The improvement of low cost, efficient photovoltaic devices is a leading technological challenge in the recent decade. There is a need to develop scalable and high-throughput manufacturing techniques that could reduce costs and improve manufacturing of chalcogenide solar cells. Copper, indium, gallium, and selenium (CIGS) Thin films polycrystalline heterojunction solar cells appear to be most appropriate with to cost and ease of manufacture. Currently Cu (In,Ga) (Se, S)2 materials hold the highest record cell efficiency of 22.3% in laboratory scale for thin films solar cells and the efficiency still be boosted by improving the different layers of the photovoltaic devices. CIGS chalcogenide absorber layers has been a leading candidate material in photovoltaic devices for thin films solar cells and space applications due to its unique optical-electronic properties as well as its radiation resistance. In the present work, thin films of Cu (In, Ga) (Se, S)2 were deposited at room temperature on glass substrates coated with ITO and Mo by electrodeposition techniques. The obtained polycrystalline thin films were characterized by UV-Vis spectroscopy, X-ray diffraction (XRD), scanning electron microscopy (SEM), atomic force microscopy (AFM), transmission electron microscopy (TEM) and energy dispersive spectroscopy (EDS) analysis. Thin films of Cu (In, Ga) (Se, S)2 grown by electrodeposition were subsequently processed into several sets of conditions including vacuum heat treatment, heat treatment in the presence of selenium or sulfur, heat treatment in nitrous gas atmosphere (N2H2) at different temperature and processing times. To improve the composition and the crystalline structure of the thin layers and to optimize the electro-optical properties a heat treatment of the thin films was developed in two stages after the electrodeposition. It was observed that the first annealing step (heating treatment at 450 °C in a selenium atmosphere 40 minutes) produced an appreciable improvement in the crystalline structure in the thin layer composition. In a second stage a sulfurization of the CuGaSe2 films was performed at 400 °C for 10 min in the presence of molecular sulfur and under the forming gas atmosphere. The effect of sulfurization was the complete conversion of selenium to sulfur and, therefore, the transformation of CuGaSe2 into CuGaS2. The formation of CuGaS2 thin films was evidenced by the by the displacement of the diffraction peaks of the CuGaSe2 towards higher angles to which makes the X-Ray diffraction 18 pattern which makes it coincide with the diffraction pattern of the CuGaSe2 films, and by the shift towards the blue (higher energies) of the optical gap. The optical gap found for the CuGaSe2 layer was 1.66 eV, while the optical gap for the CuGaS2 was raised up to 2.2 eV. CdS thin films have been widely used as buffer layer in CIGS solar cells. However, when alloyed with Zn, ZnCdS can still improve its performance as buffer layer. ZnCdS can be used as buffer and as window material in photoconductive devices and in heterojunction thin film solar cells due the possibility to tune the bandgap with the content of Zn. The band spacing of this ternary material can be from 2.42 to 3.50 eV, depending on the Cd/Zn ratio. / La obtención de dispositivos fotovoltaicos más eficientes y de bajo coste es uno de los desafíos tecnológicos más importantes de las últimas décadas. Existe la necesidad de desarrollar técnicas de fabricación escalables y de alto rendimiento que puedan reducir los costos y mejorar la fabricación de células solares de capa fina. Las células solares de heterounión de capas finas de seleniuro (o sulfuro) de cobre, indio y galio (CIGS) parecen estar bien adaptadas lograr este reto debido a su bajo costo, facilidad de fabricación y elevado rendimiento de los dispositivos. En la actualidad, Cu(In, Ga)Se2 ostenta el record de eficiencia de células solares con 22,3% a escala de laboratorio y esta eficiencia todavía puede ser acrecentada si se mejoran las diferentes capas de los dispositivos fotovoltaicos. Además, las capas absorbedoras de calcogenuros CIGS son un material candidato importante en dispositivos fotovoltaicos para capas delgadas celdas solares para aplicaciones espaciales debido a sus propiedades electrónicas, así como a su resistencia a la radiación. En el presente trabajo, las películas delgadas de Cu(In, Ga)(Se, S)2 se depositaron a temperatura ambiente sobre sustratos de vidrio recubiertos con ITO y Mo mediante técnicas electroquímicas. Las películas finas policristalinas obtenidas se caracterizaron por espectroscopia óptica UV-Vis, difracción de rayos X (XRD), microscopía electrónica de barrido (SEM), microscopía de fuerza atómica (AFM), microscopía electrónica de transmisión (TEM) y espectroscopia de energía dispersiva (EDS). Las películas finas de Cu(In, Ga)(Se, S)2 crecidas por electrodeposición se procesaron posteriormente en varios conjuntos de condiciones que incluían tratamiento térmico en vacío, tratamiento térmico en presencia de selenio o de azufre, tratamiento térmico en atmósfera gas nidrón (N2H2) a diferentes temperaturas y tiempos de procesado. Para mejorar la composición y la estructura cristalina de las capas finas y para optimizar las propiedades