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Showing 11 to 14 of 14 (0.111 seconds)| 11 |
Computational Studies on Interstellar Molecular Species : From Formation to DetectionEtim, Emmanuel Edet January 2016 (has links) (PDF)
Initiated with the purpose of assigning the Fraunhofer lines in the solar spectrum to atomic transitions in the 18th century, the collaboration between spectroscopists and astrophysicists has remained fruitful, successful and ever fascinating. This collaboration has resulted in the unique detection of over 200 different molecular species in the interstellar medium (ISM). These interstellar molecular species play significant roles in diverse fields such as atmospheric chemistry, astrochemistry, prebiotic chemistry, astrophysics, astronomy, astrobiology, etc, and in our understanding of the solar system ''the world around us''. This Thesis work focuses on understanding of the different aspects of the chemistry of the various classes of these molecular species.
Chapter one starts with an historical perspective of what is now regarded as Molecular Astrophysics or Astrochemistry and discusses the interstellar medium and its properties; interstellar molecular species and their importance; molecular spectroscopy as an indispensible tool in interstellar chemistry and the different formation routes of these molecular species. It also discusses hydrogen bonding which is one of the most important of all the intermolecular interactions. The chapter ends by setting the stage for the present investigations.
The chapter two of the Thesis saddled with the task of describing the methodology employed in this Thesis begins by setting the stage on the importance of computational chemistry in interstellar chemistry. It discusses the Gaussian 09 suite of programs and the various theoretical methods used in all the quantum chemical calculations reported in this Thesis. The chapter ends with a brief summary on the homebuilt Pulsed Nozzle Fourier Transform Microwave (PN-FTMW) spectrometer used for the preliminary studies on Isoprene...Argon weakly bound complex reported in the appendix.
After the introductory chapters, chapter three begins with what is unarguably one of the most important classes of interstellar molecular species - 'interstellar isomers'. In this chapter, the Energy, Stability and Abundance (ESA) relationship existing among interstellar molecular species has been firmly established using accurate thermochemical parameters obtained with the composite models and reported observational data. From the relationship, “Interstellar abundances of related species are directly proportional to their stabilities in the absence of the effect of interstellar hydrogen bonding”. The immediate consequences of the relationship in addressing some of the questions in interstellar chemistry such as: Where are Cyclic Interstellar Molecules? What are the possible candidates for astronomical observation? Why are more Interstellar Cyanides than isocyanides? among others are briefly discussed. Following the ESA relationship, other studies addressing some of the whys and wherefores in interstellar chemistry are discussed in details. From ESA relationship, though there has not been any successful astronomical observation of any heterocycle, the ones so far searched remain the best candidates for astronomical observation in their respective isomeric groups. The observation of the first branched chain molecule in
ISM is in agreement with the ESA relationship and the C5H9N isomers have been shown to contain potential branched chain interstellar molecules. That molecules with the C-C-O backbone have less potential of formation in ISM as compared to their counterparts with the C-O-C backbone has been demonstrated not to be true following the ESA relationship. A detailed investigation on the relationship between molecular partition function and astronomical detection of isomeric species (or related molecules) shows that there is no direct correlation between the two rather there is a direct link between the thermodynamic stability of the isomeric species (or related molecules) and their interstellar abundances which influences the astronomical observation of some isomers at the expense of others.
Chapter four presents an interesting and a fascinating phenomenon among the interstellar molecular species as it discusses for the first time, the existence and effects of Interstellar Hydrogen Bonding. This interstellar hydrogen bonding is shown to be responsible for the deviations from thermodynamically controlled processes, delayed observation of the most stable isomers, unsuccessful observations of amino acids among other happenings in interstellar chemistry and related areas. On the prediction that ketenes are the right candidates for astronomical searches among their respective isomers, a ketenyl radical; HCCO has recently been detected in line with this prediction. The deviation from the rule that the ratio of an interstellar sulphur molecule to its oxygen analogue is close to the cosmic S/O ratio is well accounted for on the basis of hydrogen bonding on the surface of the dust grains. Detecting weakly bound complexes in ISM has not been a major interest in the field so far but the detectability of weakly bound complexes in ISM is very possible as discussed in this chapter. Following the conditions in which these complexes are observed in the terrestrial laboratory as compared to the ISM conditions; it suffices to say that weakly bound complexes are present and are detectable in ISM. They could even account for some of the 'U' lines.
Chapter five of the Thesis discusses the Linear Interstellar Carbon Chains which are the dominant theme in interstellar chemistry accounting for over 20% of all the known interstellar and circumstellar molecular species. Accurate spectroscopic parameters within experimental accuracy of few kHz which are the indispensable tools for the astronomical observation of these molecular species; are obtained for over 200 different species from the various chains using an inexpensive combined experimental and theoretical approach. With the availability of the spectroscopic parameters; thermodynamics is utilized in accounting for the known systems and in examining the right candidates for astronomical searches. These molecular species are shown to also obey the ESA relationship observed for the isomeric species discussed in chapter three of this work. The effect of kinetics on the formation processes of these molecular species is well controlled by thermodynamics as discussed in this chapter. Finally, the application of these studies in reducing the 'U' lines and probing new molecular species has been briefly summarized.
