Paolo Pani

In general relativity, a black hole has long been regarded as a perfect mirror: no matter what fields fall onto it, it does not deform. The tidal Love numbers, which measure how a body deforms under an external tidal field, turned out to be zero for scalar, electromagnetic, and gravitational perturbations.

Einstein's general relativity describes gravity as the curvature of spacetime — much like a heavy weight pressing down on a stretched elastic sheet. Black holes are regions where this curvature reaches extreme values, the deepest "funnels" in the fabric of the universe.

When two neutron stars circle each other, they don't remain rigid spheres. The partner's gravity stretches each star, creating tidal bulges — much like the Moon raises ocean tides on Earth. But unlike water, here it's superdense matter that deforms: a teaspoon of this stuff weighs billions of tons.