Radiative-cooling-based nighttime electricity generation with power density exceeding 100 mW/m2

被引:33
作者
Omair, Zunaid [1 ]
Assawaworrarit, Sid [1 ]
Fan, Lingling [1 ]
Jin, Weiliang [1 ]
Fan, Shanhui [1 ]
机构
[1] Stanford Univ, Edward L Ginzton Lab, Stanford, CA 94305 USA
关键词
COMPREHENSIVE PHOTONIC APPROACH; ENERGY; DESIGN; PAINTS;
D O I
10.1016/j.isci.2022.104858
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The outer space (3 K) represents an important thermodynamic resource. It has been known for decades that at nighttime, a sky-facing thermal emitter radiating strongly within the atmospheric transparency window (8-13 pm), can reach below the ambient temperature. In recent studies, thermoelectric generators were used to harness this temperature difference between the emitter and ambient to generate electricity. However, the demonstrated power density has been limited by parasitic thermal losses. Here we show that these parasitic losses can be reduced through thermal engineering. We present a simple model showing the optimum power density can be approached by controlling the relation between the emitter area and the thermal resistance of the thermoelectric generator. We show that the stacking of multiple thermoelectric generators is an effective way to approach this optimum. We experimentally demonstrate a generated electric power density >10C mW/m(2), representing > 2-fold improvement over the previous results for nighttime radiative cooling.
引用
收藏
页数:10
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