Chapter six discusses Interstellar Ions and Isotopologues which are two unique classes of interstellar molecular species. Different studies on interstellar ions and isotopologues are presented. From the studies on interstellar protonated species with over 100 molecular species; protonated species resulting from a high proton affinity prefers to remain protonated
rather than transferring a proton and returning to its neutral form as compared to its analogue that gives rise to a lower proton affinity from the same neutral species. The studies on detectable interstellar anions account for the known interstellar anions and predict members of the C2nO-, C2nS-, C2n-1Si-, HC2nN-, CnP-, and C2n chains as outstanding candidates for astronomical observation including the higher members of the C2nH- and C2n-1N- groups whose lower members have been observed. From high level ab initio quantum chemical calculations; ZPE and Boltzmann factor have been used to explain the observed deuterium enhancement and the possibility of detecting more deuterated species in ISM. Though all the heterocycles that have so far been searched for in ISM have been shown to be the right candidates for astronomical observation as discussed in the ESA relationship, they have also been shown to be strongly bonded to the surface of the interstellar dust grains thereby reducing their abundances, thus, contributing to their unsuccessful detection except for furan which is less affected by hydrogen bonding. The D-analogues of the heterocycles are shown from the computed Boltzmann factor to be formed under the dense molecular cloud conditions where major deuterium fractionation dominates implying very high D/H ratio above the cosmic D/H ratio which suggests the detectability of these deuterated species.
Chapter seven examines the isomerization of the most stable isomer (which is probably the most abundant) to the less stable isomer(s) as one of the plausible formation routes for interstellar molecular species. An extensive investigation on the isomerization enthalpies of 243 molecular species from 64 isomeric groups is reported. From the results, the high abundances of the most stable isomers coupled with the energy sources in interstellar medium drive the isomerization process even for relative enthalpy difference as high as 67.4 kcal/mol. Specifically, the cyanides and their corresponding isocyanides pairs appear to be effectively synthesized via this process. The following potential interstellar molecules; CNC, NCCP, c-C5H, methylene ketene, methyl Ketene, CH3SCH3, C5O, 1,1-ethanediol, propanoic acid, propan-2-ol and propanol are identified and discussed. In all the isomeric groups, isomerization appears to be an effective route for the formation of the less stable isomers (which are probably less abundant) from the most stable ones.
Chapter eight summarizes the conclusions drawn from the different studies presented in this Thesis and also highlights some of the future directions of these studies. The first appendix presents the preliminary study on Isoprene...Ar weakly bound complex while the second appendix contains a study on interstellar C3S describing the importance of accurate dipole moment in calculating interstellar abundances of molecular species and in astrophysical and astronomical models.
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Synthèse de tétrazoles oxabicycliques, leurs transformations en une vaste diversité de composés hétérocycliques fonctionnalisés et étude en DFT de l’équilibre tétrazole-azidoazométhine avec des motifs de types benzo- et pyrido- diazidodiazinesDeschênes-Simard, Benoît 12 1900 (has links)
Les tétrazoles ont une place importante dans la chimie médicinale contemporaine par leurs caractéristiques spatiales et électroniques uniques. Leur haute teneur en azote leur confère également des qualités requises dans le développement de substances explosives et de haute énergie. Le développement de nouveaux outils synthétiques pour les créer prend donc ici tout son sens.
Dans cet ouvrage, il est tout d’abord question d’une nouvelle méthode de synthèse qui génère des tétrazoles bicycliques en conditions douces par l’entremise d’azidonitriles aliphatiques séparés par trois ou quatre atomes de carbone (effet de proximité) et d’acides de Lewis. De plus, cette méthode de synthèse présente une réaction tandem qui génère des tétrazoles oxabicycliques 1,5-dialkylés via une cycloaddition 1,3-dipolaire diastéréosélective à partir d’azidoacétals ou d’azidocétals arborant un azoture proximal. La réaction s’effectue dans le nitrométhane de 0 °C à la température ambiante avec du TMSCN et est promue par une variété d’acides de Lewis dont le BF3OEt2. Les aspects mécanistiques de la réaction (l’ouverture des acétals, l’équilibre entre les éthers de cyanhydrine, la cycloaddition 1,3-dipolaire diastéréosélective et le réarrangement de Boyer-Schmidt-Aubé) ainsi que les paramètres réactionnels (solvants, acides de Lewis, stœchiométrie, sources de cyanure, etc.) seront en outre abordés.
