• <tr id="yyy80"></tr>
  • <sup id="yyy80"></sup>
  • <tfoot id="yyy80"><noscript id="yyy80"></noscript></tfoot>
  • 99热精品在线国产_美女午夜性视频免费_国产精品国产高清国产av_av欧美777_自拍偷自拍亚洲精品老妇_亚洲熟女精品中文字幕_www日本黄色视频网_国产精品野战在线观看 ?

    Nano Ag-enhanced photoelectric conversion efficiency in all-inorganic,hole-transporting-layer-free CsPbIBr2 perovskite solar cells

    2022-12-28 09:55:32YoumingHuang黃友銘YizhiWu吳以治XiaoliangXu許小亮FeifeiQin秦飛飛ShihanZhang張詩涵JiakaiAn安嘉凱HuijieWang王會杰andLingLiu劉玲
    Chinese Physics B 2022年12期
    關(guān)鍵詞:劉玲

    Youming Huang(黃友銘) Yizhi Wu(吳以治) Xiaoliang Xu(許小亮) Feifei Qin(秦飛飛) Shihan Zhang(張詩涵)Jiakai An(安嘉凱) Huijie Wang(王會杰) and Ling Liu(劉玲)

    1Tiangong University,Tianjin 300387,China

    2University of Science and Technology of China,Hefei 230026,China

    3Nanjing University of Posts and Telecommunications,Nanjing 210003,China

    4Shanxi Normal University,Shanxi 041004,China

    Keywords: Ag nanoparticles,local surface plasmons,perovskite solar cells based on CsPbIBr2

    1. Introduction

    With a decline in fossil energy resources (i.e., oil and coal) leading to a global energy crisis and the environmental pollution associated with these fossil fuels, the demand for clean and sustainable energy sources has become an important topic of growing concern for all. Solar cells convert the inexhaustible energy of the sun into electricity,representing one of the most promising solutions for harnessing solar energy.[1,2]Perovskite solar cells(PSCs)have attracted much attention due to their advantages of low production cost and simple fabrication. The power conversion efficiency (PCE)of PSCs has improved from 3.81% in 2009 to 25.7%[3–8]in 2022. The light absorption layer of highly efficient PSCs mostly contains organic groups. These organic groups are easily degraded in high-temperature, high-humidity environments,which restricts the development of organic PSCs.[9,10]Researchers have therefore turned their attention to the field of all-inorganic PSCs which have much better stability. Allinorganic PSCs based on CsPbIBr2material have excellent stability and stand out among the various types of all-inorganic PSCs. Maet al.[11]first reported CsPbIBr2-based PSCs, and achieved a PCE of 4.7%. Yanget al.[12]modified the surface of CsPbIBr2film with bifunctional dye molecules,and the optimized perovskite solar cells achieved an open circuit voltage(VOC)of 1.37 V and a PCE of 10.13%.

    In 2021, Duet al.[13]used (NiCo)1?yFeyOx-decorated graphene oxide (GO) as a hole booster in an all-inorganic CsPbIBr2PSC. A best efficiency of 10.95% was achieved,arising from the charge transfer doping effect between(NiCo)1?yFeyOxand GO. According to the latest report, the PCE of hole transport layer (HTL)-free carbon electrode CsPbIBr2perovskite solar cells has reached 11.04%,[14]but this is still far from the current maximum efficiency of PSCs.It can be seen that CsPbIBr2-based PSCs have good stability, but their PCE is low. The absorption of incident light by PSCs has an important influence on device performance.Therefore, the performance of CsPbIBr2-based PSCs can be improved by improving the absorption of incident light by these devices. Many attempts have been made to improve the performance of the PSCs,including modification of the lightabsorbing layer or doping of photoactive nanostructures.[15–17]Atwater and Polman[18]described the physical mechanism by which surface plasmon resonance (SPR) of metal nanostructures enhances the light absorption of solar cells, mainly including light scattering by metal nanoparticles (NPs) and near-field enhancement of the localized surface plasmon resonance (LSPR), which can be applied to solar cells. In recent years, SPR has been used in many fields.[19]Although LSPR of metal NPs is used to enhance the absorption of incident light by PSCs,there has been relatively little research work on this.[20–22]

    Wanget al.[23]and Leeet al.[24]have demonstrated the incorporation of Au NPs into the HTL of photovoltaic (PV)devices. Their results show that the SPR characteristics of Au NPs can greatly improve the light absorption capacity and photocurrent density of cell devices, accompanied by a small reduction in photovoltage. Cuiet al.[25]and Zhanget al.[26]incorporated Au NPs into the electron transport layer (ETL)of PSCs. The metal nanostructures in solar cells not only increase the optical path of light scattering[27,28]but can also could produce dipole–dipole interaction and resonance energy transfer,[29]which is expected to improve the PCE of PV devices. There have been no reports about metal NPs enhancing CsPbIBr2-based PSCs.