electro-ópticas se desarrolló un tratamiento térmico de las películas finas en dos etapas posterior a la electrodeposición. Se observó que la primera etapa de recocido (tratamiento térmico a 450 ºC en una atmósfera de selenio durante 40 minutos) producía una mejora apreciable en la estructura cristalina y en la composición de la capa fina. 20 En una segunda etapa se realizó una sulfuración de las películas de CuGaSe2 se realizó a 400 °C durante 10 min en presencia de azufre molecular y bajo la atmósfera reductora de gas nidrón. El efecto de la sulfuración fue la completa conversión del selenio en azufre y, por tanto, la transformación de CuGaSe2 en CuGaS2. La formación de películas delgadas de CuGaS2 se evidenció por el desplazamiento de los picos de difracción de las capas de CuGaSe2 hacia ángulos más altos hasta lo que hace que el patrón de difracción de rayos X lo que hace que coincida con el patrón de difracción del CuGaS2 y por el desplazamiento hacia el azul (energías más altas) del gap óptico. El gap óptico encontrado para las capas de CuGaSe2 era de 1,66 eV, mientras que el gap óptico para las capas de CuGaS2 se elevó hasta 2,2 eV. Las películas delgadas de CdS se han utilizado ampliamente como capa tampón en células solares CIGS. Sin embargo, cuando se alea con Zn, para formar el ternario ZnCdS, todavía puede mejorar su rendimiento como capa buffer. ZnCdS puede utilizarse como tampón y como ventana óptica en dispositivos fotoconductores y en células solares de capa fina de heterounión debido a la posibilidad de ajustar el bandgap con el contenido de Zn. / L'obtenció de dispositius fotovoltaics més eficients i més barats és un dels reptes tecnològics més importants de les últimes dècades. Hi ha la necessitat de desenvolupar tècniques de fabricació que siguen escalables i d'alt rendiment i que permeten reduir els costos de fabricació i millorar el rendiment de les cèl·lules solars de capa fina. Les cèl·lules solars de heterounió de capes fines de seleniur (o sulfur) de coure, indi i gal·li (CIGS) semblen estar ben adaptades per assolir aquest repte degut a del seu baix cost, facilitat de fabricació i elevat rendiment dels dispositius. En l'actualitat, el Cu(In, Ga)Se2 ostenta el rècord d'eficiència de cèl·lules solars amb 22,3% a escala de laboratori i aquesta eficiència encara pot ser augmentada si es milloren les característiques de les diferents capes dels dispositius fotovoltaics. Les capes absorbidores de calcogenurs CIGS són un candidat important per dispositius fotovoltaics per a pel·lícules primes en cel·les solars i aplicacions espacialles degut a les seues propietats electròniques així com a la seua resistència a la radiació. En el present treball, les pel·lícules primes de Cu(In, Ga)(Se, S)2 es van dipositar a temperatura ambient sobre substrats de vidre recoberts amb ITO i Mo mitjançant tècniques electroquímiques. Les pel·lícules fines policristal·lines obtingudes es van caracteritzar per espectroscòpia òptica UV-Vis, difracció de raigs X (XRD), microscòpia electrònica de rastreig (SEM), microscòpia de força atòmica (AFM), microscòpia electrònica de transmissió (TEM) i espectroscòpia d'energia dispersiva (EDS). Les pel·lícules fines de Cu(In, Ga)(Se, S)2 crescudes per electrodeposició es van processar posteriorment en diversos conjunts de condicions que incloïen tractament tèrmic en buit, tractament tèrmic en presència de seleni o de sofre, tractament tèrmic en atmosfera reductora de gas nidró (N2H2) a diferents temperatures i temps de processat. Per millorar la composició i l'estructura cristal·lina de les capes fines i per optimitzar les propietats electro-òptiques es va desenvolupar un tractament tèrmic de les pel·lícules fines en dues etapes posterior a la electrodeposició. Es va observar que la primera etapa de recuit (tractament tèrmic a 450 º C en una atmosfera de seleni durant 40 minuts) produïa una millora apreciable en l'estructura cristal·lina i en la composició de la capa fina. 24 En una segona etapa es va dur a terme una sulfuració de les pel·lícules de CuGaSe2 que es va realitzar a 400 °C durant 10 min en presència de sofre molecular i sota l'atmosfera reductora de gas nidró. L'efecte de la sulfuració va ser la completa conversió seleni en sofre i, per tant, la transformació de CuGaSe2 a CuGaS2. La formació de pel·lícules primes de CuGaS2 es va evidenciar pel desplaçament dels pics de difracció de les capes de CuGaSe2 cap angles més alts fins el que fa que el patró de difracció de raigs X el que fa que coincideixi amb el patró de difracció del CuGaS2 i pel desplaçament cap al blau (energies més altes) del gap òptic. El gap òptic trobat per a les capes de CuGaSe2 era de 1,66 eV, mentre que el gap òptic per a les capes de CuGaS2 es va elevar fins a 2,2 eV. Les pel·lícules primes de CdS s'han utilitzat àmpliament com a capa amortidora en cèl·lules solars de CIGS. No obstant això, quan s'alea amb Zn per formar ZnCdS encara pot millorar el seu rendiment com a capa d'amortiment. ZnCdS pot utilitzar-se com capa tampó i com a finestra òptica en dispositius fotoconductors i en cèl·lules solars de pel·lícula fina d'heterounió degut a la possibilitat d'ajustar el seu bandgap que depoen del contingut de Zn. / Ullah, S. (2017). THIN FILM SOLAR CELLS BASED ON COPPER-INDIUMGALIUM SELENIDE (CIGS) MATERIALS DEPOSITED BY ELECTROCHEMICAL TECHNIQUES [Tesis doctoral no publicada]. Universitat Politècnica de València. https://doi.org/10.4995/Thesis/10251/86290 / TESIS

