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We apply the covariant anomaly cancellation method to compute the Hawkingfluxes from the event and cosmic horizons of the Schwarzschild-de Sitter blackhole. The derivation is new from the existing ones as we split the space inthree different regions (near to and away from the event and cosmic horizons)and write down the covariant energy-momentum tensor using three step functionswhich covers the whole region leading elegantly to the conditions required tocompute the Hawking fluxes from the event and cosmic horizons.

Hawking radiation from black holes in de Sitter spaces via covariant anomalies