Structure of star-burst dendrimers: A comparison between small angle x-ray scattering and computer simulation results

Rathgeber, S.; Pakula, T.; Urban, V.

doi:10.1063/1.1768516

Journal Article

Structure of star-burst dendrimers: A comparison between small angle x-ray scattering and computer simulation results

Rathgeber, S.FZJ* ; Pakula, T.FZJ* ; Urban, V.FZJ*

2004
American Institute of Physics Melville, NY

The journal of chemical physics 121, 3840 - 3853 (2004) [10.1063/1.1768516]

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Please use a persistent id in citations: http://hdl.handle.net/2128/1190 doi:10.1063/1.1768516

Abstract: We investigated the generation dependent shape and internal structure of star-burst dendrimers under good solvent conditions using small angle x-ray scattering and molecular modeling. Measurements have been performed on poly(amidoamine) dendrimers with generations ranging from g=0 up to g=8 at low concentrations in methanol. We described the static form factor P(q) by a model taking into account the compact, globular shape as well as the loose, polymeric character of dendrimers. Monomer distributions within dendrimers are of special interest for potential applications and have been characterized by the pair correlation function gamma(r), as well as by the monomer and end-group density profile, rho(r) and rho(e)(r), respectively. Monomer density profiles and gamma(r) can be derived from P(q) by modeling and via a model independent approach using the inverse Fourier transformation algorithm first introduced by Glatter. Experimental results are compared with computer simulations performed for single dendrimers of various generations using the cooperative motion algorithm. The simulation gives direct access to gamma(r) and rho(r), allows an independent determination of P(q), and yields in addition to the scattering experiment information about the distribution of the end groups. Excellent qualitative agreement between experiment and simulation has been found.

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