Electronic Coupling Effects and Charge Transfer Between Organic
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Theoretical Electron Affinities of Pahs and Electronic Absorption Spectra Of
A&A 432, 585–594 (2005) Astronomy DOI: 10.1051/0004-6361:20042246 & c ESO 2005 Astrophysics Theoretical electron affinities of PAHs and electronic absorption spectra of their mono-anions G. Malloci1,2,G.Mulas1, G. Cappellini2,3, V. Fiorentini2,3, and I. Porceddu1 1 INAF - Osservatorio Astronomico di Cagliari – Astrochemistry Group, Strada n. 54, Loc. Poggio dei Pini, 09012 Capoterra (CA), Italy e-mail: [gmalloci;gmulas;iporcedd]@ca.astro.it 2 Dipartimento di Fisica, Università degli Studi di Cagliari, Complesso Universitario di Monserrato, S. P. Monserrato-Sestu Km 0,700, 09042 Monserrato (CA), Italy e-mail: [giancarlo.cappellini;vincenzo.fiorentini]@dsf.unica.it 3 INFM - Sardinian Laboratory for Computational Materials Science (SLACS) Received 25 October 2004 / Accepted 8 November 2004 Abstract. We present theoretical electron affinities, calculated as total energy differences, for a large sample of polycyclic aromatic hydrocarbons (PAHs), ranging in size from azulene (C10H8) to dicoronylene (C48H20). For 20 out of 22 molecules under study we obtained electron affinity values in the range 0.4–2.0 eV, showing them to be able to accept an additional electron in their LUMO π orbital. For the mono-anions we computed the absolute photo-absorption cross-sections up to the vacuum ultraviolet (VUV) using an implementation in real time and real space of the Time-Dependent Density Functional Theory (TD–DFT), an approach which has already been proven to yield accurate results for neutral and cationic PAHs. Comparison with available experimental data hints that this is the case for mono-anions as well. We find that PAH anions, like their parent molecules and the corresponding cations, display strong π∗ ← π electronic transitions in the UV. -
Photo-Processing of Astro-Pahs
Photo-processing of astro-PAHs C Joblin1, G Wenzel1, S Rodriguez Castillo1,2, A Simon2,H Sabbah1,3, A Bonnamy1, D Toublanc1, G Mulas1,4, M Ji1, A Giuliani5,6, L Nahon5 1Institut de Recherche en Astrophysique et Plan´etologie(IRAP), Universit´ede Toulouse (UPS), CNRS, CNES, 9 Avenue du Colonel Roche, F-31028 Toulouse Cedex 4, France 2Laboratoire de Chimie et Physique Quantiques (LCPQ/IRSAMC), Universit´ede Toulouse and CNRS,UT3-Paul Sabatier, 118 Route de Narbonne, 31062 Toulouse, France 3Laboratoire Collisions Agr´egatsR´eactivit´e(LCAR/IRSAMC), Universit´ede Toulouse (UPS), CNRS, 118 Route de Narbonne, F-31062 Toulouse, France 4Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (Cagliari), Italy 5Synchrotron SOLEIL, L'Orme des Merisiers, F-91192 Gif-sur-Yvette Cedex, France 6INRA, UAR1008, Caract´erisationet Elaboration des Produits Issus de l'Agriculture, F-44316 Nantes, France E-mail: [email protected] Abstract. Polycyclic aromatic hydrocarbons (PAHs) are key species in astrophysical environments in which vacuum ultraviolet (VUV) photons are present, such as star-forming regions. The interaction with these VUV photons governs the physical and chemical evolution of PAHs. Models show that only large species can survive. However, the actual molecular properties of large PAHs are poorly characterized and the ones included in models are only an extrapolation of the properties of small and medium-sized species. We discuss here experiments performed on trapped ions including some at the SOLEIL VUV beam line DESIRS. We focus + on the case of the large dicoronylene cation, C48H20, and compare its behavior under VUV processing with that of smaller species. -
L115 Modeling the Unidentified Infrared Emission With
The Astrophysical Journal, 511:L115±L119, 1999 February 1 q 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A. MODELING THE UNIDENTIFIED INFRARED EMISSION WITH COMBINATIONS OF POLYCYCLIC AROMATIC HYDROCARBONS L. J. Allamandola, D. M. Hudgins, and S. A. Sandford NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035 Received 1998 July 13; accepted 1998 November 24; published 1999 January 18 ABSTRACT The infrared emission band spectrum associated with many different interstellar objects can be modeled successfully by using combined laboratory spectra of neutral and positively charged polycyclic aromatic hydro- carbons (PAHs). These model spectra, shown