Ensuite, le motif de tétrazole oxabicyclique a été l’objet de diversifications, de fonctionnalisations et de transformations afin d’en valoriser l’utilité. Des réactions d’alkylations, d’azoturations radicalaires, de bêta-éliminations et de diversifications de la chaîne latérale ont été étudiées. De ces mêmes motifs de tétrazoles, la synthèse de tétrazoles azabicycliques et celle de morpholines 2,6-polysubstituées ont aussi été investiguées. La synthèse d’un sel de tétrazolium et l’alkylation de 5-tétrazolyllithiums ont aussi fait l’objet d’études préliminaires.
Enfin, une étude théorique en DFT a été effectuée pour mieux comprendre l’équilibre tétrazole-azidoazométhine sur des motifs de types benzo- et pyrido- diazidodiazines parents à la 6-azidotétrazolo[5,1-a]phthalazine, un métabolite toxique du Gymnodinium breve (Ptychodiscus brevis, aussi actuellement connu sous le nom de Karenia brevis). Les aspects thermodynamiques, les états de transition, les orbitales HOMO, les cartes de potentiels d’ionisation locaux, les cartes de densité de la LUMO, les effets de solvant et certains paramètres permettant d’évaluer l’aromaticité (indices de Bird, ordres de liaison minimaux de Jug, indices HOMA et NICS) ont été considérés dans l’étude. Le constat a été que certaines des analyses théoriques peuvent constituer de bons outils prédictifs, particulièrement avec des considérations thermodynamiques, mais que cette approche a aussi ses limites qui sont principalement dues aux incertitudes inhérentes aux calculs théoriques. / Tetrazoles have an important place in contemporary medicinal chemistry due to their unique spatial and electronic characteristics. Their high nitrogen content also gives them the qualities required for the development of explosive and high energy substances. The development of new synthetic tools to create them takes here all its meaning.
Therefore, in this work, a new synthesis method that generates bicyclic tetrazoles under mild conditions using aliphatic azidonitriles separated by three or four carbon atoms (proximity effect) and Lewis acids will first be discussed. In addition, a tandem reaction which generates 1,5-dialkylated oxabicyclic tetrazoles via a diastereoselective 1,3-dipolar cycloaddition from azidoacetals or azidoketals bearing a proximal azide will also be disclosed. The reaction is carried out in nitromethane at 0 °C to room temperature with TMSCN and is promoted by a variety of Lewis acids including BF3OEt2. The mechanistic aspects of the reaction (acetal opening, equilibrium between cyanohydrin ethers, diastereoselective 1,3-dipolar cycloaddition and Boyer-Schmidt-Aubé rearrangement) as well as the reaction parameters (solvents, Lewis acids, stoichiometry, cyanide sources, etc.) will be discussed.
Furthermore, the oxabicyclic tetrazole unit was involved in diversifications, functionalizations and transformations to enhance its utility. Reactions of alkylations, radical azidations, beta-eliminations and diversifications of the side chain were applied. From these same tetrazole units, the synthesis of azabicyclic tetrazoles and that of 2,6-polysubstituted morpholines was also investigated. The synthesis of a tetrazolium salt and the alkylation of 5 tetrazolyllithiums were also the subject of preliminary studies.
Finally, a theoretical DFT study was carried out to have a better understanding of the tetrazole-azidoazomethine equilibrium on benzo- and pyrido- diazidodiazines similar to 6 azidotetrazolo [5,1-a] phthalazine, a toxic metabolite from Gymnodinium breve (Ptychodiscus brevis, actually known as Karenia brevis). Thermodynamic aspects, transition states, HOMO orbitals, local ionization potential maps, LUMO density maps, solvent effects, and some parameters to evaluate the aromaticity (Bird index, Jug minimum bond order, HOMA index and NICS) were considered in the study. It has been noted that some of the theoretical analysis can be good predictive tools, particularly with thermodynamic considerations, but they also have their limits, which are mainly due to the uncertainties inherent in the theoretical calculations.
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Charge transport and energy levels in organic semiconductors / Ladungstransport und Energieniveaus in organischen HalbleiternWidmer, Johannes 25 November 2014 (has links) (PDF)
Organic semiconductors are a new key technology for large-area and flexible thin-film electronics. They are deposited as thin films (sub-nanometer to micrometer) on large-area substrates. The technologically most advanced applications are organic light emitting diodes (OLEDs) and organic photovoltaics (OPV). For the improvement of performance and efficiency, correct modeling of the electronic processes in the devices is essential. Reliable characterization and validation of the electronic properties of the materials is simultaneously required for the successful optimization of devices. Furthermore, understanding the relations between material structures and their key characteristics opens the path for innovative material and device design.
In this thesis, two material characterization methods are developed, respectively refined and applied: a novel technique for measuring the charge carrier mobility μ and a way to determine the ionization energy IE or the electron affinity EA of an organic semiconductor.
