Open access peer-reviewed chapter - ONLINE FIRST

III-Nitride Nanowires: Future Prospective for Photovoltaic Applications

By Soumyaranjan Routray and Trupti Lenka

Submitted: June 9th 2020Reviewed: November 13th 2020Published: December 7th 2020

DOI: 10.5772/intechopen.95011

Downloaded: 56


Photovoltaic (PV) technology could be a promising candidate for clean and green source of energy. The nanowire technology provides extra mileage over planar solar cells in every step from photon absorption to current generation. Indium Gallium Nitride (InxGa1-xN) is a recently revised material with such a bandgap to absorb nearly whole solar spectrum to increase the conversion efficiency copiously. One of the major technological challenge is in-built polarization charges. This chapter highlights the basic advantageous properties of InxGa 1−xN materials, its growth technology and state-of-the-art application towards PV devices. The most important challenges that remain in realizing a high-efficiency InxGa 1−xN PV device are also discussed. III-Nitride nanowires are also explored in detail to overcome the challenges. Finally, conclusions are drawn about the potential and future aspect of InxGa 1−xN material based nanowires towards terrestrial as well as space photovoltaic applications.


  • III-nitride
  • polarization charges
  • efficiency
  • InGaN/GaN
  • nanowires
  • stress
  • strain

1. Introduction

Photovoltaic (PV) technology is the most emerging way of harnessing huge amount of energy from sun light as compared to solar thermal and photo electrochemical cells [1]. PV devices convert incident photons from sunlight to electricity upon exposed to light. PVs are popular because of its compactness and can be used anywhere for different application [2]. Additionally, involvement of nanostructures further boost the performance of solar cell. Over the past decade, nanostructured solar cell has become hot topics within research community due to its potential to enhance the spectral response of cell. Although, first generation silicon wafer based solar cell leads the current global PV market, however this conventional technology do not have any further scope to improve efficiency and reduce cost [3]. Additionally, it is also not recommended to use Silicon based solar cell for space application due to its low radiation tolerance. Second generation thin film technology such as hydrogenated amorphous silicon (a-Si: H), CIGS, and CdTe could not line-up with wafer-based silicon due to use of rare earth elements and low stability [4, 5]. Furthermore, highly efficient compound semiconductors based third generation solar cell have a demerit of high cost which limits its use in terrestrial applications. Hence, the hunt for low cost high performance solar cell are still unachievable. In the meantime, involvement of nanotechnology could bring a ray of hope for future generation solar cell. Nanowire (NW) geometry has remarkable advantages over planner geometry due to optical, electrical, and mechanical effects. New charge separation mechanisms, low defects and low cost also add more mileage to this journey. Looking towards the current scenario, existing PV technologies aren’t the solid foundation for the future projection of the renewable energy generation. None of the existing technology can satisfy global energy demand in future [2, 5]. Moreover, if the material or technological limitations restrict the future roadmap of PV technology, then the incorporation of new efficient materials and transpose of technology will be an assurance against high cost and low efficiency solar cells. Newly explored InxGa1-xN material brings an bunch of opportunities for future PV technology, having capability to absorb full solar spectrum using a single absorber material. One of the major properties of InGaN material is its tunable bandgap from 0.6 to 3.4 eV by changing ‘In’ content [6, 7, 8, 9, 10]. It also has easy growth of nanowire and nanorod structures with proven technology [11, 12, 13, 14]. It is a direct bandgap material where photon absorption and direct interband transition can be occurred without interference of phonons to conserve momentum. Additionally, high absorption coefficient of 105 is an additional benefit for good absorption with thin layer. Hence the cost can be minimized as well as recombination rate can also be minimized. InGaN also possess a high saturation velocity and a low effective mass of charge carriers, which ensures the more carrier separation along the junction. High radiation tolerance of InGaN are always appreciated for harsh environments. Moreover, InGaN solar cell do not contain any toxic elements such as arsenic, cadmium or phosphorous as used in MJ solar cell. Thus, it is evident that InxGa 1−xN is an extremely allegiant PV material that can enable several photovoltaic devices [15, 16]. It is required to explore state-of-art of different InGaN based PV technologies and new possibilities of InGaN as a hopeful material for future technology [17, 18]. Hence, in this chapter a scope of III-Nitride and its progress with nanostructures have been discussed in order to explore more on future generation solar cell.

