Physical properties of particle agglomerates with respects to the planet formation process
Final Report Abstract
The project has dealt with two important aspects of dust with respect to the planet formation process. In a first part we have performed molecular dynamics simulations to of dust agglomerates, that consisted of a large number of individual monomers. After careful calibration we used this direct method to calculate continuum properties of dust agglomerates such as tensile and shear strength that are difficult to access experimentally. By considering collisions between agglomerates we could show that bouncing between particles occurs only for large filling factor and low velocities, and that the fragmentation barrier can be shifted to 10m/s, and beyond for non-equal collision partners. Both effects tend to relax the bouncing as well as fragmentation barrier. In the second part we studied the interaction of the dust with the ambient gas in turbulent disks that are driven by the VSI. Here, we find first a strong bunching of the particles in the turbulent eddies (rolls), and secondly relative velocities of about 10m/s that would just allow for further particles growth. Wit respect to the stochastic nature of the flow, we could show that the turbulence is strongly anisotropic. Embedded planets experience a faster inward migration than classical type I. We have extended the study of embedded planets by including the accretion properties of dust particles.
Publications
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Compression behavior of porous dust agglomerates, 2012, A&A 541, A59
Seizinger, A.; Speith, R. & Kley, W.
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The Physics of Protoplanetesimal Dust Agglomerates. VII. The Low-velocity Collision Behavior of Large Dust Agglomerates, 2012, ApJ 758, id.35
Schräpler, R.; Blum, J.; Seizinger, A. & Kley, W.
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2013, The properties of dust agglomerates, Dissertation, University of Tübingen
Seizinger, A.
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Bouncing behavior of microscopic dust aggregates, 2013, A&A 551, A65
Seizinger, A. & Kley, W.
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Erosion of dust aggregates, 2013, A&A 560, A45
Seizinger, A.; Krijt, S. & Kley, W.
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Tensile and shear strength of porous dust agglomerates, 2013, A&A 559, A19
Seizinger, A.; Speith, R. & Kley, W.
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Bridging the Gap Between Hydrocodes, 2015, LPI Contribution No. 1861, p.1082
Martellato, E.; Schäfer, C.; Wandel, O.; Cremonese, G. & Kley, W.
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Particle dynamics in discs with turbulence generated by the vertical shear instability, 2016, A&A 594, A57
Stoll, M.H.R. & Kley, W.
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2017, Dynamics of Dust and Planets in turbulent Accretion Disks, Dissertation, University of Tübingen
Stoll, M.
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Anisotropic hydrodynamic turbulence in accretion disks, 2017, A&A 599, L6
Stoll, M.H.R.; Kley, W. & Picogna, G.
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Planet-disc interaction in laminar and turbulent discs, 2017, A&A 604, A28
Stoll, M.H.R.; Picogna, G. & Kley, W.