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Coexistence of multiple regimes for near-field thermal radiation between two layers supporting surface phonon polaritons in the infrared

机译:支持红外表面声子极化子的两层之间近场热辐射的多种机制共存

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We demonstrate the coexistence of different near-field thermal radiation regimes between two layers supporting surface phonon polaritons (SPhPs) in the infrared. These regimes exist when the distance of separation between the media d is much smaller than the dominant emission wavelength. This coexistence is noticed after computations of the near-field radiative heat transfer coefficient h_r for silicon carbide films using fluctuational electrodynamics and following an asymptotic analysis of h_r. We show that the emergence of these regimes is a function of a dimensionless variable D defined as the ratio of the layer thickness t to d. When D》 1 for both films, SPhPs dominating near-field radiant energy exchange do not couple within the layers, such that h_r follows a d~(-2) power law as for the case of two planar half-spaces. When D 《 1 for both layers, the dominant SPhPs couple within the films, thus resulting in a splitting of the spectral distribution of flux into two distinct modes. Despite this splitting, the asymptotic expansion reveals that h_r varies as d~(-2) due to the fact that the spectral bands of high emission and absorption are essentially the same for both films. However, when both layers have a thickness of the order of a nanometer or less, a purely theoretical regime emerges where hr follows a d~4 asymptote. Also, when one layer has D 《 1 while the other one is characterized by D 》1, there is an important mismatch between the spectral bands of high emission and absorption of the films, thus resulting in a h_r varying as d~(-3). These various near-field thermal radiation regimes are finally summarized in a comprehensive regime map. This map provides a clear understanding of near-field thermal radiation regimes between two layers, which are particularly important for designing highly efficient nanoscale-gap thermophotovoltaic power generation devices.
机译:我们证明了在红外中支持表面声子极化子(SPhPs)的两层之间不同近场热辐射机制的共存。当介质d之间的分离距离远小于主要发射波长时,存在这些机制。在使用波动电动力学计算碳化硅膜的近场辐射传热系数h_r之后,并根据h_r的渐近分析,注意到了这种共存。我们表明,这些制度的出现是一个无量纲变量D的函数,该变量定义为层厚t与d的比值。当两张膜都为D》 1时,主导近场辐射能量交换的SPhP不在层内耦合,因此h_r遵循d〜(-2)幂定律,就像两个平面半空间的情况一样。当两层的D <1时,主要的SPhPs在薄膜内耦合,从而导致通量的光谱分布分裂为两个不同的模式。尽管有这种分裂,但渐进扩展表明h_r随d〜(-2)的变化而变化,这是因为两个薄膜的高发射和吸收光谱带基本相同。但是,当两个层的厚度都在纳米级或更小时,就会出现纯粹的理论状态,其中hr遵循d〜4渐近线。同样,当一层具有D 1而另一层具有D》 1的特征时,薄膜的高发射和吸收光谱带之间存在重要的失配,因此导致h_r随d〜(-3)变化)。最后,将这些不同的近场热辐射状况汇总在一个综合的状况图中。该图清楚地了解了两层之间的近场热辐射状态,这对于设计高效的纳米级间隙热光电发电设备特别重要。

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