Electronic and optical properties of semiconducting nanocrystals, that can be engineered and manipulated by various ways like varying size, shape, composition, structure, has been a subject of intense research for more than last two decades. The size dependency of these properties in semiconductor nanocrystals is direct manifestation of the quantum confinement effect. Study of electronic and optical properties in smaller dimensions provides a platform to understand the evolution of fundamental bulk properties in the semiconductors, often leading to realization and exploration of entirely new and novel properties. Not only of fundamental interests, the semiconductor nanocrystals are also shown to have great technological implications in diverse areas. Besides size tunable properties, introduction of impurities, like transition metal ions, gives rise to new functionalities in the semicon-ductor nanocrystals. These materials, termed as doped semiconductor nanocrystals, have been the subject of great interest, mainly due to the their interesting optical properties. Among different transition metal doped semiconductor nanocrystals, manganese doped systems have drawn a lot on attention due to their certain advantages over other dopants. One of the major advantages of Mn doped semiconductor nanocrystals is that they do not suffer from the problem of self-absorption of emission, which quite often, is consid-ered detrimental in their undoped counterparts. The doped nanocrystals are known to produce a characteristic yellow-orange emission upon photoexcitation of the host that is relatively insensitive to the surface degradation of the host. This emission, originating from an atomic d-d transition of Mn2+ ions, has been a subject of extensive research in the recent past. In spite of the spin forbidden nature of the specific d-d transition, namely 6A1 −4 T1, these doped nanocrystals yield intense phosphorescence. However, one major drawback of utilizing this system for a wide range application has been the substantial inability of the community to tune the emission color of Mn-doped systems in spite of an intense effort over the years; the relative constancy of the emission color in these systems has been attributed to the essentially atomic nature of the optical transition involving localized Mn d levels. Interestingly, however, the Mn emission has a very broad spectral line-width in spite of its atomic-like origin. While the long (∼ 1 ms) emission life-time of the de-excitation process is well-studied and understood in terms of the spin and orbitally forbidden nature of the transition, there is little known concerning the process of energy transfer to the Mn from the host in the excitation step. In this thesis, we have studied the ultrafast dynamic processes involved in Mn emission and addressed the issues related to its tunability and spectral purity. Chapter 1 provides a brief introduction to the fundamental concepts relevant to the studies carried out in the subsequent chapters of this thesis. This chapter is started with a small preview of the nanomaterials in general, followed by a discussion on semiconducting nanomaterials, evolution of their electronic structure with dimensions and size as well as the effect of quantum confinement on their optical properties. As all the semiconducting nanomaterials studied in the thesis are synthesized via colloidal synthesis routes, a separate section is devoted on colloidal semiconducting nanomaterials, describing various ways of modifying or tuning their optical properties. This is followed by an introduction to the important class of materials “doped semiconductor nanocrystals”. With a general overview and brief history of these materials, we proceed to discuss about various aspects of manganese doped semiconductor nanocrystals in great details, highlighting the origin of the manganese emission and the associated carrier dynamics as well as different reported synthetic strategies to prepare these materials. The chapter is closed with the open questions related to manganese doped semiconductor nanocrystals and the scope of the present work. Chapter 2 describes different experimental and theoretical methods that have been employed to carry out different studies presented in the thesis. It includes common experimental techniques like UV-Vis absorption spectroscopy, steady-state and time-resolved photoluminescence spectroscopy used for optical measurements, X-ray diffraction, trans-mission electron microscopy and atomic absorption spectroscopy used for structural and elemental analysis. Experimental tools to perform special studies like transient absorption and single nanocrystal spectroscopy are also discussed. Finally, theoretical fitting method used to analyse various spectral data has been discussed briefly. Chapter 3 deals with the dynamic processes involved in the photoexcitation and emission in manganese doped semiconductor nanocrystals. For this study, Mn doped ZnCdS alloyed nanocrystal has been chosen as a model system. There are various radiative