Bound states of scalar fields exist outside quintessence-dressed AdS black holes for sufficiently large |w| or angular momentum, and quintessence alters the Hawking temperature so that large black holes radiate less.
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Formation of Bound States in Quintessence Alternative Theories
Bound states of scalar fields exist outside quintessence-dressed AdS black holes for sufficiently large |w| or angular momentum, and quintessence alters the Hawking temperature so that large black holes radiate less.