For the mobility measurements, a new evaluation approach for space-charge limited current (SCLC) measurements in single carrier devices is developed. It is based on a layer thickness variation of the material under investigation. In the \"potential mapping\" (POEM) approach, the voltage as a function of the device thickness V(d) at a given current density is shown to coincide with the spatial distribution of the electric potential V(x) in the thickest device. On this basis, the mobility is directly obtained as function of the electric field F and the charge carrier density n. The evaluation is model-free, i.e. a model for μ(F, n) to fit the measurement data is not required, and the measurement is independent of a possible injection barrier or potential drop at non-optimal contacts. The obtained μ(F, n) function describes the effective average mobility of free and trapped charge carriers. This approach realistically describes charge transport in energetically disordered materials, where a clear differentiation between trapped and free charges is impossible or arbitrary.
The measurement of IE and EA is performed by characterizing solar cells at varying temperature T. In suitably designed devices based on a bulk heterojunction (BHJ), the open-circuit voltage Voc is a linear function of T with negative slope in the whole measured range down to 180K. The extrapolation to temperature zero V0 = Voc(T → 0K) is confirmed to equal the effective gap Egeff, i.e. the difference between the EA of the acceptor and the IE of the donor. The successive variation of different components of the devices and testing their influence on V0 verifies the relation V0 = Egeff. On this basis, the IE or EA of a material can be determined in a BHJ with a material where the complementary value is known. The measurement is applied to a number of material combinations, confirming, refining, and complementing previously reported values from ultraviolet photo electron spectroscopy (UPS) and inverse photo electron spectroscopy (IPES).
These measurements are applied to small molecule organic semiconductors, including mixed layers. In blends of zinc-phthalocyanine (ZnPc) and C60, the hole mobility is found to be thermally and field activated, as well as increasing with charge density. Varying the mixing ratio, the hole mobility is found to increase with increasing ZnPc content, while the effective gap stays unchanged. A number of further materials and material blends are characterized with respect to hole and electron mobility and the effective gap, including highly diluted donor blends, which have been little investigated before. In all materials, a pronounced field activation of the mobility is observed. The results enable an improved detailed description of the working principle of organic solar cells and support the future design of highly efficient and optimized devices. / Organische Halbleiter sind eine neue Schlüsseltechnologie für großflächige und flexible Dünnschichtelektronik. Sie werden als dünne Materialschichten (Sub-Nanometer bis Mikrometer) auf großflächige Substrate aufgebracht. Die technologisch am weitesten fortgeschrittenen Anwendungen sind organische Leuchtdioden (OLEDs) und organische Photovoltaik (OPV). Zur weiteren Steigerung von Leistungsfähigkeit und Effizienz ist die genaue Modellierung elektronischer Prozesse in den Bauteilen von grundlegender Bedeutung. Für die erfolgreiche Optimierung von Bauteilen ist eine zuverlässige Charakterisierung und Validierung der elektronischen Materialeigenschaften gleichermaßen erforderlich. Außerdem eröffnet das Verständnis der Zusammenhänge zwischen Materialstruktur und -eigenschaften einen Weg für innovative Material- und Bauteilentwicklung.
Im Rahmen dieser Dissertation werden zwei Methoden für die Materialcharakterisierung entwickelt, verfeinert und angewandt: eine neuartige Methode zur Messung der Ladungsträgerbeweglichkeit μ und eine Möglichkeit zur Bestimmung der Ionisierungsenergie IE oder der Elektronenaffinität EA eines organischen Halbleiters.
Für die Beweglichkeitsmessungen wird eine neue Auswertungsmethode für raumladungsbegrenzte Ströme (SCLC) in unipolaren Bauteilen entwickelt. Sie basiert auf einer Schichtdickenvariation des zu charakterisierenden Materials. In einem Ansatz zur räumlichen Abbildung des elektrischen Potentials (\"potential mapping\", POEM) wird gezeigt, dass das elektrische Potential als Funktion der Schichtdicke V(d) bei einer gegebenen Stromdichte dem räumlichen Verlauf des elektrischen Potentials V(x) im dicksten Bauteil entspricht. Daraus kann die Beweglichkeit als Funktion des elektrischen Felds F und der Ladungsträgerdichte n berechnet werden. Die Auswertung ist modellfrei, d.h. ein Modell zum Angleichen der Messdaten ist für die Berechnung von μ(F, n) nicht erforderlich. Die Messung ist außerdem unabhängig von einer möglichen Injektionsbarriere oder einer Potentialstufe an nicht-idealen Kontakten. Die gemessene Funktion μ(F, n) beschreibt die effektive durchschnittliche Beweglichkeit aller freien und in Fallenzuständen gefangenen Ladungsträger. Dieser Zugang beschreibt den Ladungstransport in energetisch ungeordneten Materialien realistisch, wo eine klare Unterscheidung zwischen freien und Fallenzuständen nicht möglich oder willkürlich ist.
