Context. Dust aggregates consist of polydisperse grains following a power-law size distribution with an exponent of around 2.5, called the Mathis-Rumpl-Nordsieck (MRN) distribution. Aims. We compare the outcome of collisions between polydisperse granular aggregates with those of monodisperse aggregates. Methods. Granular-mechanics simulations were used to study aggregate collisions. Results. Both with respect to the fragmentation threshold and to energy dissipation, MRN aggregates behave as monodisperse aggregates if their size corresponds approximately to the geometric mean of the largest and smallest radius of the MRN distribution. Conclusions. Our results allow the polydisperse aggregates to be substituted with monodisperse aggregates, w...
We investigate disruptive collisions of aggregates comprised of particles with different interaction...
Particles in Saturn's main rings range in size from dust to kilometer-sized objects. Their size dist...
<p>We study the aggregation of monomers in an aerosol via non-dimensional Langevin simulations, in w...
Context. Dust aggregates consist of polydisperse grains following a power-law size distribution with...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charact...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charac...
Context. Collisions between porous dust aggregates are crucial for the evolution of protoplanetary d...
Context. Collisions between dust particles may lead to agglomerate growth or fragmentation, dependin...
We carry out three-dimensional Smoothed Particle Hydrodynamics simulations of spherical homogeneous ...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
Context. The collisional evolution of submillimeter-sized porous dust aggregates is important in man...
Context. Collisional growth of dust aggregates is an essential process in forming planetes...
Inelastic particles are used to model the behavior of granular media. On the level of individual gra...
International audienceBy means of the contact dynamics method together with a particle fracture mode...
We investigate disruptive collisions of aggregates comprised of particles with different interaction...
Particles in Saturn's main rings range in size from dust to kilometer-sized objects. Their size dist...
<p>We study the aggregation of monomers in an aerosol via non-dimensional Langevin simulations, in w...
Context. Dust aggregates consist of polydisperse grains following a power-law size distribution with...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charact...
The coagulation of dust aggregates occurs in various astrophysical environments. Each one is charac...
Context. Collisions between porous dust aggregates are crucial for the evolution of protoplanetary d...
Context. Collisions between dust particles may lead to agglomerate growth or fragmentation, dependin...
We carry out three-dimensional Smoothed Particle Hydrodynamics simulations of spherical homogeneous ...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
Context. Bouncing collisions of dust aggregates within the protoplanetary disk may have a significan...
Context. The collisional evolution of submillimeter-sized porous dust aggregates is important in man...
Context. Collisional growth of dust aggregates is an essential process in forming planetes...
Inelastic particles are used to model the behavior of granular media. On the level of individual gra...
International audienceBy means of the contact dynamics method together with a particle fracture mode...
We investigate disruptive collisions of aggregates comprised of particles with different interaction...
Particles in Saturn's main rings range in size from dust to kilometer-sized objects. Their size dist...
<p>We study the aggregation of monomers in an aerosol via non-dimensional Langevin simulations, in w...