here for the ®rst time, alleviate the principal spectroscopic criticisms previously leveled at the PAH hypothesis and demonstrate that mixtures of free molecular PAHs can indeed account for the overall appearance of the widespread interstellar infrared emission spectrum. Furthermore, these models give us insight into the structures, stabilities, abundances, and ionization balance of the interstellar PAH population. These, in turn, re¯ect conditions in the emission zones and shed light on the microscopic processes involved in the carbon nucleation, growth, and evolution in circumstellar shells and the interstellar medium. Subject headings: infrared: ISM: lines and bands Ð ISM: individual (Orion Bar, IRAS 2227215435) Ð line: formation Ð line: identi®cation Ð line: pro®les Ð molecular data Ð radiation mechanisms: nonthermal 1. INTRODUCTION resemblance of the -
Coronene Encapsulation in Singlewalled Carbon Nanotubes
CHEMPHYSCHEM ARTICLES DOI: 10.1002/cphc.201301200 Coronene Encapsulation in Single-Walled Carbon Nanotubes: Stacked Columns, Peapods, and Nanoribbons Ilya V. Anoshkin,*[a] Alexandr V. Talyzin,*[b] Albert G. Nasibulin,[a, e] Arkady V. Krasheninnikov,[c] Hua Jiang,[a] Risto M. Nieminen,[d] and Esko I. Kauppinen[a] Encapsulation of coronene inside single-walled carbon nano- tions between the coronene molecules and the formation of tubes (SWNTs) was studied under various conditions. Under hydrogen-terminated graphene nanoribbons. It was also ob- high vacuum, two main types of molecular encapsulation were served that the morphology of the encapsulated products observed by using transmission electron microscopy: coronene depend on the diameter of the SWNTs. The experimental re- dimers and molecular stacking columns perpendicular or tilted sults are explained by using density functional theory calcula- (45–608) with regard to the axis of the SWNTs. A relatively tions through the energies of the coronene molecules inside small number of short nanoribbons or polymerized coronene the SWNTs, which depend on the orientation of the molecules molecular chains were observed. However, experiments per- and the diameter of the tubes. formed under an argon atmosphere (0.17 MPa) revealed reac- 1. Introduction Graphene nanoribbons (GNRs) are of great interest for various in SWNTs by using thermally induced fusion of the molecular applications due to their unique electronic properties.[1–7] GNRs precursors: coronene and perylene.[17] The nanoribbons exhib- -
Hexa-Peri-Hexabenzocoronene in Organic Electronics*
Pure Appl. Chem., Vol. 84, No. 4, pp. 1047–1067, 2012. http://dx.doi.org/10.1351/PAC-CON-11-09-24 © 2012 IUPAC, Publication date (Web): 13 March 2012 Hexa-peri-hexabenzocoronene in organic electronics* Helga Seyler, Balaji Purushothaman, David J. Jones, Andrew B. Holmes, and Wallace W. H. Wong‡ School of Chemistry, Bio21 Institute, University of Melbourne, 30 Flemington Road, Parkville, Victoria 3010, Australia Abstract: Polycyclic aromatic hydrocarbons (PAHs) are in a class of functional organic com- pounds with increasing importance in organic electronics. Their tunable photophysical prop- erties and typically strong intermolecular associations make them ideal materials in applica- tions where control of charge mobility is essential. Hexa-peri-hexabenzocoronene (HBC) is a disc-shaped PAH that self-associates into columnar stacks through strong π–π interactions. By decorating the periphery of the HBC molecule with various substituents, a range of prop- erties and functions can be obtained including solution processability, liquid crystallinity, and semiconductivity. In this review article, the synthesis, properties, and functions of HBC derivatives are presented with focus on work published in the last five years. Keywords: hexabenzocoronene; materials chemistry; molecular electronics; organic electron- ics; organic semiconductors; photovoltaics; polycyclic aromatics; self-organization. INTRODUCTION Polycyclic aromatic hydrocarbons (PAHs) are defined as fused ring materials consisting of sp2 carbon centers and can be considered as segments of graphite. The dominant intermolecular force is often face- to-face π–π interactions with some examples of face-to-edge (or herringbone) assembly. Although PAHs can often be found naturally in combustion residues, analytically pure and discrete PAHs can only be obtained through synthesis. -