Die Messung von IE und EA wird mithilfe temperaturabhängiger Messungen an Solarzellen durchgeführt. In geeigneten Bauteilen mit einem Mischschicht-Heteroübergang (\"bulk heterojunction\" BHJ) ist die Leerlaufspannung Voc im gesamten Messbereich oberhalb 180K eine linear fallende Funktion der Temperatur T. Es kann bestätigt werden, dass die Extrapolation zum Temperaturnullpunkt V0 = Voc(T → 0K) mit der effektiven Energielücke Egeff , d.h. der Differenz zwischen EA des Akzeptor-Materials und IE des Donator-Materials, übereinstimmt. Die systematische schrittweise Variation einzelner Bestandteile der Solarzellen und die Überprüfung des Einflusses auf V0 bestätigen die Beziehung V0 = Egeff. Damit kann die IE oder EA eines Materials bestimmt werden, indem man es in einem BHJ mit einem Material kombiniert, dessen komplementärer Wert bekannt ist. Messungen per Ultraviolett-Photoelektronenspektroskopie (UPS) und inverser Photoelektronenspektroskopie (IPES) werden damit bestätigt, präzisiert und ergänzt.
Die beiden entwickelten Messmethoden werden auf organische Halbleiter aus kleinen Molekülen einschließlich Mischschichten angewandt. In Mischschichten aus Zink-Phthalocyanin (ZnPc) und C60 wird eine Löcherbeweglichkeit gemessen, die sowohl thermisch als auch feld- und ladungsträgerdichteaktiviert ist. Wenn das Mischverhältnis variiert wird, steigt die Löcherbeweglichkeit mit zunehmendem ZnPc-Anteil, während die effektive Energielücke unverändert bleibt. Verschiedene weitere Materialien und Materialmischungen werden hinsichtlich Löcher- und Elektronenbeweglichkeit sowie ihrer Energielücke charakterisiert, einschließlich bisher wenig untersuchter hochverdünnter Donator-Systeme. In allen Materialien wird eine deutliche Feldaktivierung der Beweglichkeit beobachtet. Die Ergebnisse ermöglichen eine verbesserte Beschreibung der detaillierten Funktionsweise organischer Solarzellen und unterstützen die künftige Entwicklung hocheffizienter und optimierter Bauteile.
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Charge transport and energy levels in organic semiconductorsWidmer, Johannes 02 October 2014 (has links)
Organic semiconductors are a new key technology for large-area and flexible thin-film electronics. They are deposited as thin films (sub-nanometer to micrometer) on large-area substrates. The technologically most advanced applications are organic light emitting diodes (OLEDs) and organic photovoltaics (OPV). For the improvement of performance and efficiency, correct modeling of the electronic processes in the devices is essential. Reliable characterization and validation of the electronic properties of the materials is simultaneously required for the successful optimization of devices. Furthermore, understanding the relations between material structures and their key characteristics opens the path for innovative material and device design.
In this thesis, two material characterization methods are developed, respectively refined and applied: a novel technique for measuring the charge carrier mobility μ and a way to determine the ionization energy IE or the electron affinity EA of an organic semiconductor.
For the mobility measurements, a new evaluation approach for space-charge limited current (SCLC) measurements in single carrier devices is developed. It is based on a layer thickness variation of the material under investigation. In the \"potential mapping\" (POEM) approach, the voltage as a function of the device thickness V(d) at a given current density is shown to coincide with the spatial distribution of the electric potential V(x) in the thickest device. On this basis, the mobility is directly obtained as function of the electric field F and the charge carrier density n. The evaluation is model-free, i.e. a model for μ(F, n) to fit the measurement data is not required, and the measurement is independent of a possible injection barrier or potential drop at non-optimal contacts. The obtained μ(F, n) function describes the effective average mobility of free and trapped charge carriers. This approach realistically describes charge transport in energetically disordered materials, where a clear differentiation between trapped and free charges is impossible or arbitrary.
The measurement of IE and EA is performed by characterizing solar cells at varying temperature T. In suitably designed devices based on a bulk heterojunction (BHJ), the open-circuit voltage Voc is a linear function of T with negative slope in the whole measured range down to 180K. The extrapolation to temperature zero V0 = Voc(T → 0K) is confirmed to equal the effective gap Egeff, i.e. the difference between the EA of the acceptor and the IE of the donor. The successive variation of different components of the devices and testing their influence on V0 verifies the relation V0 = Egeff. On this basis, the IE or EA of a material can be determined in a BHJ with a material where the complementary value is known. The measurement is applied to a number of material combinations, confirming, refining, and complementing previously reported values from ultraviolet photo electron spectroscopy (UPS) and inverse photo electron spectroscopy (IPES).
