Inverse problems for Lorentzian manifolds and non-linear hyperbolic equations

TL;DR

This paper addresses two inverse problems on Lorentzian manifolds: reconstructing spacetime regions from light observations and developing a non-linear hyperbolic equation method to determine spacetime structures from wave data.

Contribution

It introduces a novel approach utilizing non-linearity to solve inverse problems for non-linear hyperbolic equations, advancing beyond linear problem solutions.

Findings

Reconstructed the conformal type of unknown spacetime regions from light observation sets.

Developed a new method leveraging non-linearity to solve inverse problems for semilinear wave equations.

Determined the topological, differentiable, and conformal structures of 4D spacetimes from wave data.

Abstract

We study two inverse problems on a globally hyperbolic Lorentzian manifold $(M,g)$. The problems are: 1. Passive observations in spacetime: Consider observations in a neighborhood $V\subset M$ of a time-like geodesic $\mu$. Under natural causality conditions, we reconstruct the conformal type of the unknown open, relatively compact set $W\subset M$, when we are given $V$, the conformal class of $g|_V$, and the light observations sets $P_V(q)$ corresponding to all source points $q$ in $W$. The light observation set $P_V(q)$ is the intersection of $V$ and the light-cone emanating from the point $q$, i.e., the points in the set $V$ where light from a point source at $q$ is observed. 2. Active measurements in spacetime: We develop a new method for inverse problems for non-linear hyperbolic equations that utilizes the non-linearity as a tool. This enables us to solve inverse problems for non-linear equations for which the corresponding problems for linear equations are still unsolved. To illustrate this method, we solve an inverse problem for semilinear wave equations with quadratic non-linearities. We assume that we are given the neighborhood $V$ of the time-like geodesic $\mu$ and the source-to-solution operator that maps the source supported on $V$ to the restriction of the solution of the wave equation in $V$. When $M$ is 4-dimensional, we show that these data determine the topological, differentiable, and conformal structures of the spacetime in the maximal set where waves can propagate from $\mu$ and return back to $\mu$.