2. Planar, nanodisk and nanowire III-nitride solar cells

In the present context mainly different geometry of III-Nitride GaN/InGaN material based solar cell are considered, such as planar, nanodisk and nanowire types. Theoretically, it is anticipated that power conversion efficiency more than 40% could be achievable with GaN/InGaN junctions [19, 20]. However, practically achievable efficiency is quite low [21, 22]. One of the major challenges is the association of in-house defects with InGaN layer at higher ‘In’ content. Which in turn leads to stuck of immobile charges (known as polarization charges) along interfaces and reduces minority lifetime. Recently III-Nitride nanowires (NWs) are proposed as stand-alone PV devices due to enhanced light trapping, defect and stress-free growth [23, 24]. In general, two widely used structure for nanowire solar cell are (i) axial junction and (ii) radial junction. Axial junction is also known as nanodisk (ND) whereas radial junction is known as core-shell-shell (CSS) solar cell. Vapor–liquid–solid (VLS) technique is one of the popular methods to grow the GaN/InGaN nnaowires [23]. The fabricated NWs have hexagonal cross-section with {0001} orientation of top facet and {1–100}/ {10–10} orientation alongside walls of NWs [23]. Literature shows the comparative analysis of planar and circular NWs reported by Y. Zeng et al. [25] and B.M. Kayes et al. [26] with achievable conversion efficiency of more than 33% and 50% for Si and GaAs respectively. Additionally, ND and NW SCs are reported by Christesen et al. [27], which shows comparative better performance in CSS-NW SCs. The analysis in literature taken circular cross-section into consideration for NWs but in practice, III-Nitride NWs possess either hexagonal or triangular cross-section. Hence, in this chapter, a scope has been taken to analyze the CSS-NW and ND type SCs with hexagonal crystallographic orientations as per the fabricated devices. The chapter also emphasis on effect of polarization induced electric field with a different ‘In’ compositions of InxGa1-xN. The schematic of planar, ND and CSS-NW SCs as shown in Figure 1 and simulated using VICTORY 3D Luminous TCAD. Optical and electrical properties are solved using Poisson’s equation, drift diffusion, and photo generation-recombination models. All the structures are designed with n/i/p junctions, which helps to reverse the electric field and match with polarization-induced electric field [28, 29]. A uniform 40 nm and 100 nm thickness are taken for n- and p-GaN layer of three structures. Thin Ni/Au (5 nm/5 nm) layer is used as contact for all three considered cells. Incorporation of Ni layer may reduce series resistance and hence enhance fill factor (FF) of the solar cell. The thickness of intrinsic InGaN layer is varied from 6 nm to 200 nm to optimize the thickness in planar, ND and CSS-NW solar cell. The surface recombination velocity of 105 cm/s is taken into consideration for all three structure. The minority carrier lifetime is as follows [29].

Figure 1.

Schematics of n-i-p heterojunctions with (a) planar (b) nanodisk (ND) and (c) CSS-NW based solar cell [29].


Where σn/pis the capture cross sections of electron or hole, thermal velocity of carriers, ϑthermal(≈107cm/s), the defect density (cm−2), Ndefect, electron capture coefficient for acceptor or donor, Cn/p, and nis the free electron concentrations.

All the material parameters for GaN and InGaN with different compostion can be found from [30]. The interpolation method is used to calculate all parameters for InxGa1-xN composite alloys. Defect density in the order of 1017, 1014 and 1012 are incorporated for planar, ND and CSS-NW SCs respectively [31].

The model developed by Romanov et al. [32] and Mastro et al. [33] are implemented here to calculate polarization charges along InGaN/GaN heterointerfaces and is expressed as,


Where PLspandPTspare spontaneous polarizations for top and bottom layer respectively, PLzpzis the piezoelectric polarization along the interface which solely depends on strain profile, φis the angle between planes and basal plane. Angle φis considered as 0° for polar {0001} facet and 90° for nonpolar {1–100}/{10–10} facets [33]. Finally, material parameters are incorporated into VICTORY 3D Luminous TCAD to simulate solar cell.

