Numerical simulations of highly porous dust aggregates in the low-velocity collision regime

Astronomy and Astrophysics

Volumn 513, Issue 11, 2010, Pages

  Geretshauser, R J ^a   Speith, R ^a   Guttler C ^b   Krause, M ^b   Blum, J ^b  

^a UNIVERSITY OF TÜBINGEN   (Germany)

^b TECHNICAL UNIVERSITY OF BRAUNSCHWEIG   (Germany)

Author keywords

Hydrodynamics; Methods: laboratory; Methods: numerical; Planets and satellites: formation; Protoplanetary disks

Indexed keywords

AGGLOMERATION; AGGREGATES; COMPACTION; COMPRESSIVE STRENGTH; COMPUTER SIMULATION; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; FLUID DYNAMICS; HYDRODYNAMICS; MATHEMATICAL MODELS; NUMERICAL METHODS; PLANETS; SATELLITES; SILICON COMPOUNDS; VAN DER WAALS FORCES; VELOCITY;

BULK MODULUS; CALIBRATION PROCESS; COEFFICIENT OF RESTITUTION; COMPUTER PROGRAM; DENSITY STRUCTURES; DUST GRAINS; FRAGMENT MASS DISTRIBUTION; GAS FLOWS; HIGH VELOCITY; LOW-VELOCITY; LOW-VELOCITY COLLISION; MACROSCOPIC MATERIALS; METHODS: LABORATORY; NUMERICAL SCHEME; NUMERICAL SIMULATION; PLANETS AND SATELLITES: FORMATION; PLASTIC PROPERTY; POROSITY MODELS; POROUS OBJECT; PROTOPLANETARY DISKS; RELATIVE VELOCITY; SIMULATED DUST; SMOOTH PARTICLE HYDRODYNAMICS; SOLID BODIES; SPH CODE;

EXPERIMENTS;

EID: 77951869201     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913596     Document Type: Article

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