Topological Analysis of Pahs Using Irregularity Based Indices
Article Volume 12, Issue 3, 2022, 2970 - 2987 https://doi.org/10.33263/BRIAC123.29702987 Topological Analysis of PAHs using Irregularity based Indices Julietraja Konsalraj 1,* , Venugopal Padmanabhan 2 , Chellamani Perumal 3 1 Department of Mathematics, Sri Sivasubramaniya Nadar College of Engineering, Kalavakkam – 603 110, India; [email protected] (J.K.); 2 Department of Mathematics, Shiv Nadar University Chennai, Kalavakkam – 603 110, India; [email protected] (V.P.); 3 Department of Mathematics, Sacred Heart College (Autonomous), Tirupattur – 635 601, Tirupattur Dt., India; [email protected] (C.P.); * Correspondence: [email protected] (J.K.); Scopus Author ID 57218631900 Received: 8.06.2021; Revised: 15.07.2021; Accepted: 22.07.2021; Published: 8.08.2021 Abstract: Topological descriptors are non-empirical graph invariants that characterize the structures of chemical molecules. The structural descriptors are vital components of QSAR/QSPR studies which form the basis for theoretical chemists to design and investigate new chemical structures. Irregularity indices are a class of topological descriptors that have been employed to study certain chemical properties of compounds. This article aims to compute analytical expressions of irregularity indices for three important classes of polycyclic aromatic hydrocarbons. The intriguing properties of these classes of compounds have several potential applications in wide-raging fields, which warrant a study of their properties from a structural perspective. Additionally, the 3D graphical representations of a few indices are presented, which will aid in analyzing the similarity of behavior among the indices. Keywords: topological descriptors; benzenoid systems; graph-theoretical methods; irregularity indices. © 2021 by the authors. This article is an open-access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). -
Expanded Aromatic Monomers for Functional Porous Polymers
EXPANDED AROMATIC MONOMERS FOR FUNCTIONAL POROUS POLYMERS by Arosha Aruni Kumari Karunathilake APPROVED BY SUPERVISORY COMMITTEE: ___________________________________________ Dr. Ronald A. Smaldone, Chair ___________________________________________ Dr. Michael C. Biewer ___________________________________________ Dr. John W. Sibert ___________________________________________ Dr. Yves J. Chabal Copyright 2017 Arosha Aruni Kumari Karunathilake All Rights Reserved To my loving parents and to my loving husband, Eranda EXPANDED AROMATIC MONOMERS FOR FUNCTIONAL POROUS POLYMERS by AROSHA ARUNI KUMARI KARUNATHILAKE, BS DISSERTATION Presented to the Faculty of The University of Texas at Dallas in Partial Fulfillment of the Requirements for the Degree of DOCTOR OF PHILOSOPHY IN CHEMISTRY THE UNIVERSITY OF TEXAS AT DALLAS May 2017 ACKNOWLEDGMENTS First and foremost, I would like to acknowledge my research advisor and mentor, Dr. Ronald A. Smaldone, for his endless scientific guidance, unwavering support and enthusiasm throughout the years. His guidance and encouragement were always behind my success. I thank members of my supervisory committee Dr. Michael C. Biewer, Dr. John W. Sibert and Dr. Yves J. Chabal for their constructive advice and new ideas. Their advice and comments helped me to add value to my research work and to come up with high quality outputs. I respect and appreciate all my colleagues from the Smaldone group, both past and present: Dr. Christina Thompson for getting me started in the lab and introducing me to projects, Dr. Sumudu Wijenayake for enduring friendship and technical expertise, Fei Li for his support and encouragement at my early years, Sampath Alhakoon for his valuable discussions and always being there to help me, Gayan Adikari for his friendship, support and encouragement, Yinhuwan Xie for positive attitude and sense of humor, Vicky, Josh, Daniel and Grant for their helpful nature and company. -
Astronomy Astrophysics
