spectral range for singe junction solar cells, and according to the Shockley-Queisser model the photocurrent is expected to be below 9.7 mA cm −2 . [2] However, a relatively high V oc of 1.4-1.5 V was reported, which makes this material system a great candidate for applications such as tandem configuration or other systems requiring spectral splitting. [2][3][4][5][6][7] Significant efforts were undertaken to investigate and optimize the V oc of CH 3 NH 3 PbBr 3 solar cells. [2][3][4][5][6][7][8][9] Engineering advanced hole transport layers (HTL) such as carbon nanotubes, [2] 2,2′,7,7′-tetrakis(N,Ndi-p-methoxyphenyl-amine)-9,9′-spirobifluorene (spiro-OMeTAD), [5,7] poly (indenofluoren-8-triarylamine) (PIF8-TAA), [3,4] and 4,4-bis(N-carbazolyl)-1,1-biphenyl (CBP) [6] resulted in V oc within a range of 1.4-1.5 V for solution-processed perovskite solar cells. Sheng et al. demonstrated a high V oc of 1.45 V using the architecture TiO 2 / CH 3 NH 3 PbBr 3 /spiro-OMeTAD via a vaporassisted depositon. [7] Kim et al. modified the TiO 2 surfaces with carboxyl groups and employed no HTL for CH 3 NH 3 PbBr 3 solar cells, producing a V oc of 1.37 V. [8] Dymshits et al. reported a V oc of 1.35 V for Al 2 O 3 /CH 3 NH 3 PbBr 3 perovskite solar cells without HTL. [9] These studies focused more on the V oc improvement via interface engineering and via optimizing the CH 3 NH 3 PbBr 3 film quality. Despite significant progress toward unraveling the V oc limitation of CH 3 NH 3 PbBr 3 solar cells, the limiting V oc (V oc,rad ) is still unknown to the best of our knowledge. Besides,
Perovskite solar cells based on CH