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Cited article:

Formulating Compressive Strength of Dust Aggregates from Low to High Volume Filling Factors with Numerical Simulations

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The Astrophysical Journal 953 (1) 6 (2023)
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Tensile strength and surface energy of CO2 ice in the context of planet formation

M Fritscher and J Teiser
Monthly Notices of the Royal Astronomical Society 512 (3) 3754 (2022)
https://doi.org/10.1093/mnras/stac676

Planetesimal Formation in the Warm, Inner Disk: Experiments with Tempered Dust

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The Astrophysical Journal 837 (1) 59 (2017)
https://doi.org/10.3847/1538-4357/837/1/59

Free collisions in a microgravity many-particle experiment. III. The collision behavior of sub-millimeter-sized dust aggregates

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Icarus 225 (1) 75 (2013)
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FROM DUST TO PLANETESIMALS: AN IMPROVED MODEL FOR COLLISIONAL GROWTH IN PROTOPLANETARY DISKS

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The Astrophysical Journal 764 (2) 146 (2013)
https://doi.org/10.1088/0004-637X/764/2/146

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High Performance Computing in Science and Engineering ‘12 51 (2013)
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Growth and fragmentation of centimetre-sized dust aggregates: the dependence on aggregate size and porosity

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Planetesimal formation by sweep-up: how the bouncing barrier can be beneficial to growth

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Crossing barriers in planetesimal formation: The growth of mm-dust aggregates with large constituent grains

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Impact on porous targets: Penetration, crater formation, target compaction, and ejection

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Experiments on centimeter-sized dust aggregates and their implications for planetesimal formation

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Evolution of macroscopic dust agglomerates – Implications for planetesimal growth

J. Teiser, I. Engelhardt, M. Küpper, et al.
EAS Publications Series 58 213 (2012)
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