    In this work, Ag NP enhancement of CsPbIBr2-based PSCs with the structure FTO/(Ag)ZnO/CsPbIBr2/carbon(FTO is fluorine-doped tin oxide) is investigated. Different devices are obtained by controlling the surface coverage ratio (SC) of Ag NPs on the FTO surface. In this paper SC is defined as the proportion of the solar cell area with Ag NPs compared with the total solar cell area. When SC=10%the CsPbIBr2-based PSC achieves its best PCE of 2.7%,which is 9.76%higher than that of the control cells. Moreover,we use the finite difference time domain(FDTD)method to simulate the structure of our designed solar cell devices. The model devices with different Ag NP SCs are obtained by controlling the interval size of Ag NPs on the FTO substrate surface. The simulated transmittance, reflectance and absorptivity and also the simulated electric field distribution of each cross section are obtained using FDTD. We further analyze the Ag NP-enhanced CsPbIBr2PSCs. It is demonstrated that the near field enhancement and forward scattering of Ag NPs can enhance the performance of CsPbIBr2-based PSCs.To the best of our knowledge, there have been no reports using this method to improve the device performance of such CsPbIBr2PSCs. Ag NPs were chosen from among various metal NPs(Au, Ag, Al, etc.) due to their low price and relatively good controllability in the synthesis process.[30,31]

    2. Experimental methods

    2.1. Materials

    AgNO3(99.8%) was purchased from Tianjin Yingda Sparseness & Nobel Reagent Chemical Factory. Acetone(99.5%), ethyl alcohol (EtOH; 99.7%) and sodium citrate trihydrate (99%) were purchased from Tianjin Fengchuan Chemical Reagent Technology Co., Ltd. ZnO ceramic target (99.99%) was purchased from Zhongnuo New Material(Beijing) Technology Co., Ltd. Lead (II) bromide (PbBr2;99. 99%) and cesium iodide (CsI; 99.99%) were purchased from Xi’an Polymer Light Technology. Dimethylsulfoxide(DMSO;99.8%)was purchased from Aladdin.FTO glass substrates (7 ?) were received from Luoyang Guluo Glass Co.,Ltd.Commercial conductive carbon paste was purchased from Shanghai MaterWin New Materials Co.,Ltd. All these chemicals and reagents were used directly without any further purification.

    2.2. Device fabrication

    Figure 1 shows a flow chart of the laboratory preparation of enhanced CsPbIBr2-based PSCs. After boiling 150 mL of AgNO3solution (mass fraction 0.018%), 2 mL of sodium citrate trihydrate solution(mass fraction 2%)was added. This was stirred evenly and boiled then washed with EtOH several times, followed by dispersion in EtOH for 3 min to obtain Ag NPs with a diameter for about 150 nm. FTO glass was cleaned ultrasonically for 15 min in deionized water, acetone and EtOH, then dried with nitrogen. The FTO glass was put into a plasma cleaning machine for 10 min and the Ag NP solution was directly dripped onto the cleaned FTO surface.Three different Ag NP SC surfaces were obtained by controlling the amount of solution. ZnO films were deposited onto the FTO by radio-frequency sputtering. The sputtering time was 60 min, the sputtering power was 50 W, the flow rate of argon (purity 99.99%) was 14 sccm and the working pressure was 3 Pa. After plasma cleaning of FTO with ZnO films,CsPbIBr2films were deposited on the ZnO films in a glove box using one-step spin coating. Then 50μL of CsPbIBr2precursor solution was dropped on the ZnO film and the substrate rotated. For the spin coating, the rotation speed of the stage was 3000 rpm for 40 s. The above samples were annealed at 160?C for 20 min. The CsPbIBr2precursor solution was prepared according to the literature: 370 mg PbBr2and 259 mg CsI were dissolved in 1 mL of DMSO at room temperature.Finally,carbon electrodes were deposited on the CsPbIBr2layer as the HTL and back electrodes and annealed at 100?C for 20 min. The active area of each device was 0.20 cm2.

    Fig. 1. Flowchart for preparing enhanced CsPbIBr2-based PSCs in the laboratory.

    2.3. Characterization

    Surface morphologies of the films were analyzed using a field emission scanning electron microscope(SEM;Gemini 300). Photoluminescence spectra (PL) were recorded using a fluorescence spectrometer (Hitachi, F7000). Ultraviolet–visible (UV–vis) absorption spectra were recorded using a UV–vis near-infrared spectrophotometer (PerkinElmer,Lambda 35). TheJ–Vcurves of the CsPbIBr2-based PSCs were obtained using a Keithley 2400 source meter under AM 1.5 G illumination at 100 mW·cm?2(Newport Oriel Sol3A),which was calibrated using a standard silicon solar cell. Measurements of external quantum efficiency (EQE) were performed using a quantum efficiency measurement system(QER,EnliTech)in the 300 nm–700 nm wavelength range.

    3. Results and discussion

    The SEM image of Ag NPs prepared on the surface of the FTO substrate is shown in Fig. 2(a). Spherical Ag NPs with a diameter of about 150 nm can be seen. The UV–vis absorption spectrum of Ag NPs in EtOH is shown in Fig. 2(b). It can be seen that the Ag NP structure has a specific SPR absorption peak at about 475 nm. A SEM image of Ag NPs agglomerated and stacked on the FTO substrate is shown in Fig.2(c). As shown in Fig.3(a),when SC=5%,Ag NPs on the surface of the FTO substrate are sparsely distributed and relatively uniform.As the SC of the Ag NPs increases to 10%,the Ag NPs on the surface of the FTO substrate show local aggregation(see Fig.3(b)),but are still monolayer structures.When SC further increases to 15% (Fig. 3(c)), a large number of Ag NPs on the surface of the FTO substrate become aggregated into clusters. It can be seen that Ag NPs accumulate with increasing SC; we believe that the reasons for this phenomenon are the uneven distribution of NPs accompanied by solvent volatilization and the increase in the number of Ag NPs,which may be caused by anisotropy of the FTO substrate.

