The quantum black hole of Oppenheimer-Snyder (a collapse model with quantum corrections) was studied in the presence of dark energy and a cloud of strings. Using the 6th-order WKB method, the quasi-normal mode frequencies (damped oscillations after perturbation) and greybody factors (which determine the emission spectrum) were calculated. It turned out that the string parameters, quantum deformation, and quintessence significantly affect how the black hole 'sounds' and how much energy it transmits. This helps us understand how quantum effects and dark energy can change the observational signatures of black holes.
A black hole, disturbed by a merger, rings at its own unique frequencies, like a bell. Each hole has its own 'voice', by which astronomers determine its characteristics. In a new study, scientists examined how this sound is affected by dark energy and hypothetical clouds of microscopic strings.
They looked at quantum black holes—very small objects where quantum effects are significant—and calculated changes in their vibrations. Also considered was the 'grayness factor': a measure of how easily radiation can escape the influence of the hole, without which signals from gravitational waves cannot be decoded. It turned out that both dark energy and string parameters noticeably shift the frequencies and transparency to light.
These calculations are a step toward future detectors. Learning to isolate such changes in signals could allow us to 'hear' not only the mass and spin of the hole, but also the contribution of dark energy. It is amazing that such mini-holes, likely born in the first moments of the Universe, could bring us the echo of the Big Bang.
🎯 The 'grayness factor' owes its name to neutron stars: it was devised for calculations of their radiation, and it gained widespread fame thanks to the works of [scientist:Stephen Hawking]Stephen Hawking[/scientist] on black hole evaporation.