Vertical illumination of light source on the front surface of the device is consider during all analysis as shown in Figure 1. Transport of carriers and separation mechanisms in the device depends solely on its geometrical structure. Here, carrier transport in planar, ND and NW type solar cell are explored with the help of energy band diagram. Figure 2(a) shows that tilt of energy band along i-InGaN region is not in favor of carrier collection due to detrimental polarization effect along {0001} orientation of planar Solar cell. Similarly, ND type solar cell also suffers from polarization effect due to axial growth along {0001} orientation. Hence height of barrier along the junction increases in case of planar and ND solar cell as shown in Figure 2. High potential barrier hinders the diffusion of photogenerated carriers to either sides of the contact. Consequently, carrier collection degrades along {0001} interface. Similarly, potential valley is also observed next to barrier along the interfaces, which stocks carriers leading towards low collection.

Figure 2.

Energy band diagram of (a) planar (b) ND and (c) CSS-NW solar cell at 100 nm, 150 nm, and 180 nm i-InGaN thickness respectively.

Thus, with increase in bias voltage, photogenerated carriers accumulate inside the potential valley rather than traveling in i-region. In contrast, CSS-NW type solar cells do not show this effect because of radial separation of carriers. Polarization charges have negligible effect on CSS-NW due to nonpolar facets as shown in Figure 2(c). The inclination energy band in CSS-NW solar cell is in favor of carrier collection. Potential barriers are less as shown in Figure 2(c). Hence a hassle-free movement of carriers is possible in CSS-NW solar cell.

Figure 3 shows dependency of short-circuit current density (Jsc) on ‘In’ composition and thickness of i-InGaN absorber layer. In planar structure, diffusion length carriers are quite low due to high density of defects, which consequently leads to a poor Jsc. Thus, higher thickness of i-InGaN do not contribute more towards current due to low diffusion length of carriers. It is also observed that increase in ‘In’ composition leads to higher polarization charges [24], which also block some of the diffused carriers before collection. Thus Jscshows a poor performance at higher ‘In’ fraction as shown in Figure 3. However, Jscis high in radial junctions as compared to axial junctions. In order to interpret this result, Shockley diode equation is considered for short circuit current as

Figure 3.

Short circuit current density (Jsc) at 10%, 20%, and 30%, ‘In’ content for (a) planar (b) Nanodisk and (c) CSS-NW solar cell.


Where volume of the absorption region is, Vactive, photo-generation rate, grand position vector is given by a. The optical photo generation rate, gris considered as constant g across the entire NW solar cell, which simplifies the complexity of the model.

Thus Jsccan be expressed as


Where, active absorption layer is, Lactive.It is noteworthy to mention that due to the structural advantages, CSS-NW possess more than two-fold enhancement in active absorption region, which in turn support more photon absorption and high current. Therefore, it is observed that Jscis quite enhanced in CSS-NW case as compared to ND and planar counterparts. It is due to the high absorption region of CSS structure and higher diffusion length of carriers. Depending on the structural advancement, carrier diffusion length, and lifetime, an optimized 180 nm, 150 nm and 100 nm active layers are obtained for CSS-NW, ND and planar structure respectively as given in Figure 3.

Figure 4 shows the current density-voltage-power density (J-V-P) curve of n-GaN/i-In0.1Ga0.9N/p-GaN planar, ND and NW type solar cell. The optimized thickness of 100 nm, 150 nm and 180 nm i-InGaN is considered for all performance analysis. It shows a higher Jsc in CSS-NW as compared to ND and planar structure. It is anticipated that higher current in CSS-NW solar cell is mainly due to higher active absorption region and efficient carrier separation. It is important to highlight that planar and ND type solar cells shows a stair-case type J-V curve, which is not there in CSS-NW. It is may be due to low degree of strain relaxation or higher stress generation along the interface which is again related to structural issues of device. Hence, it is always important to engineer the device structure as per the material properties of the absorber layer. High defect density along the interface is also play a major role for low current in planar and ND solar cell. CSS-NW do not possess a staircase J-V curve due to low defect density, low stress and high degree of strain relaxation. It is also observed that the depth of stair-case in J-V curve is increasing with higher ‘In’ contents. Additionally, higher Jsc value of 2.82 mA/cm2 is noted in CSS-NW solar cell (Figure 5).