    The UV–vis absorption spectra of the ZnO/CsPbIBr2film when SC=10% and SC=0% are shown in Fig. 4(a). Both show similar absorption characteristics within the visible spectrum (400 nm–700 nm), and their absorption edges are in the same position. In the visible light range of 400 nm–700 nm,the ZnO/CsPbIBr2film(SC=10%)has a stronger absorption intensity, which could be attributed to spectral overlap between CsPbIBr2films and plasmon resonance of Ag NPs.[32,33]Correspondingly,more photocarriers are generated,which is conducive to an increase in the short circuit current densityJsc. The PL spectra of the ZnO/CsPbIBr2film at SC=10% and SC=0% are shown in Fig. 4(b). It can be seen that the emission peaks of both samples are at 605 nm.The emission peak intensity of the SC=10%sample is higher than that of the SC=0%one.The SC=10%sample achieved an integrated PL intensity of 9.40 arb. units compared with 8.14 arb. units for the sample without Ag NP doping, an increase of 15.48% in integrated PL intensity. The surface of Ag NPs has a strong local field which increases the photon density and the excited state density in the device. As a result, the number of electron–hole pairs increases, radiation recombination is enhanced and fluorescence intensity is improved. The increase in the PL intensity of perovskite films on the ZnO with SC=10% is due to the above reasons. It has been proved that SPR can improve PL intensity.[33]It is useful to boost theVOCof PSCs because theVOCof solar cells is positively correlated with the emission peak intensity of the light absorption layer.[34,35]In Fig. 4(b), there are many peaks besides the main peak in the PL spectrum; we believe that this phenomenon is caused by defect luminescence of ZnO materials and perovskite materials. The cross-sectional SEM image of the carbon-based CsPbIBr2PSC device is presented in Fig. S1 and a layered structure can be clearly identified. We show the energy level schematic diagram of the FTO/(Ag)ZnO/CsPbIBr2/carbon solar cell in Fig.5.

    Fig.2. (a)SEM image of Ag NPs on the FTO substrate. (b)Uv–vis absorption spectra of Ag NPs. (c)SEM image of Ag NPs agglomerated and stacked on the FTO substrate.

    Fig.3. SEM images of a FTO substrate with different Ag SCs: (a)SC=5%,(b)SC=10%,(c)SC=15%.

    We changed the particle SC of Ag NPs on the FTO surface and then prepared the devices. Table S1 shows the parameters of each device. As the Ag NP SC increased from 0 to 10%,the PCE of PSCs increased from 2.46%to 2.70%. When the SC is 10%, the solar cell achieves its best performance.ItsVOCis 0.8 V,Jscis 8.02 mA·cm?2and FF is 0.42. These enhancements are mainly due to the introduction of Ag NPs,which improve the light absorption of the CsPbIBr2PSC and finally turn into excess photogenerated carriers. In addition,perovskite is a direct band gap material; it is easy to recombine radiation and re-emit usable photons to realize the photon cycle effect.[36,37]As the addition of Ag NPs gives the film a higher fluorescence intensity, the generation and separation ability of photogenerated carriers can be improved through the photon cycle effect. The improvement of the sample with SC=5% is not so obvious because there are insufficient Ag NPs to excite the surface plasmons. However, as the Ag NP SC further increases to 15%,the PCE of the PSC decreases to 1.27%. In this condition, too many Ag NPs on the surfaces(Fig. 3(c)) hinder light from entering into the CsPbIBr2and decrease the absorption of incident light.

    Fig.4. UV–vis absorption spectra of ZnO/CsPbIBr2 thin films with different Ag SCs. (b)PL spectra of ZnO/CsPbIBr2 thin films with different Ag SCs.

    Fig.5. Corresponding energy band diagrams of CsPbIBr2 PSCs.

    Figure 6(a) shows theJ–Vcurve of the device when the Ag NP SC is 10%and 0%.When the AgNP SC is 0%,theVOCof the device is 0.72 V and theJscis 7.46 mA·cm?2. TheVOCandJscof the device with SC=10% increased to 0.8 V and 8.02 mA·cm?2, respectively. This indicates that the addition of Ag NPs improves the performance of the device.

    The EQE curves of the corresponding solar cells are illustrated in Fig.6(b). It can be seen that the spectral response range of both devices is roughly in the 300 nm–600 nm wavelength range. The EQE value of the device with SC=10%is higher than the device without Ag NPs. Furthermore, across the optical response range, the maximum EQE of the device with SC=10%is 66.57%,which is significantly higher than that of the device (63.20%) without Ag NPs. The improved EQE value facilitates the enhancement of the photoelectric conversion properties.

    Fig.6. (a)Current density–voltage(J–V)characterization of PSCs with different Ag SCs. (b) External quantum efficiency (EQE) characterization of PSCs with different Ag SCs.

    Fig.7. Simulated absorptance of the samples with different Ag SCs.

    To further investigate the influence of the near-field enhancement of the LSPR by Ag NPs on the performance of PSCs, a 3D model was established using the FDTD method. The ‘Johnson and Christy’ model was adopted for the Ag NPs. The numerically simulated device structure(see Fig. S2(a)) is glass/FTO (350 nm)/ZnO (200 nm)/CsPbIBr2(250 nm)/carbon and the spherical Ag NPs are embedded at the FTO/ZnO interface. The numbers in brackets represent the actual thickness of the corresponding layer.