These measurements are applied to small molecule organic semiconductors, including mixed layers. In blends of zinc-phthalocyanine (ZnPc) and C60, the hole mobility is found to be thermally and field activated, as well as increasing with charge density. Varying the mixing ratio, the hole mobility is found to increase with increasing ZnPc content, while the effective gap stays unchanged. A number of further materials and material blends are characterized with respect to hole and electron mobility and the effective gap, including highly diluted donor blends, which have been little investigated before. In all materials, a pronounced field activation of the mobility is observed. The results enable an improved detailed description of the working principle of organic solar cells and support the future design of highly efficient and optimized devices.:1. Introduction
2. Organic semiconductors and devices
2.1. Organic semiconductors
2.1.1. Conjugated π system
2.1.2. Small molecules and polymers
2.1.3. Disorder in amorphous materials
2.1.4. Polarons
2.1.5. Polaron hopping
2.1.6. Fermi-Dirac distribution and Fermi level
2.1.7. Quasi-Fermi levels
2.1.8. Trap states
2.1.9. Doping
2.1.10. Excitons
2.2. Interfaces and blend layers
2.2.1. Interface dipoles
2.2.2. Energy level bending
2.2.3. Injection from metal into semiconductor, and extraction
2.2.4. Excitons at interfaces
2.3. Charge transport and recombination in organic semiconductors
2.3.1. Drift transport
2.3.2. Charge carrier mobility
2.3.3. Thermally activated transport
2.3.4. Diffusion transport
2.3.5. Drift-diffusion transport
2.3.6. Space-charge limited current
2.3.7. Recombination
2.4. Mobility measurement
2.4.1. SCLC and TCLC
2.4.2. Time of flight
2.4.3. Organic field effect transistors
2.4.4. CELIV
2.5. Organic solar cells
2.5.1. Exciton diffusion towards the interface
2.5.2. Dissociation of CT states
2.5.3. CT recombination
2.5.4. Flat and bulk heterojunction
2.5.5. Transport layers
2.5.6. Thin film optics
2.5.7. Current-voltage characteristics and equivalent circuit
2.5.8. Solar cell efficiency
2.5.9. Limits of efficiency
2.5.10. Correct solar cell characterization
2.5.11. The \"O-Factor\"
3. Materials and experimental methods
3.1. Materials
3.2. Device fabrication and layout
3.2.1. Layer deposition
3.2.2. Encapsulation
3.2.3. Homogeneity of layer thickness on a wafer
3.2.4. Device layout
3.3. Characterization
3.3.1. Electrical characterization
3.3.2. Sample illumination
3.3.3. Temperature dependent characterization
3.3.4. UPS
4. Simulations
5.1. Design of single carrier devices
5.1.1. General design requirements
5.1.2. Single carrier devices for space-charge limited current
5.1.3. Ohmic regime
5.1.4. Design of injection and extraction layers
5.2. Advanced evaluation of SCLC – potential mapping
5.2.1. Potential mapping by thickness variation
5.2.2. Further evaluation of the transport profile
5.2.3. Injection into and extraction from single carrier devices
5.2.4. Majority carrier approximation
5.3. Proof of principle: POEM on simulated data
5.3.1. Constant mobility
5.3.2. Field dependent mobility
5.3.3. Field and charge density activated mobility
5.3.4. Conclusion
5.4. Application: Transport characterization in organic semiconductors
5.4.1. Hole transport in ZnPc:C60
5.4.2. Hole transport in ZnPc:C60 – temperature variation
5.4.3. Hole transport in ZnPc:C60 – blend ratio variation
5.4.4. Hole transport in ZnPc:C70
5.4.5. Hole transport in neat ZnPc
5.4.6. Hole transport in F4-ZnPc:C60
5.4.7. Hole transport in DCV-5T-Me33:C60
5.4.8. Electron transport in ZnPc:C60
5.4.9. Electron transport in neat Bis-HFl-NTCDI
5.5. Summary and discussion of the results
5.5.1. Phthalocyanine:C60 blends
5.5.2. DCV-5T-Me33:C60
5.5.3. Conclusion
6. Organic solar cell characteristics: the influence of temperature
6.1. ZnPc:C60 solar cells
6.1.1. Temperature variation
6.1.2. Illumination intensity variation
6.2. Voc in flat and bulk heterojunction organic solar cells
6.2.1. Qualitative difference in Voc(I, T)
6.2.2. Interpretation of Voc(I, T)
6.3. BHJ stoichiometry variation
6.3.1. Voc upon variation of stoichiometry and contact layer
6.3.2. V0 upon stoichiometry variation
6.3.3. Low donor content stoichiometry
6.3.4. Conclusion from stoichiometry variation
6.4. Transport material variation
6.4.1. HTM variation
6.4.2. ETM variation
6.5. Donor:acceptor material variation
6.5.1. Donor variation
6.5.2. Acceptor variation
6.6. Conclusion
7. Summary and outlook
7.1. Summary
7.2. Outlook
A. Appendix
A.1. Energy pay-back of this thesis
A.2. Tables and registers / Organische Halbleiter sind eine neue Schlüsseltechnologie für großflächige und flexible Dünnschichtelektronik. Sie werden als dünne Materialschichten (Sub-Nanometer bis Mikrometer) auf großflächige Substrate aufgebracht. Die technologisch am weitesten fortgeschrittenen Anwendungen sind organische Leuchtdioden (OLEDs) und organische Photovoltaik (OPV). Zur weiteren Steigerung von Leistungsfähigkeit und Effizienz ist die genaue Modellierung elektronischer Prozesse in den Bauteilen von grundlegender Bedeutung. Für die erfolgreiche Optimierung von Bauteilen ist eine zuverlässige Charakterisierung und Validierung der elektronischen Materialeigenschaften gleichermaßen erforderlich. Außerdem eröffnet das Verständnis der Zusammenhänge zwischen Materialstruktur und -eigenschaften einen Weg für innovative Material- und Bauteilentwicklung.
