A second high energy Hawking radiation predicted

Hawking's horizon surface area-entropy A black body radiation peaks at wavelength $\sim$A$^{1/2}$ $\sim$Unruh temperature T$^{-1}$. I predict a second higher Unruh temperature component with peak wavelength $\sim$ proper quantum thickness of the horizon $\sim$(LA$^{1/2}$)$^{1/2}$ with energy density $\sim$T$^{4}$ $\sim$hc/L$^2$A. The two Hawking surface and thickness radiations form a Carnot heat engine. L $=$ L$_{\mathrm{p}}$ corresponds to random black body gravity waves. L $\sim$ h/m$_{\mathrm{e}}$c for virtual electron-positron pairs stuck to the horizon corresponds to thermal photons. These apply both to observer independent black hole horizons as well as observer-dependent past and future cosmological horizons bounding the causal diamond. For gravity wave Hawking thickness radiation hc/L$_{\mathrm{p}}$$^2$A is the observed dark energy density if we use the future deSitter horizon entropy A. The Unruh effect suggests that the w $= \quad +$ 1/3 black body radiation for accelerating detectors corresponds to w $=$ -1 for the distant local inertial frame detectors.