The compaction of highly porous dust agglomerates by a gas-velocity gradient and its application to dust growth in turbulent protoplanetary disks

Rainer Schräpler; Jürgen Blum; Daniyar Balapanov; Andrei Vedernikov

doi:https://doi.org/10.5194/epsc2024-72

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EPSC Abstracts

Vol. 17, EPSC2024-72, 2024, updated on 03 Jul 2024

https://doi.org/10.5194/epsc2024-72

Europlanet Science Congress 2024

© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The compaction of highly porous dust agglomerates by a gas-velocity gradient and its application to dust growth in turbulent protoplanetary disks

Rainer Schräpler¹, Jürgen Blum

¹, Daniyar Balapanov², and Andrei Vedernikov²

Rainer Schräpler et al.

¹Universität Braunschweig, Institut für Geophysik und extraterrestrische Physik, Germany (r.schraepler@tu-bs.de)
²Université Libre de Bruxelles, Microgravity Research Center, CP 165/62 Avenue F.D. Roosevelt 50,1050 Bruxelles, Belgium

How to cite: Schräpler, R., Blum, J., Balapanov, D., and Vedernikov, A.: The compaction of highly porous dust agglomerates by a gas-velocity gradient and its application to dust growth in turbulent protoplanetary disks, Europlanet Science Congress 2024, Berlin, Germany, 8–13 Sep 2024, EPSC2024-72, https://doi.org/10.5194/epsc2024-72, 2024.

This abstract has been withdrawn on 04 Jul 2024.