Title :
Effects of the charge-dipole interaction on the coagulation of fractal aggregates
Author :
Matthews, Lorin Swint ; Hyde, Truell W.
Author_Institution :
Center for Astrophys, Space Phys., & Eng. Res., Baylor Univ., Waco, TX, USA
fDate :
4/1/2004 12:00:00 AM
Abstract :
A numerical model with broad applications to complex (dusty) plasmas is presented. The self-consistent N-body code allows simulation of the coagulation of fractal aggregates, including the charge-dipole interaction of the clusters due to the spatial arrangement of charge on the aggregate. It is shown that not only does a population of oppositely charged particles increase the coagulation rate, the inclusion of the charge-dipole interaction of the aggregates as well as the electric dipole potential of the dust ensemble decreases the gelation time by a factor of up to 20. It is further shown that these interactions can also stimulate the onset of gelation, or "runaway growth," even in a population of particles charged to a monopotential where previously it was believed that like-charged grains would inhibit coagulation. Gelation is observed to occur due to the formation of high-mass aggregates with fractal dimensions greater than two, which act as seeds for runaway growth.
Keywords :
coagulation; dusty plasmas; fractals; plasma simulation; charge-dipole cluster interaction effects; charged particles; coagulation rate; complex dusty plasmas; dust ensemble; electric dipole potential; fractal aggregate coagulation; fractal dimensions; gelation time; high-mass aggregates; like-charged grains; monopotential; runaway growth; self-consistent N-body code; spatial charge arrangement; Aggregates; Coagulation; Dusty plasma; Electrons; Fractals; Physics; Planets; Plasma chemistry; Plasma density; Plasma temperature; Complex; dust coagulation; dusty; fractal aggregates; plasma; preplanetary dust aggregation;
Journal_Title :
Plasma Science, IEEE Transactions on
DOI :
10.1109/TPS.2004.826107