How a Black Hole Gives Birth to Sound Particles ✛ ✎ ✦

Original: "Acoustic Hawking radiation as a tunnelling effect in Michel accretion"
· Nisha Jangid, Arnab K. Ray
arXiv:2607.00037 · 2026-06-28 · arXiv non-exclusive · independent analysis · 1 min
In the gas river around a black hole, sound encounters an invisible wall, and tiny ringing particles pierce through.

In a swift river where water flows faster than sound, a shout from the bank will be carried downstream but never return. The boundary where the flow speed matches the speed of sound is the sonic horizon. Below it, silence reigns. That very same boundary is created by infalling gas around a black hole. This was described mathematically by Schwarzschild. At the threshold of the sound barrier, the vacuum begins to produce quanta of sound — phonons. This process is the acoustic twin of Hawking radiation. An unexpected twist: spacetime curvature acts like a loudspeaker. It shifts frequencies upward, creating an analog of the blueshift of light, and makes the sound hundreds of times 'louder' than the temperature alone would allow. So in the noise of infalling gas, gravity intertwines with quantum fields and opens a window onto the mysteries of singularities and quantum thermodynamics.

The temperature of this sound radiation for a solar-mass black hole would be just a few billionths of a degree above absolute zero, but gravity can make it hundreds of times 'louder'.

\Omega = \omega \sqrt{1 + 3 a_c^2}
The curvature of spacetime increases the frequency of emitted phonons compared to a laboratory reference frame.
T_H = \frac{\hbar}{2\pi k_B} \left. \frac{d}{dr} \left( a_0 \sqrt{f+u_0^2} - |u_0| \right) \right|_{r_c}
The radiation temperature of the acoustic black hole, determined by the surface gravity at the sonic horizon.
Scientists
George GamowLeo EsakiStephen HawkingJacob BekensteinHenri PoincaréFritz Zwicky
Concepts
Hawking radiation hawking radiation mechanism black hole accretion winds sound wave acoustic oscillations black hole resonance wave amplification speed of sound ultrasound baryon acoustic oscillations phononic crystal echo moiré pattern effects Bekenstein-Hawking entropy radio loud quasar wind scalar perturbations overtones Hall effect thermal hall effect