N-particle-simulations of dust growth: I. growth driven by brownian motion

Icarus

Volumn 141, Issue 2, 1999, Pages 388-398

  Kempf, Sascha ^a,b   Pfalzner, Susanne ^b   Henning, Thomas K ^b  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b FRIEDRICH SCHILLER UNIVERSITY JENA   (Germany)

Author keywords

Computer techniques; Planetary formation; Planetesimals; Solar nebula

Indexed keywords

EID: 0033209530     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.1999.6171     Document Type: Article

References (36)

1. Bell K. R., Cassen P. M., Klahr H. H., Henning Th. The structure and appearance of protostellar accretion disks: Limits on disk flaring. Astrophys. J. 486:1997;372-387.
2. Blum J., Wurm G., Kempf S., Henning Th. The Brownian motion of dust particles in the solar nebula. Icarus. 124:1996;441-451.
3. Blum, J., G. Wurm, T. Poppe, and L. Heim1999. Aspects of laboratory dust aggregation with relevance to the formation of planetesimals. In Laboratory Astrophysics and Space ResearchP. Ehrenfreud, H. Kochan, K. Krafft, and V. Pirronello, Eds. pp. 399-425. Kluwer Academic, Dordrecht.
4. Brown W., Ball R. Computer simulation of chemically limited aggregation. J. Phys. A18:1985;L517-L521.
5. Chandrasekhar S. Stochastic problems in physics and astronomy. Rev. Mod. Phys. 15:1943;1-89.
6. Chokshi A., Tielens A., Hollenbach D. Dust coagulation. Astrophys. J. 407:1993;806-819.
7. Cuzzi J., Dobrovolskis A., Champney J. Particle-gas dynamics in the midplane of the solar nebula. Icarus. 106:1993;102-134.
8. Epstein P. On the resistance experienced by spheres in their motion through gases. Phys. Rev. 22:1923;710-733.
9. Ermak D., Buckholz H. Numerical integration of the Langevin equation: Monte Carlo simulation. J. Comp. Phys. 35:1980;169-182.
10. Goldreich P., Ward W. The formation of planetesimals. Astrophys. J. 183:1973;1051-1061.
11. Johnson K., Kendall K., Roberts A. Surface energy and the contact of elastic solids. Proc. R. Soc. Lond. A. 324:1971;301-313.
12. Kang K., Redner S., Meakin P., Leyvraz F. Long-time crossover phenomena in coagulation kinetics. Phys. Rev. A. 33:1986;1171-1182.
13. Kempf S. Mikrophysik und Dynamik des Brownschen Staubwachstums in protoplanetaren Scheiben. 1998.
14. Kempf S., Pfalzner S. An effective algorithm for simulating diffusion-driven aggregation. Comput. Phys. Commun. 1999.
15. Kempf, S., S. Pfalzner, and Th. Henning1996. Self-consistent simulation of the Brownian stage of dust growth. In From Stardust to PlanetesimalsY. Pendleton and A. Tielens, Eds., pp. 163-166. ASP, San Francisco.
16. Kolb M. Unified description of static and dynamic scaling for kinetic cluster formation. Phys. Rev. Lett. 53:1984;1653-1665.
17. Leyvraz F. Large-time behavior of the Smoluchowski equation of coagulation. J. Phys. A18:1984;L941-L945.
18. Markiewicz W. J., Mizuno H., Voelk H. J. Turbulence induced relative velocity between two grains. Astron. Astrophys. 242:1991;286-289.
19. Meakin P. Effects of cluster trajectories on cluster-cluster aggregation: A comparsion of linear and Brownian trajectories in two- and three-dimensional simulations. Phys. Rev. A. 29:1984;997-999.
20. Meakin P. Fractal aggregates in geophysics. Rev. Geophys. 29:1991;317-354.
21. Mizuno H., Markiewicz W., Völk H. Grain growth in turbulent protoplanetary accretion disks. Astron. Astrophys. 195:1988;183-192.
22. Mountain R., Mulholland W., Baum H. Simulation of aerosol agglomeration in the free molecular and continuum flow regime. J. Colloid Interface Sci. 114:1986;67-81.
23. Ossenkopf V. Dust coagulation in dense molecular clouds: The formation of fluffy grains. Astron. Astrophys. 280:1993;617-646.
24. Ruden S., Pollack J. The dynamical evolution of the protosolar nebula. Astrophys. J. 375:1991;740-760.
25. Sablotny R. Über den Einfluß der Koagulation von Staubteilchen auf die Chemie in kalten Molekülwolken. 1996.
26. Safronov V. Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets. 1972.
27. Shakura N., Sunyaev R. Black holes in binary systems: Observational appearance. Astron. Astrophys. 24:1973;337-355.
28. Smirnov B. The properties of fractal clusters. Phys. Rep. 188:1990;1-78.
29. Smoluchowski M. Versuch einer mathematischen Theorie der Koagulationskinetik kolloider Lösungen. Z. Phys. Chemie. 92:1917;129-168.
30. van Dongen P. Upper critical dimension in irreversible aggregation. Phys. Rev. Lett. 63:1989;1281-1284.
31. Vicsek T. Fractal Growth Phenomena. 1992.
32. Vicsek T., Family F. Dynamic scaling for aggregation of clusters. Phys. Rev. Lett. 52:1984;1669-1672.
33. Völk H., Jones F., Morfill G., Röser. Collisons of grains in a turbulent gas. Astron. Astrophys. 85:1980;316-325.
34. Weidenschilling S. Evolution of grains in a turbulent solar nebula. Icarus. 60:1984;533-557.
35. Wurm G., Blum J. Experiments on preplanetary dust aggregation. Icarus. 132:1998;125-136.
36. Ziff, R. 1984, Aggregation kinetics via smoluchowski's equation. In, Kinetics of Aggregation and Gelation, F. Family and D. Landau, Eds, North Holland, Amsterdam.