampton)

Co-authors

Barry Wardell (University College Dublin) Jeremy Miller (University of Southampton) Prof. Leor Barack (University of Southampton) Niels Warburton (University College Dublin)

Presentation Materials

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