A Black Hole with Two Thermometers ✎ express

Original: "Two-Horizon Sector Thermodynamics as a Diagnostic for the Bi-Hair Organization of NUT Charge"
· Di Wu, Robert B. Mann, Shuang-Qing Wu
arXiv:2607.23644 · 2026-07-26 · arXiv non-exclusive · independent analysis · 1 min
Hidden thermal memory at event horizons defies familiar laws.

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A pot of boiling water is covered with two lids — an inner and an outer one. The thermometer under each shows its own temperature, but their harmonic mean (a special averaging method where you add the reciprocals) always remains unchanged. Heat seems to obey an invisible rule. The thermodynamics of black holes with a NUT charge, a peculiar gravitational parameter reminiscent of a magnetic charge, works in a similar way.

The harmonic mean of two numbers is not the usual arithmetic mean but the reciprocal of the average of the reciprocals. For the temperatures of the two horizons, it acts as a single "thermostat."

The physicists decided to test whether such a hole can be described honestly — not by tweaking temperatures to fit the answer, but by measuring them at both horizons. It turned out that a complete picture requires accounting for hidden rotation. This quantity is not like the familiar rotation of a star; it arises from a combination of mass and NUT charge, as if an invisible flywheel spins deep inside the hole.

Hidden rotation is not a new geometric parameter but a "thermodynamic hair": a property that shows up only in energy conservation laws, not in the fabric of spacetime itself.

This approach is reminiscent of diagnosing an engine by sound: without looking under the hood, you can detect a hidden malfunction. Here, the "sound" is played by thermal relations, and the "engine" is the black hole itself.

The NUT charge is named after three scientists (Newman, Unti, and Tamburino) and behaves almost like a magnetic monopole, but in gravity.

In Greg Egan's novel "The Light of Other Days," travelers encounter black holes whose hidden parameters alter the laws of physics around them.

Scientists
Stephen HawkingJacob BekensteinJohn Archibald WheelerWilliam UnruhFritz ZwickyKarl Schwarzschild
Concepts
no-hair theorem black hole thermodynamics scalar hair black hole carnot limit zeroth law of thermodynamics event horizon stability charge to mass ratio hawking area law kerr metric horizon area Noether's theorem