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Determination of space-time structures from gravitational perturbations
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Determination of space-time structures from gravitational perturbations
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We study inverse problems for the Einstein equations with source fields in a general form. Under a microlocal linearization stability condition, we show that by generating small gravitational perturbations and measuring the responses near a freely falling observer, one can uniquely determine the background Lorentzian metric up to isometries in a region where the gravitational perturbations can travel to and return. We apply the result to two concrete examples when the source fields are scalar fields (i.e. Einstein-scalar field equations) and electromagnetic fields (i.e. Einstein-Maxwell equations).
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