    As shown in Fig.S2(a),perfectly matched layer boundary conditions were used in thez-direction and periodic boundary conditions were used in thex/y-direction. The diameter of Ag NPs was set to 150 nm and different SCs were used. The SC can be obtained by changing the intervals between two particles.Figure S2(b)shows thex–zplane(y=0)and the monitoring positions of eachx–yplane. The simulated transmittance of the samples with different Ag SCs is shown in Fig. S3(a).When Ag NPs are put on the FTO surface the transmittance decreases with increasing the Ag NP SC,which may increase the blocking of incident light. Figure S3(b) shows the simulated reflectance of the samples with different Ag SCs. The sample without the addition of Ag NPs has the lowest reflectance.According to the simulated reflectivity and transmittance, it can be inferred that the absorption rate of the device increases with increase of in SC.The monitoring positions of reflectivity and transmittance refer to Fig.S2(a).

    The absorptance of different samples was plotted according to Fig. S3, as shown in Fig. 7. It can be seen that the position of the absorption peak is about 425 nm. As can be seen in the figure, the absorbance of the sample without the addition of Ag NPs is lower. In addition,the absorptance with SC=15% is lower than that with SC=10%, indicating that excessive Ag NPs will reduce the absorption of incident light.

    Fig. 8. Simulated electric field distribution (λ =425 nm) in the x–z plane(y=0): (a)SC=0%,(b)SC=10%.

    The simulated electric field distribution with an excitation wavelength of 425 nm is shown in Figs. 8 and 9. Hereλ=425 nm due to its position close to the resonance absorption peak of Ag NPs,and it has higher absorptance than with other wavelengths. Figures 8(a) and 8(b) are the simulated electric field distributions of the devices with SC=0% and SC=10% atλ=425 nm, where all figures are in thex–zplane (y=0). As shown in Fig. 8(b), the electric field intensity of the CsPbIBr2layer of the device with SC=10% is greater than that of the SC=0%device. More incident light would be absorbed because the rate of absorption of light is proportional to the intensity for a given wavelength. Figure 8 is divided into three areas: (i) 0 nm

    Figure 9 shows the simulated electric field distribution on thex–yplane for different values ofz. The monitoring positions on eachx–yplane correspond to (i), (ii), and (iii), respectively, in Fig. S2(b). Figures 9(a) and 9(b) show that the electric field intensity of the device (forz=?205 nm) with SC=10%is significantly higher than that of the device with SC=0%; this indicates that the absorption of incident light is improved. As shown in Figs. 9(c) and 9(d), the electric field intensity of the device(forz=?350 nm)with SC=10%is significantly higher than that of the device with SC=0%.Compared with Fig. 9(b), the areas in Fig. 9(d) where electric field intensity significantly increased were at the edge of the plane. Figures 9(e) and 9(f) show that the electric field intensity of the device (forz=?450 nm) with SC=10% is significantly higher than that of the device with SC=0%. The form of electric field enhancement shown in Fig.9(f)is similar to Figs.9(b)and 9(d), but the blue region in the center of the plane is larger. The blue areas in the center of the plane in Figs.9(b),9(d),and 9(f)are the area below the Ag NPs in the model.

    As this area is shielded by Ag NPs it cannot be irradiated by incident light. Compared with other areas, the blue area absorbs less incident light,resulting in a low electric field intensity. However, the electric field intensity around the blue region is significantly enhanced compared with that in other areas,due to the forward scattering of the incident light by the Ag NPs. The reason for this phenomenon is that after incident light is scattered forward by Ag NPs, the scattered light path intersects with other incident light paths on the plane. The light-absorbing layer therefore absorbs more incident light energy and hence could stimulate more photocarriers in the CsPbIBr2layer. It can be seen from Figs. 9(b), 9(d) and 9(f)that the blue area in the samex–yplane increases with the location of the monitoring plane away from the ZnO/CsPbIBr2plane. The above phenomenon shows a distinct angular distribution,which is consistent with the forward-scattering feature in Fig. 8(b). As is generally known, the forward-scattering effect of Ag NPs is an important factor that improves the performance of devices. Moreover,it can be seen from Figs.9(b),9(d)and 9(f)that the electric field around the blue area of the plane is not uniform, and the electric field in the region not affected by the forward-scattering effect is also increased,indicating that enhancement of the electric field cannot simply be attributed to the forward-scattering effect of Ag NPs but is also related to the near-field enhancement of the LSPR.Therefore,it is reasonable to believe that the enhancement of device performance is caused by the near-field enhancement of the LSPR and forward scattering of Ag NPs.

    Fig.9. Simulated electric field distribution(λ =425 nm)in x–y plane below the CsPbIBr2 layer: (a),(b)z=?205 nm;(c),(d)z=?350 nm;(e),(f)z=?450 nm. (a),(c),(e),(g)SC=0%;(b),(d),(f),(h)SC=10%.

    4. Conclusion

    In summary, we conducted experimental and numerical simulation studies on Ag NP-enhanced all-inorganic hole-free PSCs based on CsPbIBr2materials. The near-field enhancement and forward scattering of Ag NPs are utilized to improve the absorption of incident light and enhance the performance of the device. When a Ag NP solution was dropped on the surface of FTO, the PCE of the PSCs reached 2.70%when SC=10%,which was 9.76%higher than that of devices with SC=0%. We can understand the experimental results through numerical simulation using the FDTD method. Considering the feasibility of this technology,our experiment provides a method for improving the efficiency of all-inorganic PSCs based on CsPbIBr2materials.

