https://doi.org/10.1140/epjc/s10052-025-14477-3
Regular Article - Theoretical Physics
Searching for quantum-gravity footprint around stellar-mass black holes
1
Osservatorio Astronomico di Brera, Istituto Nazionale di Astrofisica (INAF), Via E. Bianchi, 46, 23807, Merate, Italy
2
Sezione di Milano, Istituto Nazionale di Fisica Nucleare (INFN), Via G. Celoria, 16, 20133, Milan, Italy
3
Osservatorio Astrofisico di Torino, Istituto Nazionale di Astrofisica (INAF), Via Osservatorio, 20, 10025, Pino Torinese, Italy
4
Osservatorio Astrofisico di Catania, Istituto Nazionale di Astrofisica (INAF), Via Santa Sofia, 78, 95123, Catania, Italy
5
Sezione di Catania, Istituto Nazionale di Fisica Nucleare (INFN), Via Santa Sofia, 64, 95123, Catania, Italy
Received:
30
April
2025
Accepted:
27
June
2025
Published online:
8
July
2025
According to the asymptotically safe gravity, black holes may have characteristics different from those described according to general relativity if the running of the gravitational constant coupling happens at low energies. Particularly, they should be more compact, with a smaller event horizon, which in turn affects the other quantities dependent on it, like the photon ring and the size of the innermost stable circular orbit. We decided to test the latter hypothesis by searching in the literature for observational measurements of the inner radius of the accretion disk around stellar-mass black holes. We selected the smallest values measured when the disk was in high/soft state, made them homogeneous by taking into account the most recent and more reliable values of mass, spin, viewing angle, and distance from the Earth, and compared with the expectations of the Kerr metric. We do not find any significant deviation. Some doubtful cases can be easily understood as due to specific states of the object during the observation or instrumental biases.
© The Author(s) 2025
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