Formation of Bound States in Quintessence Alternative Theories
George Koutsoumbas, Andri Machattou, Eleftherios Papantonopoulos
TL;DR
This work analyzes bound states of scalar perturbations outside the horizon of a quintessence-dressed AdS black hole by deriving a generalized Regge-Wheeler equation and associated potentials. It shows that quintessence, via parameters $a$ and $w$, modifies the background metric and Hawking temperature, which in turn shape the Regge-Wheeler potential and the existence of bound states. Bound-state masses emerge only for sufficiently large $|w|$ and/or angular momentum $l$, with masses increasing approximately linearly with $a$ and bandwidths decreasing for higher $l$, while charge $Q$ can suppress bound-state formation. The results bridge black-hole thermodynamics, quintessence physics, and quantum bound-state phenomena, suggesting cosmological implications and guiding future studies of quasinormal modes in such backgrounds.
Abstract
We study the formation and behaviour of bound states formed outside the horizon of a black hole in the presence of quintessence matter. Calculating the Regge and Wheeler potential for general metric function, we find that the presence of quintessence influences significantly the metric function and the Hawking temperature. We show that large black holes radiate less in the presence of quintessence matter and it seems to live longer, while small black holes radiate more in comparison with the model in the absence of quintessence. Bound states emerge at large enough quintessence parameter $|w|$ or angular momentum.