    Acknowledgments

    Project supported by the National Natural Science Foundation of China(Grant Nos.11504264,21802092,51501128,52072005, and 51872279) and the Scientific Research Plan Project of Tianjin Municipal Education Commission (Grant No.2017KJ097).

    猜你喜歡
    劉玲
    數(shù)與代數(shù)復(fù)習(xí)指導(dǎo)
    ——數(shù)的認識
    『比的化簡』大家談
    Electron excitation processes in low energy collisions of hydrogen–helium atoms
    Optoelectronic oscillator-based interrogation system for Michelson interferometric sensors
    刺莓華
    我們愛老師
    描述人物的不同造型
    What is middle school like
    森林里的怪婆婆
    如何描述植物
    国产高清视频在线播放一区 | 免费观看人在逋| 国产免费又黄又爽又色| 精品亚洲成a人片在线观看| 一边摸一边做爽爽视频免费| 丁香六月天网| 午夜福利免费观看在线| 亚洲精品日韩在线中文字幕| 亚洲国产av新网站| 人人澡人人妻人| 午夜福利影视在线免费观看| 亚洲专区中文字幕在线| 女性生殖器流出的白浆| 99热国产这里只有精品6| 久久综合国产亚洲精品| 九色亚洲精品在线播放| 亚洲欧美中文字幕日韩二区| 日韩,欧美,国产一区二区三区| 久久久欧美国产精品| 国产成人一区二区在线| 国产精品.久久久| 久久人妻福利社区极品人妻图片 | 精品一区在线观看国产| 真人做人爱边吃奶动态| 午夜日韩欧美国产| 亚洲专区国产一区二区| 国产欧美日韩一区二区三区在线| 韩国精品一区二区三区| 国产一区有黄有色的免费视频| 在线观看免费视频网站a站| 精品人妻一区二区三区麻豆| 日本欧美视频一区| 人人妻人人爽人人添夜夜欢视频| 国产精品二区激情视频| 亚洲国产日韩一区二区| 黄色一级大片看看| 国产亚洲欧美在线一区二区| 国产熟女欧美一区二区| 久久久亚洲精品成人影院| 亚洲色图 男人天堂 中文字幕| 色精品久久人妻99蜜桃| 欧美成狂野欧美在线观看| 亚洲国产av新网站| 男女边吃奶边做爰视频| 国产免费视频播放在线视频| 啦啦啦啦在线视频资源| 亚洲中文av在线| 美女主播在线视频| av国产久精品久网站免费入址| 国产欧美日韩一区二区三区在线| 国产男女超爽视频在线观看| 在线av久久热| 一边摸一边抽搐一进一出视频| 国产一区有黄有色的免费视频| 国产有黄有色有爽视频| 性少妇av在线| 老司机午夜十八禁免费视频| 一级黄片播放器| 一本大道久久a久久精品| 777久久人妻少妇嫩草av网站| 免费在线观看影片大全网站 | 999精品在线视频| 亚洲国产看品久久| 一二三四社区在线视频社区8| videosex国产| 亚洲一区二区三区欧美精品| 精品国产乱码久久久久久小说| 一本—道久久a久久精品蜜桃钙片| 欧美中文综合在线视频| 伦理电影免费视频| 激情五月婷婷亚洲| 人人妻,人人澡人人爽秒播 | 新久久久久国产一级毛片| 天天躁狠狠躁夜夜躁狠狠躁| 日韩欧美一区视频在线观看| 亚洲久久久国产精品| 一级毛片黄色毛片免费观看视频| 天天躁夜夜躁狠狠久久av| 日韩伦理黄色片| 18禁裸乳无遮挡动漫免费视频| 国产精品一区二区免费欧美 | www日本在线高清视频| 日韩中文字幕欧美一区二区 | 菩萨蛮人人尽说江南好唐韦庄| 国产亚洲午夜精品一区二区久久| 亚洲精品国产av成人精品| 性色av一级| 91字幕亚洲| 宅男免费午夜| 另类精品久久| 国产日韩欧美亚洲二区| 久久狼人影院| 久久鲁丝午夜福利片| 99国产综合亚洲精品| 永久免费av网站大全| 男的添女的下面高潮视频| 丝袜人妻中文字幕| 亚洲欧洲国产日韩| 高清av免费在线| 国产日韩一区二区三区精品不卡| 国产成人免费无遮挡视频| 老司机影院成人| a 毛片基地| 国产爽快片一区二区三区| 国产在线观看jvid| 国产精品国产av在线观看| 久久久久精品人妻al黑| 成人亚洲精品一区在线观看| 国产精品av久久久久免费| 成人黄色视频免费在线看| 日韩一卡2卡3卡4卡2021年| 狂野欧美激情性xxxx| 天天躁日日躁夜夜躁夜夜| 少妇 在线观看| 另类精品久久| videos熟女内射| 