Im Rahmen dieser Dissertation werden zwei Methoden für die Materialcharakterisierung entwickelt, verfeinert und angewandt: eine neuartige Methode zur Messung der Ladungsträgerbeweglichkeit μ und eine Möglichkeit zur Bestimmung der Ionisierungsenergie IE oder der Elektronenaffinität EA eines organischen Halbleiters.
Für die Beweglichkeitsmessungen wird eine neue Auswertungsmethode für raumladungsbegrenzte Ströme (SCLC) in unipolaren Bauteilen entwickelt. Sie basiert auf einer Schichtdickenvariation des zu charakterisierenden Materials. In einem Ansatz zur räumlichen Abbildung des elektrischen Potentials (\"potential mapping\", POEM) wird gezeigt, dass das elektrische Potential als Funktion der Schichtdicke V(d) bei einer gegebenen Stromdichte dem räumlichen Verlauf des elektrischen Potentials V(x) im dicksten Bauteil entspricht. Daraus kann die Beweglichkeit als Funktion des elektrischen Felds F und der Ladungsträgerdichte n berechnet werden. Die Auswertung ist modellfrei, d.h. ein Modell zum Angleichen der Messdaten ist für die Berechnung von μ(F, n) nicht erforderlich. Die Messung ist außerdem unabhängig von einer möglichen Injektionsbarriere oder einer Potentialstufe an nicht-idealen Kontakten. Die gemessene Funktion μ(F, n) beschreibt die effektive durchschnittliche Beweglichkeit aller freien und in Fallenzuständen gefangenen Ladungsträger. Dieser Zugang beschreibt den Ladungstransport in energetisch ungeordneten Materialien realistisch, wo eine klare Unterscheidung zwischen freien und Fallenzuständen nicht möglich oder willkürlich ist.
Die Messung von IE und EA wird mithilfe temperaturabhängiger Messungen an Solarzellen durchgeführt. In geeigneten Bauteilen mit einem Mischschicht-Heteroübergang (\"bulk heterojunction\" BHJ) ist die Leerlaufspannung Voc im gesamten Messbereich oberhalb 180K eine linear fallende Funktion der Temperatur T. Es kann bestätigt werden, dass die Extrapolation zum Temperaturnullpunkt V0 = Voc(T → 0K) mit der effektiven Energielücke Egeff , d.h. der Differenz zwischen EA des Akzeptor-Materials und IE des Donator-Materials, übereinstimmt. Die systematische schrittweise Variation einzelner Bestandteile der Solarzellen und die Überprüfung des Einflusses auf V0 bestätigen die Beziehung V0 = Egeff. Damit kann die IE oder EA eines Materials bestimmt werden, indem man es in einem BHJ mit einem Material kombiniert, dessen komplementärer Wert bekannt ist. Messungen per Ultraviolett-Photoelektronenspektroskopie (UPS) und inverser Photoelektronenspektroskopie (IPES) werden damit bestätigt, präzisiert und ergänzt.
