PIPages
Labs

Peter Hintz

Pennsylvania State University, PA·Mathematics & Statistics

Black holes are regions of space where gravity is so strong that not even light can escape. Gravitational waves are ripples in space and time.

Fields

Mathematics & Statistics

Physics

Topics

general relativity

black holes

Kerr spacetime

Grants
1 known grant, through May 2028

What they work on

  1. Prove nonlinear stability of Kerr black holes, the standard model of a rotating black hole, for all spins below the maximum, showing that small disturbances decay over time, using geometric and microlocal analysis of wave equations.
  2. Analyze the stability of several classes of spacetimes containing many black holes, using tools from hyperbolic partial differential equations, the mathematics of waves, together with spectral and scattering theory.
  3. Construct solutions of Einstein's field equations for large-mass-ratio black hole mergers and for black hole scattering, and give a precise description of their overall geometry using geometric singular analysis.

More about the research

Detectors have measured these waves coming from pairs of black holes that spiral together and merge. After a merger, the single black hole left behind quickly settles into a steady state, a process called ringdown. Einstein's equations of general relativity describe all of this, but they are hard nonlinear partial differential equations. Nonlinear means effects feed back on themselves; partial differential equations describe how quantities change across space and time. Computer simulations can solve these equations approximately, yet basic questions still need rigorous mathematical proof.

Why it matters

This is basic mathematical research. Proving that black hole models are stable would put the black hole descriptions used in astrophysics and gravitational-wave astronomy on firm theoretical ground. The new methods for wave equations may also be useful for other problems involving waves and hyperbolic equations.

Known grants

From NIH and NSF research grants. Labs often have other funding we can't see.

Mathematical Analysis of Single- and Many-black-hole Spacetimes

NSF · Jun 2026 – May 2028

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Sergiu Klainerman

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Work toward proving the nonlinear stability of Kerr black holes with large angular momentum, removing the main obstacle to extending known results for slowly rotating black holes.

Sung-Jin Oh

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Prove a forward-in-time scattering criterion for initially outgoing solutions of the energy-critical wave maps and hyperbolic Yang-Mills equations, as a step toward the soliton resolution conjecture in the one-soliton regime.

Xuwen Zhu

Northeastern University, MA·Mathematics & Statistics

Study how gravitational instantons, four-dimensional spaces that solve Einstein's equations, degenerate and how their moduli spaces are structured, using geometric microlocal analysis and PDE techniques.

The school

Pennsylvania State University: 60 labs on PI Pages, $1.3B a year on research, 743 research doctorates a year.

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