亚洲精品美女久久av网站| 青草久久国产| 成人影院久久| 亚洲精品一卡2卡三卡4卡5卡 | 日韩av在线免费看完整版不卡| 国产精品九九99| 国产免费视频播放在线视频| 午夜免费观看性视频| 老司机靠b影院| 建设人人有责人人尽责人人享有的| 又紧又爽又黄一区二区| 热re99久久精品国产66热6| 涩涩av久久男人的天堂| 国产一卡二卡三卡精品| 国产熟女欧美一区二区| 99香蕉大伊视频| 国产激情久久老熟女| 不卡av一区二区三区| 午夜福利乱码中文字幕| 免费高清在线观看视频在线观看| 亚洲国产最新在线播放| 另类亚洲欧美激情| 麻豆国产av国片精品| 91精品伊人久久大香线蕉| 精品人妻一区二区三区麻豆| 十八禁人妻一区二区| 黄色怎么调成土黄色| 亚洲 国产 在线| 免费女性裸体啪啪无遮挡网站| 国产激情久久老熟女| 丰满饥渴人妻一区二区三| 亚洲国产日韩一区二区| 777米奇影视久久| 国产黄色视频一区二区在线观看| 赤兔流量卡办理| 亚洲天堂av无毛| 大片免费播放器 马上看| 少妇精品久久久久久久| 国产色视频综合| 午夜日韩欧美国产| 国产一卡二卡三卡精品| 日韩大片免费观看网站| 一级a爱视频在线免费观看| 国产成人一区二区在线| 成年女人毛片免费观看观看9 | 日韩精品免费视频一区二区三区| 成人黄色视频免费在线看| 国产免费一区二区三区四区乱码| 久久毛片免费看一区二区三区| 日本色播在线视频| 我要看黄色一级片免费的| h视频一区二区三区| 国产黄频视频在线观看| 欧美人与性动交α欧美软件| 亚洲国产精品999| 亚洲av成人精品一二三区| 亚洲精品日本国产第一区| 亚洲男人天堂网一区| 国产成人av教育| 男人爽女人下面视频在线观看| 久久av网站| 日本wwww免费看| 五月天丁香电影| 美女福利国产在线| 成人午夜精彩视频在线观看| 精品久久久久久电影网| 欧美精品亚洲一区二区| 夫妻性生交免费视频一级片| 成人影院久久| 欧美精品高潮呻吟av久久| 久久久久久久久久久久大奶| 久久精品久久精品一区二区三区| 日韩精品免费视频一区二区三区| 国产成人av教育| a级毛片黄视频| 国产成人一区二区在线| 日韩av免费高清视频| 亚洲五月色婷婷综合| 国产亚洲欧美在线一区二区| 国产男人的电影天堂91| 老熟女久久久| 亚洲人成电影观看| 免费日韩欧美在线观看| av有码第一页| 中文字幕最新亚洲高清| 丝袜喷水一区| 国产国语露脸激情在线看| 老司机亚洲免费影院| 1024香蕉在线观看| 日韩大片免费观看网站| 在线亚洲精品国产二区图片欧美| 男女边摸边吃奶| 日日摸夜夜添夜夜爱| 巨乳人妻的诱惑在线观看| 久久九九热精品免费| 欧美日韩国产mv在线观看视频| 国产欧美日韩一区二区三 | 91麻豆av在线| 女人被躁到高潮嗷嗷叫费观| 久久久亚洲精品成人影院| 国产精品一区二区在线不卡| 黄色视频在线播放观看不卡| 在线 av 中文字幕| 亚洲国产精品一区三区| 精品一区二区三区av网在线观看 | 欧美在线黄色| 国产伦人伦偷精品视频| 亚洲国产中文字幕在线视频| 国产精品99久久99久久久不卡| 精品亚洲成a人片在线观看| 美女高潮到喷水免费观看| 亚洲精品美女久久av网站| 国产一区有黄有色的免费视频| 日韩精品免费视频一区二区三区| 90打野战视频偷拍视频| 欧美日韩视频精品一区| 啦啦啦在线观看免费高清www| 免费在线观看日本一区| 天堂俺去俺来也www色官网| 久久精品熟女亚洲av麻豆精品| 欧美日韩综合久久久久久| 黄色片一级片一级黄色片| 啦啦啦在线免费观看视频4| 午夜精品国产一区二区电影| 五月开心婷婷网| 午夜激情久久久久久久| 精品国产超薄肉色丝袜足j| 久久久久精品人妻al黑| 少妇人妻久久综合中文| 999精品在线视频| cao死你这个sao货| 亚洲中文日韩欧美视频| 国产精品久久久人人做人人爽| 极品人妻少妇av视频| 久久久精品区二区三区| 欧美xxⅹ黑人| 国产成人免费无遮挡视频| 考比视频在线观看| 国产男人的电影天堂91| 在线观看人妻少妇| 日韩制服骚丝袜av| 悠悠久久av| 男女下面插进去视频免费观看| 亚洲 欧美一区二区三区| 亚洲国产看品久久| 各种免费的搞黄视频| 免费在线观看影片大全网站 | 欧美精品av麻豆av| 亚洲欧美色中文字幕在线| 美女主播在线视频| 老司机在亚洲福利影院| 涩涩av久久男人的天堂| 日日摸夜夜添夜夜爱| 一二三四在线观看免费中文在| 成人午夜精彩视频在线观看| 婷婷色麻豆天堂久久| 9色porny在线观看| 精品亚洲乱码少妇综合久久| 中文字幕人妻丝袜制服| 亚洲,一卡二卡三卡| 午夜福利乱码中文字幕| 国产男人的电影天堂91| 人人妻,人人澡人人爽秒播 | 91九色精品人成在线观看| 欧美黑人欧美精品刺激| 伦理电影免费视频| avwww免费| 免费不卡黄色视频| www.