Hawking temperatures for emergent gravity metrics of KN and KNAdS are calculated along θ=0, modified by dark energy from DBI k-essence fields, with metrics satisfying Einstein equations at large r.
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The Hawking temperature in the context of dark energy for Kerr-Newman and Kerr-Newman-AdS backgrounds
Hawking temperatures for emergent gravity metrics of KN and KNAdS are calculated along θ=0, modified by dark energy from DBI k-essence fields, with metrics satisfying Einstein equations at large r.