and nonrdiative recombination pathways of the photogenerated carriers and they often compete with each other. We have studied the dynamics of all possible pathways of carrier relaxation, viz. excitonic recombination, surface state emission and Mn d-d transition. The main highlight of this chapter is the determination of the time-scale to populate surface states and the Mn d-states after the photoexcitation of the host. Employing femtosecond pump-probe based transient absorption study we have shown that the Mn dopant states are populated within sub-picosecond of the host excitation, while it takes a few picoseconds to populate the surface states. Keeping in mind the typical life-time of the excitonic emission (∼ a few ns), the ultra-fast process of energy transfer from the host to the Mn ions explains why the presence of Mn dopant ions quenches the excitonic as well as the surface state emissions so efficiently. Chapter 4 presents a study of manganese emission in ZnS nanocrystals of different sizes. By varying the size of the ZnS host nanocrystal, we show that one can tune the Mn emission over a limited range. In particular, with a decrease in host size, the Mn emission has been observed to red-shift. We have attributed this shift in Mn emission to the change in the ratio of surface to bulk dopant ions with the variation of the host size, noting that the strength of the ligand field at the Mn site should depend on the position of the Mn ion relative to the surface due to a systematic lattice relaxation in such nanocrystals. The ligand field affects the emission wavelength directly by controlling the splitting of the t2 and e levels of Mn2+ ions. The surface dopant ions experience a strong ligand field due to distorted tetrahedral environment which leads to larger splitting of these t2 and e states. We further corroborated these results by performing doping concentration dependent emission and life-time studies. In Chapter 5 addresses two fundamental challenges related to manganese photolumines-cence, namely the lack of a substantial emission tunability and presence of a very broad spectral width (∼ 180-270 meV). The large spectral width is incompatible with atomic-like manganese 4T1 −6 A1 transition. On the other hand, if this emission is atomic in nature, it should be relatively unaffected by the nature of the host, though it can be manipulated to some extent as discussed in Chapter 3. The lack of Mn emission tunability and spectral purity together seriously limit the usefulness of Mn doped semiconductor nanocrystals. To understand why the Mn emission tunability range is very limited (typically 565-630 nm) and to understand the true nature of this emission, we carried out single nanocrystal imaging and spectroscopy on Mn doped ZnCdS alloyed nanocrystals. This study reveals that Mn emission, in fact, can vary over a much wider range (∼ 370 meV) and exhibits widths substantially lower (∼ 60-75 meV) than reported so far. We explained the occur-rence of Mn emission in this broad spectral range in terms of the possibility of a large number of symmetry inequivalent sites resulting from random substitution of Cd and Zn ions that leads to differing extent of ligand field contributions towards the splitting of Mn d-levels. The broad Mn emission observed in ensemble-averaged measurements is the result of contribution from Mn ions at different sites of varying ligand field strengths inside the NC. Chapter 6 presents a synthetic strategy to strain-engineer a nanocrystal host lattice for a controlled tuning of the ligand field effect of the doped Mn sites. It is realized synthesizing a strained quantum dot system with the structure ZnSe/CdSe/ZnSe. A larger lattice parameter of CdSe compared to that of ZnSe causes a strain field that is maximum near the interface, gradually decreasing towards the surface. We control the positioning of Mn dopant ions at different distances from the interface, thereby doping Mn at different predetermined strain fields. With the help of this strain engineering, we are able to tune Mn emission across the entire range of the visible spectrum. This strain induced tuning of Mn emission is accompanied by life-times that is dependent on the emission energy which has been explained in terms of perturbation effect on the Mn center due to the strain generated inside the quantum dot. The spectacular emission tuning has been explained by modelling the quantum dot system as an elastic continuum containing three distinct layers under hydrostatic pressure. From this modelling, we found that the strain is max-imum at the interface and decreases continuously as one goes away from the interface. We also show that the Mn emission maximum red shifts with increasing distance of the dopants from the maximum strained region. In summary, we have performed a study on the photophysical processes in manganese doped semiconductor nanocrystals. We have emphasized in understanding of different dynamic processes associated with the manganese emission and tried to understand the true nature of manganese emission in a nanocrystal. This study has brought out some new aspects of manganese emission and opened up possibilities to tune and control manganese emission by proper design of the host material.