自偷自拍.com| 久久精品亚洲av国产电影网| 秋霞在线观看毛片| 电影成人av| 欧美人与性动交α欧美软件| 丝袜美腿诱惑在线| 丝袜美足系列| 岛国毛片在线播放| 色视频在线一区二区三区| 午夜福利乱码中文字幕| 欧美日韩亚洲国产一区二区在线观看 | 婷婷成人精品国产| 久久国产精品大桥未久av| 可以免费在线观看a视频的电影网站| 五月天丁香电影| 一区福利在线观看| 在线观看免费日韩欧美大片| 日本av手机在线免费观看| 伊人久久大香线蕉亚洲五| 国产精品av久久久久免费| 熟女少妇亚洲综合色aaa.| 又紧又爽又黄一区二区| 国产精品av久久久久免费| 日日摸夜夜添夜夜爱| 久久亚洲国产成人精品v| 国产男女内射视频| 精品国产一区二区三区四区第35| 精品久久蜜臀av无| 丝袜喷水一区| 首页视频小说图片口味搜索 | 七月丁香在线播放| a 毛片基地| 国产精品二区激情视频| 亚洲国产av影院在线观看| 无限看片的www在线观看| 午夜91福利影院| 久久国产精品影院| 国产精品.久久久| 2018国产大陆天天弄谢| 美女国产高潮福利片在线看| 午夜福利一区二区在线看| 成人手机av| 高清不卡的av网站| 极品少妇高潮喷水抽搐| 天堂中文最新版在线下载| 欧美少妇被猛烈插入视频| 久久精品亚洲熟妇少妇任你| 久久午夜综合久久蜜桃| a 毛片基地| 91成人精品电影| 夫妻性生交免费视频一级片| 亚洲免费av在线视频| 黄片播放在线免费| 日本一区二区免费在线视频| 一本大道久久a久久精品| 精品人妻1区二区| 天天操日日干夜夜撸| 久久午夜综合久久蜜桃| 亚洲图色成人| 老鸭窝网址在线观看| 国产99久久九九免费精品| 欧美精品高潮呻吟av久久| 一区二区三区精品91| 美国免费a级毛片| 欧美变态另类bdsm刘玥| 国产男女内射视频| 久久久精品免费免费高清| 亚洲精品国产一区二区精华液| tube8黄色片| 日韩大片免费观看网站| 国产成人系列免费观看| 久久久久久亚洲精品国产蜜桃av| 一个人免费看片子| 精品一区二区三区四区五区乱码 | 在线观看www视频免费| 19禁男女啪啪无遮挡网站| 亚洲国产av影院在线观看| 久久久久久久久免费视频了| 97精品久久久久久久久久精品| 国产在线免费精品| 91国产中文字幕| 黄色a级毛片大全视频| 国产日韩欧美在线精品| 桃花免费在线播放| 在线观看人妻少妇| 美女主播在线视频| 97人妻天天添夜夜摸| www.999成人在线观看| 爱豆传媒免费全集在线观看| 亚洲欧美一区二区三区国产| 看免费成人av毛片| 免费久久久久久久精品成人欧美视频| 国产成人欧美| 狠狠婷婷综合久久久久久88av| 高潮久久久久久久久久久不卡| 在线观看一区二区三区激情| 亚洲成国产人片在线观看| 国产亚洲精品第一综合不卡| 国产精品人妻久久久影院| 免费黄频网站在线观看国产| 色综合欧美亚洲国产小说| 日韩视频在线欧美| av又黄又爽大尺度在线免费看| 午夜影院在线不卡| 国产精品三级大全| h视频一区二区三区| 亚洲欧洲日产国产| 久久天堂一区二区三区四区| 91老司机精品| 国产精品.久久久| 亚洲中文日韩欧美视频| 香蕉丝袜av| 又黄又粗又硬又大视频| 男女免费视频国产| 欧美精品亚洲一区二区| 一区二区三区精品91| 久久久久久免费高清国产稀缺| 国产精品成人在线| 久久久久久久国产电影| 国产成人免费观看mmmm| 欧美97在线视频| 日韩av免费高清视频| 久久久精品免费免费高清| 伦理电影免费视频| 久久久久精品人妻al黑| 大片免费播放器 马上看| 午夜福利在线免费观看网站| 精品久久久精品久久久| 国产成人精品无人区| 777久久人妻少妇嫩草av网站| a级毛片在线看网站| 国产亚洲av高清不卡| 久久99精品国语久久久| 老汉色∧v一级毛片| 欧美日韩一级在线毛片| av在线app专区| 十分钟在线观看高清视频www| 国产精品麻豆人妻色哟哟久久| 国产男人的电影天堂91| 久久天堂一区二区三区四区| 精品少妇久久久久久888优播| 日韩,欧美,国产一区二区三区| 在线观看免费高清a一片| 亚洲av电影在线进入| 咕卡用的链子| 99国产精品一区二区蜜桃av | 亚洲少妇的诱惑av| 一区二区三区精品91| 男人爽女人下面视频在线观看| 亚洲成色77777| 天堂8中文在线网| 国产精品久久久人人做人人爽| 18禁裸乳无遮挡动漫免费视频| 午夜精品国产一区二区电影| 亚洲av国产av综合av卡| 欧美亚洲日本最大视频资源| 久久久精品国产亚洲av高清涩受| 国产成人系列免费观看| www.