scholarly journals Theoretical Analysis of Effects of π-Conjugating Substituents on Building Blocks for Conducting Polymers

1999 ◽  
Vol 64 (20) ◽  
pp. 7419-7425 ◽  
Author(s):  
Ulrike Salzner ◽  
J. B. Lagowski ◽  
P. G. Pickup ◽  
R. A. Poirier
Keyword(s):  
Theoretical Analysis ◽  
Conducting Polymers ◽  
Building Blocks

β-Terthiophene aldehyde and phosphonate: key building blocks for the synthesis of functionalised conducting polymers

2001 ◽  
Vol 42 (49) ◽  
pp. 8733-8735 ◽  
Author(s):  
Gavin E Collis ◽  
Anthony K Burrell ◽  
David L Officer
Keyword(s):  
Conducting Polymers ◽  
Building Blocks

Synthesis and characterization of β,β’-dimethylated dithieno[3,2-b:2’,3’-d]pyrroles and their corresponding regioregular conducting electropolymers

2021 ◽  
Author(s):  
Peter Baeuerle ◽  
Sebastian Foertsch ◽  
Elena Mena-Osteritz
Keyword(s):  
Conducting Polymers ◽  
Quantum Chemical Calculations ◽  
Quantum Chemical ◽  
Building Blocks ◽  
Synthesis And Characterization ◽  
Organic Electronic ◽  
Functional Dyes

β,β’-Dimethyl-substituted dithieno[3,2-b:2’,3’-d]pyrroles (Me-DTP) 2-7 represent novel electron-rich building blocks, which were converted to corresponding conducting polymers p(Me-DTP) and to functional dyes for organic electronic applications. Supported by quantum chemical calculations,...

New derivatives of phenylamine as novel building blocks of conducting polymers

2009 ◽  
Vol 159 (21-22) ◽  
pp. 2202-2204 ◽  
Author(s):  
Mieczyslaw Lapkowski ◽  
Sylwia Golba ◽  
Jadwiga Soloducho ◽  
Krzysztof Idzik
Keyword(s):  
Conducting Polymers ◽  
Building Blocks ◽  
Derivatives Of

scholarly journals Conducting materials as building blocks for electronic textiles

MRS Bulletin ◽  
2021 ◽  
Author(s):  
Anja Lund ◽  
Yunyun Wu ◽  
Benji Fenech-Salerno ◽  
Felice Torrisi ◽  
Tricia Breen Carmichael ◽  
...  
Keyword(s):  
Conducting Polymers ◽  
2D Materials ◽  
Building Blocks ◽  
Elastic Fibers ◽  
Electronic Textiles ◽  
Metal Electrodes ◽  
Active Materials ◽  
Textile Materials ◽  
Conducting Materials ◽  
Electrochemically Active

Abstract To realize the full gamut of functions that are envisaged for electronic textiles (e-textiles) a range of semiconducting, conducting and electrochemically active materials are needed. This article will discuss how metals, conducting polymers, carbon nanotubes, and two-dimensional (2D) materials, including graphene and MXenes, can be used in concert to create e-textile materials, from fibers and yarns to patterned fabrics. Many of the most promising architectures utilize several classes of materials (e.g., elastic fibers composed of a conducting material and a stretchable polymer, or textile devices constructed with conducting polymers or 2D materials and metal electrodes). While an increasing number of materials and devices display a promising degree of wash and wear resistance, sustainability aspects of e-textiles will require greater attention. Graphical abstract

Photochemical Evolution of Interstellar/Precometary Organic Material

1997 ◽  
Vol 161 ◽  
pp. 23-47 ◽  
Author(s):  
Louis J. Allamandola ◽  
Max P. Bernstein ◽  
Scott A. Sandford
Keyword(s):  
Origin Of Life ◽  
Building Blocks ◽  
Complex Species ◽  
Infrared Observations ◽  
Interstellar Ice ◽  
Polycyclic Aromatic ◽  
Ultraviolet Photolysis ◽  
The Origin Of Life ◽  
Simple Molecules ◽  
Complex Organic

AbstractInfrared observations, combined with realistic laboratory simulations, have revolutionized our understanding of interstellar ice and dust, the building blocks of comets. Since comets are thought to be a major source of the volatiles on the primative earth, their organic inventory is of central importance to questions concerning the origin of life. Ices in molecular clouds contain the very simple molecules H2O, CH3OH, CO, CO2, CH4, H2, and probably some NH3and H2CO, as well as more complex species including nitriles, ketones, and esters. The evidence for these, as well as carbonrich materials such as polycyclic aromatic hydrocarbons (PAHs), microdiamonds, and amorphous carbon is briefly reviewed. This is followed by a detailed summary of interstellar/precometary ice photochemical evolution based on laboratory studies of realistic polar ice analogs. Ultraviolet photolysis of these ices produces H2, H2CO, CO2, CO, CH4, HCO, and the moderately complex organic molecules: CH3CH2OH (ethanol), HC(= O)NH2(formamide), CH3C(= O)NH2(acetamide), R-CN (nitriles), and hexamethylenetetramine (HMT, C6H12N4), as well as more complex species including polyoxymethylene and related species (POMs), amides, and ketones. The ready formation of these organic species from simple starting mixtures, the ice chemistry that ensues when these ices are mildly warmed, plus the observation that the more complex refractory photoproducts show lipid-like behavior and readily self organize into droplets upon exposure to liquid water suggest that comets may have played an important role in the origin of life.

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