Figure 4.

Open circuit voltage, Voc at 10%, 20%, and 30%, ‘In’ content for (a) planar (b) Nanodisk and (c) CSS-NW solar cell.

Figure 5.

Current density (black line) – Voltage – Power density (red line) of (a) planar (b) ND and (c) CSS-NW solar cell at 100 nm, 150 nm, and 180 nm i-InGaN thickness respectively.

It is also observed that due to high degree of strain relation, low defects density and more active area of absorption, CSS-NW structure can accommodate higher thickness of active InGaN layer (W) region. Moreover, higher thickness of absorber enhances the probability of more absorption of photons from sunlight. In other hand, active region of planar and ND type solar cells cannot be increased due to are limitation of surface recombination arte, polarization induced electric field, low degree of strain relaxation and defect density. Voc of ND type solar cell is seen to be higher than CSS-NW type solar cell which is may be due to the recombination rate along the junction. However, the rate of increase in Jsc of CSS-NW structure is comparatively higher than ND and planar solar cell. Similarly, planar solar cell possesses a low as compared to ND and NW solar cell. It is mainly due to appearance of staircase type J-V curve, which in turn reduces maximum power (Pm) of solar cell. Finally, achievable conversion efficiency (η) of CSS-NW structure is increased by more than 0.5-fold and 2.5-fold, compared to ND and planar type solar cells respectively. More analysis on different types of CSS nanowire is also studied and can found in [34, 35, 36].

η (%)
Nanodisk (ND)1501.932.5287.64.28
CSS-Nanowire (NW)1802.842.4791.66.46

3. Conclusion

In this chapter, the importance of nanowire solar cell with III-Nitride material is explored in a detailed manner. A comparative analysis is carried out with planar, nanodisk and nanowire type solar cell and concluded that nanowire type structure shows a better performance as compared to others. Additionally, it is found that nanowires in InGaN materials are grown either in triangular or hexagonal orientation. The strain relaxation is more in CSS-nanowires which in turns leads to low in-house defect density along the interfaces. CSS-NWs are also able to accommodate higher thickness of intrinsic material due to high carrier diffusion length. Radial separation of carriers also provides more surface area and better control on carrier separation mechanisms. Hence, it is concluded that radial growth of nanowire provides a broad range of opportunity for performance enhancement of solar cell. The similar type of observation are also applicable to LASER and light emitting diodes, where III-Nitride materials are used.


The authors acknowledge Dept. of Science and Technology, Govt. of India for financial support for providing the instrumental facility under DST-FIST in Dept. of ECE, SRM Institute of Science and Technology, Chennai, India.

The authors also acknowledge Visvesvaraya PhD Fellowship of MeitY, Govt. of India and TEQIP-II for procurement of Silvaco TCAD tool in Department of ECE, NIT Silchar for carrying out the research work.

Conflict of interest

The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this chapter.

Appendices and nomenclature

InGaNindium gallium nitride
GaNgallium nitride
CIGScopper indium gallium selenide
CdTecadmium telluride

Download for free

chapter PDF

© 2020 The Author(s). Licensee IntechOpen. This chapter is distributed under the terms of the Creative Commons Attribution 3.0 License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

How to cite and reference

Link to this chapter Copy to clipboard

Cite this chapter Copy to clipboard

Soumyaranjan Routray and Trupti Lenka (December 7th 2020). III-Nitride Nanowires: Future Prospective for Photovoltaic Applications [Online First], IntechOpen, DOI: 10.5772/intechopen.95011. Available from:

chapter statistics

56total chapter downloads

More statistics for editors and authors

Login to your personal dashboard for more detailed statistics on your publications.

Access personal reporting

We are IntechOpen, the world's leading publisher of Open Access books. Built by scientists, for scientists. Our readership spans scientists, professors, researchers, librarians, and students, as well as business professionals. We share our knowledge and peer-reveiwed research papers with libraries, scientific and engineering societies, and also work with corporate R&D departments and government entities.

More About Us