熟女人妻精品国产| www.999成人在线观看| 午夜福利视频精品| 欧美xxⅹ黑人| 日韩一区二区三区影片| 久9热在线精品视频| 嫩草影视91久久| 一本—道久久a久久精品蜜桃钙片| 大型av网站在线播放| 国产成人免费无遮挡视频| 成在线人永久免费视频| 丝袜脚勾引网站| 欧美日韩成人在线一区二区| 男人舔女人的私密视频| av又黄又爽大尺度在线免费看| 国产av一区二区精品久久| 人人澡人人妻人| 久久精品人人爽人人爽视色| 欧美性长视频在线观看| 国产黄色免费在线视频| 中文字幕亚洲精品专区| 中文字幕色久视频| 一区二区日韩欧美中文字幕| 黑人欧美特级aaaaaa片| 亚洲av电影在线进入| 免费日韩欧美在线观看| 亚洲五月婷婷丁香| 老熟女久久久| www.精华液| 少妇被粗大的猛进出69影院| 国产激情久久老熟女| 国产日韩欧美亚洲二区| 18禁黄网站禁片午夜丰满| 性色av一级| 色精品久久人妻99蜜桃| 汤姆久久久久久久影院中文字幕| 超碰成人久久| 狠狠婷婷综合久久久久久88av| 久久精品国产综合久久久| 看十八女毛片水多多多| 日日爽夜夜爽网站| 亚洲国产日韩一区二区| 欧美久久黑人一区二区| 成年动漫av网址| 大片电影免费在线观看免费| 天天躁狠狠躁夜夜躁狠狠躁| 亚洲五月婷婷丁香| 国产一区二区三区av在线| 一本久久精品| 色网站视频免费| 9色porny在线观看| avwww免费| 日本av免费视频播放| 中文乱码字字幕精品一区二区三区| 色94色欧美一区二区| 午夜福利视频精品| 在线天堂中文资源库| xxxhd国产人妻xxx| 老汉色av国产亚洲站长工具| 人人澡人人妻人| 午夜福利,免费看| 亚洲欧洲精品一区二区精品久久久| 少妇精品久久久久久久| 成人国产av品久久久| 狠狠婷婷综合久久久久久88av| 午夜91福利影院| 午夜福利免费观看在线| 中文字幕精品免费在线观看视频| 免费高清在线观看视频在线观看| 乱人伦中国视频| 亚洲国产中文字幕在线视频| 成年人免费黄色播放视频| 超碰成人久久| 欧美成狂野欧美在线观看| 国产日韩欧美亚洲二区| 国产高清国产精品国产三级| 老司机影院毛片| 黄色视频在线播放观看不卡| 免费在线观看黄色视频的| 精品一区二区三卡| 久久久久久久精品精品| 性色av乱码一区二区三区2| 亚洲中文字幕日韩| 国产成人91sexporn| 两个人免费观看高清视频| 啦啦啦中文免费视频观看日本| 免费观看av网站的网址| 国产精品一二三区在线看| 免费不卡黄色视频| 18禁国产床啪视频网站| 91九色精品人成在线观看| 亚洲精品日韩在线中文字幕| 亚洲国产精品国产精品| 成人影院久久| 丝袜美腿诱惑在线| 激情视频va一区二区三区| 十分钟在线观看高清视频www| 18禁国产床啪视频网站| 青青草视频在线视频观看| 99国产精品免费福利视频| 成年人免费黄色播放视频| www.熟女人妻精品国产| 久久久欧美国产精品| 大码成人一级视频| 国产精品久久久av美女十八| 啦啦啦在线观看免费高清www| 精品一品国产午夜福利视频| 日本猛色少妇xxxxx猛交久久| 80岁老熟妇乱子伦牲交| 欧美大码av| 欧美黑人欧美精品刺激| 久久精品久久精品一区二区三区| 久久亚洲国产成人精品v| 亚洲av片天天在线观看| 18在线观看网站| 精品亚洲乱码少妇综合久久| 中国国产av一级| 精品久久久久久久毛片微露脸 | 国产片特级美女逼逼视频| 99香蕉大伊视频| 国产淫语在线视频| 中文字幕高清在线视频| 一级,二级,三级黄色视频| 人人妻,人人澡人人爽秒播 | av欧美777| 男男h啪啪无遮挡| 这个男人来自地球电影免费观看| 男女午夜视频在线观看| 久久久久久久久免费视频了| 国产免费福利视频在线观看| 国产欧美日韩一区二区三区在线| 男女边吃奶边做爰视频| 黑丝袜美女国产一区| 国产亚洲av高清不卡| 欧美黄色淫秽网站| 一二三四社区在线视频社区8| 国产片特级美女逼逼视频| 亚洲欧洲国产日韩| 宅男免费午夜| 不卡av一区二区三区| av福利片在线| 亚洲人成网站在线观看播放| 人妻人人澡人人爽人人| 一区在线观看完整版| 久久亚洲精品不卡| 丝袜美足系列| 青草久久国产| 精品视频人人做人人爽| 中文字幕高清在线视频| 只有这里有精品99| 久久国产精品男人的天堂亚洲| 免费一级毛片在线播放高清视频 | 一级毛片黄色毛片免费观看视频| 美女视频免费永久观看网站| 欧美中文综合在线视频| 大陆偷拍与自拍| 老汉色∧v一级毛片| 午夜久久久在线观看| 99精国产麻豆久久婷婷| 国产一级毛片在线| 免费av中文字幕在线| 美女脱内裤让男人舔精品视频| 久久久久久免费高清国产稀缺| 高清av免费在线| 国产男女超爽视频在线观看| 婷婷色av中文字幕| √禁漫天堂资源中文www| 亚洲九九香蕉| 女人被躁到高潮嗷嗷叫费观| 激情五月婷婷亚洲| 男女之事视频高清在线观看 | 国产精品成人在线| av欧美777|