A&A 390, 1153–1170 (2002) Astronomy DOI: 10.1051/0004-6361:20020478 & c ESO 2002 Astrophysics Spectroscopy of large PAHs Laboratory studies and comparison to the Diffuse Interstellar Bands R. Ruiterkamp1, T. Halasinski2, F. Salama2,B.H.Foing3, L. J. Allamandola2,W.Schmidt4, and P. Ehrenfreund1 1 Leiden Observatory, PO Box 9513, 2300 RA Leiden, The Netherlands 2 Space Science Division, NASA-Ames Research Center, Moffett Field CA 94035, USA 3 ESA Research Support Division, ESTEC/SCI-SR, PO Box 229, 2200 AG, Noordwijk, The Netherlands 4 PAH Forschungs Institut, Flurstrasse 17, 86926 Greifenberg/Ammersee, Germany Received 16 January 2002 / Accepted 27 March 2002 Abstract. Polycyclic Aromatic Hydrocarbons (PAHs) are thought to be the carriers of the ubiquitous infrared emission bands (UIBs). Data from the Infrared Space Observatory (ISO) have provided new insights into the size distribution and the structure of interstellar PAH molecules pointing to a trend towards larger-size PAHs. The mid-infrared spectra of galactic and extragalactic sources have also indicated the presence of 5-ring structures and PAH structures with attached side groups. This paper reports for the first time the laboratory measurement of the UV–Vis–NIR absorption spectra of a representative set of large PAHs that have also been selected for a long duration exposure experiment on the International Space Station ISS. PAHs with sizes up to 600 amu, including 5-ring species and PAHs containing heteroatoms, have been synthesized and their spectra measured using matrix isolation spectroscopy. The spectra of the neutral species and the associated cations and anions measured in this work are also compared to astronomical spectra of Diffuse Interstellar Bands (DIBs). -
The Laboratory Spectra
The Astrophysical Journal Supplement Series, 251:22 (16pp), 2020 December https://doi.org/10.3847/1538-4365/abc2c8 © 2020. The American Astronomical Society. All rights reserved. The NASA Ames PAH IR Spectroscopic Database: The Laboratory Spectra A. L. Mattioda1 , D. M. Hudgins2, C. Boersma1 , C. W. Bauschlicher, Jr.3 , A. Ricca1,4 , J. Cami4,5,6 , E. Peeters4,5,6 , F. Sánchez de Armas4, G. Puerta Saborido4, and L. J. Allamandola1 1 NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035, USA; [email protected] 2 NASA Headquarters, MS 3Y28, 300 E St. SW, Washington, DC 20546, USA 3 NASA Ames Research Center, MS 230-3, Moffett Field, CA 94035, USA 4 Carl Sagan Center, SETI Institute, 189 N. Bernardo Avenue, Suite 200, Mountain View, CA 94043, USA 5 Department of Physics and Astronomy, The University of Western Ontario, London, ON N6A 3K7, Canada 6 The Institute for Earth and Space Exploration, The University of Western Ontario, London ON N6A 3K7, Canada Received 2020 April 16; revised 2020 September 29; accepted 2020 October 16; published 2020 December 1 Abstract The astronomical emission features, formerly known as the unidentified infrared bands, are now commonly ascribed to polycyclic aromatic hydrocarbons (PAHs). The laboratory experiments and computational modeling performed at NASA Ames Research Center generated a collection of PAH IR spectra that have been used to test and refine the PAH model. These data have been assembled into the NASA Ames PAH IR Spectroscopic Database (PAHdb). PAHdb’s library of computed spectra, currently at version 3.20, contains data on more than 4000 species and the library of laboratory-measured spectra, currently at version 3.00, contains data on 84 species. -
Electronic Absorption Spectra of Pahs up to Vacuum UV
A&A 426, 105–117 (2004) Astronomy DOI: 10.1051/0004-6361:20040541 & c ESO 2004 Astrophysics Electronic absorption spectra of PAHs up to vacuum UV Towards a detailed model of interstellar PAH photophysics G. Malloci1,2,G.Mulas1,2, and C. Joblin3 1 INAF - Osservatorio Astronomico di Cagliari - Astrochemistry Group, Strada n.54, Loc. Poggio dei Pini, 09012 Capoterra (CA), Italy e-mail: [gmalloci;gmulas]@ca.astro.it 2 Astrochemical Research in Space Network, http://www.arsnetwork.org 3 Centre d’Étude Spatiale des Rayonnements, CNRS et Université Paul Sabatier, 9 avenue du colonel Roche, 31028 Toulouse, France e-mail: [email protected] Received 29 March 2004 / Accepted 17 June 2004 Abstract. We computed the absolute photo-absorption cross-sections up to the vacuum ultaviolet (VUV) of a total of 20 Polycyclic Aromatic Hydrocarbons (PAHs) and their respective cations, ranging in size from naphthalene (C10H8)todi- coronylene (C48H20). We used an implementation in real time and real space of the Time-Dependent Density Functional Theory (TD-DFT), an approach which was proven to yield accurate results for conjugated molecules such as benzene. Concerning the low-lying excited states of π∗ ← π character occurring in the near-IR, visible and near-UV spectral range, the computed spectra are in good agreement with the available experimental data, predicting vertical excitation energies precise to within a few tenths of eV, and the corresponding oscillator strengths to within experimental errors, which are indeed the typical accuracies currently achievable by TD-DFT. We find that PAH cations, like their parent molecules, display strong π∗ ← π electronic transitions in the UV, a piece of information which is particularly useful since a limited amount of laboratory data is available concerning the absorption properties of PAH ions in this wavelength range. -
