We used to think black holes were immune to being stretched by static fields like light or gravity—their Love numbers were always zero. But now we've found a crack in that armor: fermionic fields (the stuff of matter) can leave a mark, with non-zero Love numbers for a spinning Kerr black hole, and we've even got an exact formula. Oddly, the dissipative part vanishes for static disturbances, so there's no superradiance. This splits the boson and fermion realms, pointing to a breaking of hidden symmetries.
Black holes are regions of such intense spacetime curvature that not even light can escape. For a long time, they were thought to be utterly unyielding: neither light waves nor gravitational disturbances leave a dent on them. They're like the still surface of a dark lake, remaining unmoved no matter how long you shine a flashlight on it. But new research has shown: fields made of matter particles, such as electrons or neutrinos, make the black hole bend — just like a thrown stone sends ripples across the water. This is the first time an external influence breaks the rigidity of a black hole, and it points to a profound difference between force-carrier fields and particle fields. For non-rotating holes, these "stone" deformations don't fade: energy doesn't flow into the hole, it merely leaves an imprint. This contradicts the hidden symmetries that previously explained why black holes were impervious to ordinary fields. Fermions see gravity differently — and render it vulnerable.
🎯 The name 'Love numbers' comes from the mathematician's surname, not the English word love — it has nothing to do with feelings.