Die beiden entwickelten Messmethoden werden auf organische Halbleiter aus kleinen Molekülen einschließlich Mischschichten angewandt. In Mischschichten aus Zink-Phthalocyanin (ZnPc) und C60 wird eine Löcherbeweglichkeit gemessen, die sowohl thermisch als auch feld- und ladungsträgerdichteaktiviert ist. Wenn das Mischverhältnis variiert wird, steigt die Löcherbeweglichkeit mit zunehmendem ZnPc-Anteil, während die effektive Energielücke unverändert bleibt. Verschiedene weitere Materialien und Materialmischungen werden hinsichtlich Löcher- und Elektronenbeweglichkeit sowie ihrer Energielücke charakterisiert, einschließlich bisher wenig untersuchter hochverdünnter Donator-Systeme. In allen Materialien wird eine deutliche Feldaktivierung der Beweglichkeit beobachtet. Die Ergebnisse ermöglichen eine verbesserte Beschreibung der detaillierten Funktionsweise organischer Solarzellen und unterstützen die künftige Entwicklung hocheffizienter und optimierter Bauteile.:1. Introduction
2. Organic semiconductors and devices
2.1. Organic semiconductors
2.1.1. Conjugated π system
2.1.2. Small molecules and polymers
2.1.3. Disorder in amorphous materials
2.1.4. Polarons
2.1.5. Polaron hopping
2.1.6. Fermi-Dirac distribution and Fermi level
2.1.7. Quasi-Fermi levels
2.1.8. Trap states
2.1.9. Doping
2.1.10. Excitons
2.2. Interfaces and blend layers
2.2.1. Interface dipoles
2.2.2. Energy level bending
2.2.3. Injection from metal into semiconductor, and extraction
2.2.4. Excitons at interfaces
2.3. Charge transport and recombination in organic semiconductors
2.3.1. Drift transport
2.3.2. Charge carrier mobility
2.3.3. Thermally activated transport
2.3.4. Diffusion transport
2.3.5. Drift-diffusion transport
2.3.6. Space-charge limited current
2.3.7. Recombination
2.4. Mobility measurement
2.4.1. SCLC and TCLC
2.4.2. Time of flight
2.4.3. Organic field effect transistors
2.4.4. CELIV
2.5. Organic solar cells
2.5.1. Exciton diffusion towards the interface
2.5.2. Dissociation of CT states
2.5.3. CT recombination
2.5.4. Flat and bulk heterojunction
2.5.5. Transport layers
2.5.6. Thin film optics
2.5.7. Current-voltage characteristics and equivalent circuit
2.5.8. Solar cell efficiency
2.5.9. Limits of efficiency
2.5.10. Correct solar cell characterization
2.5.11. The \"O-Factor\"
3. Materials and experimental methods
3.1. Materials
3.2. Device fabrication and layout
3.2.1. Layer deposition
3.2.2. Encapsulation
3.2.3. Homogeneity of layer thickness on a wafer
3.2.4. Device layout
3.3. Characterization
3.3.1. Electrical characterization
3.3.2. Sample illumination
3.3.3. Temperature dependent characterization
3.3.4. UPS
4. Simulations
5.1. Design of single carrier devices
5.1.1. General design requirements
5.1.2. Single carrier devices for space-charge limited current
5.1.3. Ohmic regime
5.1.4. Design of injection and extraction layers
5.2. Advanced evaluation of SCLC – potential mapping
5.2.1. Potential mapping by thickness variation
5.2.2. Further evaluation of the transport profile
5.2.3. Injection into and extraction from single carrier devices
5.2.4. Majority carrier approximation
5.3. Proof of principle: POEM on simulated data
5.3.1. Constant mobility
5.3.2. Field dependent mobility
5.3.3. Field and charge density activated mobility
5.3.4. Conclusion
5.4. Application: Transport characterization in organic semiconductors
5.4.1. Hole transport in ZnPc:C60
5.4.2. Hole transport in ZnPc:C60 – temperature variation
5.4.3. Hole transport in ZnPc:C60 – blend ratio variation
5.4.4. Hole transport in ZnPc:C70
5.4.5. Hole transport in neat ZnPc
5.4.6. Hole transport in F4-ZnPc:C60
5.4.7. Hole transport in DCV-5T-Me33:C60
5.4.8. Electron transport in ZnPc:C60
5.4.9. Electron transport in neat Bis-HFl-NTCDI
5.5. Summary and discussion of the results
5.5.1. Phthalocyanine:C60 blends
5.5.2. DCV-5T-Me33:C60
5.5.3. Conclusion
6. Organic solar cell characteristics: the influence of temperature
6.1. ZnPc:C60 solar cells
6.1.1. Temperature variation
6.1.2. Illumination intensity variation
6.2. Voc in flat and bulk heterojunction organic solar cells
6.2.1. Qualitative difference in Voc(I, T)
6.2.2. Interpretation of Voc(I, T)
6.3. BHJ stoichiometry variation
6.3.1. Voc upon variation of stoichiometry and contact layer
6.3.2. V0 upon stoichiometry variation
6.3.3. Low donor content stoichiometry
6.3.4. Conclusion from stoichiometry variation
6.4. Transport material variation
6.4.1. HTM variation
6.4.2. ETM variation
6.5. Donor:acceptor material variation
6.5.1. Donor variation
6.5.2. Acceptor variation
6.6. Conclusion
7. Summary and outlook
7.1. Summary
7.2. Outlook
A. Appendix
A.1. Energy pay-back of this thesis
A.2. Tables and registers
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