Harvard University Logo HARVARD.EDU
Skip to main content

BHI Colloquium

Monday, March 10, 2025
11:00 AM

Send Me News from BHI

Send Me News from BHI

BHI Colloquium

Leonhard Kehrberger

Description

Why null infinity is not smooth, and how to measure it

Abstract: Be it numerical, formal, or mathematical, the typical setup for the evolution of spacetimes describing, for instance, the merger of two black holes is to make an ad hoc assumption on the initial data to have compactly supported gravitational radiation content.
This ensures that the spacetime has a smooth null infinity (it “peels”), but essentially pretends the spacetime has been stationary at some time “before” the initial data.

My talk will be about what happens when one does not ignore the past dynamics of the system: I will present mathematical results that convert scattering data assumptions in the infinite past into precise predictions on the asymptotics towards spacelike and future null infinity, showing in particular that null infinity is not smooth.
Furthermore, I will explain how this failure of null infinity to be smooth affects the asymptotics of gravitational radiation at late times (“tails”), predicting decay up to three powers slower than the usual “Price’s law” decay.

 

When

Monday, March 10, 2025 11:00 AM

Where

BHI Publication

Expanding Sgr A* dynamical imaging capabilities with an African extension to the Event Horizon Telescope

April 1, 2023
Kantzas, D.; Markoff, S.; Lucchini, M.; Ceccobello, C.; Chatterjee, K.
Astrophysical jets are relativistic outflows that remain collimated for remarkably many orders of magnitude. Despite decades of research, the…
Read The BHI Publication