Which 'temperature' you use changes black hole radiation by 100x?

Black holes in universes with a cosmological constant have two horizons — one around the black hole, one at the cosmic edge — and no single agreed-upon temperature. Applying four common temperature prescriptions to a charged, scalar-field-dressed black hole, the author finds that the Bousso–Hawking definition boosts radiated power estimates by 10–100× compared to the raw surface-gravity formula, while an entropy-based prescription suppresses it. The gap matters because it sets the baseline for any real radiation calculation in these spacetimes.