Groundstate splitting around rotating mini Blackholes
I. Sturm, F.M.C. Witte

TL;DR
This paper calculates the spin-dependent groundstate energies of fermions around rotating mini blackholes, revealing a spin-splitting effect that could produce observable X-ray signatures from primordial blackholes.
Contribution
It introduces a novel calculation of fermionic boundstates in rotating blackhole spacetime using a slow rotation approximation and minimax variational method.
Findings
Groundstate energies are 0-5% of fermions' restmass.
Spin-dependent energy splitting is about 10% of the binding energy.
Potential observable X-ray signatures from primordial blackholes.
Abstract
In this letter we present the result of a spin-dependent groundstate-energy calculation for fermionic boundstates in the spacetime around a rotating blackhole. Using a slow rotation approximation and a minimax variational approach we find boundstate energies of 0 to 5 percent of the fermions flatspace restmass. The groundstate displays a spin-dependent splitting with an energy difference of about 10 percent of the binding energy. For a dilute gas of primordial mini blackholes with gravitationally bound electrons spin-flip transitions could possibly give rise to observable signatures in the observed soft X-ray spectrum for sources at cosmological distances.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Pulsars and Gravitational Waves Research · Cosmology and Gravitation Theories