Heteroatom-Containing Carbon Nanostructures As Oxygen Reduction Electrocatalysts for PEM and Direct Methanol Fuel Cells
Heteroatom-containing Carbon Nanostructures as Oxygen Reduction Electrocatalysts for PEM and Direct Methanol Fuel Cells Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Dieter von Deak, B.S.ChE Graduate Program in Chemical Engineering * * * * The Ohio State University 2011 Dissertation Committee: Professor Umit S. Ozkan, Advisor Professor David Wood Professor James Rathman Copyright by Dieter von Deak 2011 2 ABSTRACT The main goal of this work was to undertake a fundamental investigation of precious metal-free carbon catalysts nano-structure modification to enable their use as oxygen reduction reaction (ORR) catalysts in proton exchange membrane (PEM) fuel cells. The sluggish ORR is accelerated by fiscally prohibitive loadings of Pt catalyst. The expense and availability of platinum motivate the development of non-precious metal carbon-nitroge-based ORR catalysts (CNx). The project targets the nature of oxygen reduction reaction active sites and exploring ways to create these sites by molecular tailoring of carbon nano-structures. CNx grown with phosphorous had a significant increase in the ORR active site density. CNx catalyst growth media was prepared by acetonitrile deposition over a Fe and P impregnated MgO. Rotating Ring Disk Electrode (RRDE) Activity and selectivity showed a significant increase in oxygen reduction current with CNx grown with less than a 1:1 molar ratio of P:Fe. Selectivity for the full reduction of dioxygen to water trended with increasing ORR activity for phosphorous grown CNx catalysts. Phosphorus growth altered the morphology of carbon-nitride graphite formed during pyrolysis. -
Large Polycyclic Aromatic Hydrocarbons: Synthesis and Discotic Organization*
Pure Appl. Chem., Vol. 81, No. 12, pp. 2203–2224, 2009. doi:10.1351/PAC-CON-09-07-07 © 2009 IUPAC, Publication date (Web): 31 October 2009 Large polycyclic aromatic hydrocarbons: Synthesis and discotic organization* Xinliang Feng‡, Wojciech Pisula†, and Klaus Müllen** Max Planck Institute for Polymer Research, Ackermannweg 10, 55128 Mainz, Germany Abstract: Polycyclic aromatic hydrocarbons (PAHs) have attracted enormous interest due to their unique electronic and optoelectronic properties as well as the potential applications in organic electronics. This article reviews the progress in the modern synthesis of large PAHs with different sizes, shapes, edge structures, and substituents. Due to their outstanding self- organization characteristics, the discotic liquid-crystalline properties, self-assembled nanostructures on the surfaces, as well as the application in electronic devices will be discussed. Keywords: discotic liquid crystals; hexabenzocoronene; nanographene; polycyclic aromatic hydrocarbons; self-assembly. INTRODUCTION Polycyclic aromatic hydrocarbons (PAHs) are a class of unique compounds that consist of fused con- jugated aromatic rings and do not contain heteroatoms or carry substituents [1]. These compounds can be point source (e.g., oil spill) or non-point source (e.g., atmospheric deposition) and are one of the most widespread organic pollutants. Some of them are known or suspected carcinogens, and are linked to other health problems. They are primarily formed by incomplete combustion of carbon-containing fuels such as wood, coal, diesel, fat, tobacco, or incense [2,3]. Tar also contains PAHs. Different types of combustion yield different distributions of individual PAHs which can also give rise to isomers. Hence, those produced from coal combustion are in contrast to those yielded by motor-fuel combustion, which differ from those produced by forest fires.