We present a new model for the fragmentation of dust beds in laboratory shock tube experiments. The model successfully explains the formation of layers in the bed using mass and momentum conservation. Our model includes the effect of wall friction, inherent cohesion, and gravitational overburden. We find that the pressure changes caused by the expansion wave take time to penetrate into the bed, while simultaneously increasing in magnitude. By the time the pressure difference is large enough to overcome wall friction, the overburden and the intrinsic cohesion of the bed, it has penetrated ~8-15 bead diameters into the bed, thus causing a layer of dust to be lifted off. We have found the dependence of layer size upon bead diameter and found a...
In interstellar and interplanetary space, the size distribution and composition of dust grains play ...
Presented at: Twenty-first International Colloquium on the Dynamics of Explosions and Reactive Syste...
The cores in molecular clouds are the densest and coldest regions of the interstellar medium (ISM). ...
We present a new model for the fragmentation of dust beds in laboratory shock tube experiments. The ...
Results of numerical simulation of the shock wave passing along a dusty layer are presented; the sim...
In recent years, dynamics of dust lifting behind a passing shock wave have been studied extensively....
Dust explosion hazards in areas where combustible dusts are found have caused loss of life and halte...
The thesis deals with the first stage of planet formation, namely dust coagulation from micron to mi...
Context. There is a long-standing and large discrepancy between the timescale for dust formation aro...
A prefluidized sand bed consisting of fine particles compactifies when it is subjected to a shock. W...
Knowledge-based modeling of dust lifting behind shock waves is a prerequisite for realistic simulati...
Context. The formation of planetesimals is often accredited to the collisional sticking of dust grai...
International audienceWe model the coagulation and fragmentation of dust grains during the protostel...
To treat the problem of growing protoplanetary disc solids across the meter barrier, we consider a v...
Previous work on protoplanetary dust growth shows a halt at centimeter sizes owing to the occurrence...
In interstellar and interplanetary space, the size distribution and composition of dust grains play ...
Presented at: Twenty-first International Colloquium on the Dynamics of Explosions and Reactive Syste...
The cores in molecular clouds are the densest and coldest regions of the interstellar medium (ISM). ...
We present a new model for the fragmentation of dust beds in laboratory shock tube experiments. The ...
Results of numerical simulation of the shock wave passing along a dusty layer are presented; the sim...
In recent years, dynamics of dust lifting behind a passing shock wave have been studied extensively....
Dust explosion hazards in areas where combustible dusts are found have caused loss of life and halte...
The thesis deals with the first stage of planet formation, namely dust coagulation from micron to mi...
Context. There is a long-standing and large discrepancy between the timescale for dust formation aro...
A prefluidized sand bed consisting of fine particles compactifies when it is subjected to a shock. W...
Knowledge-based modeling of dust lifting behind shock waves is a prerequisite for realistic simulati...
Context. The formation of planetesimals is often accredited to the collisional sticking of dust grai...
International audienceWe model the coagulation and fragmentation of dust grains during the protostel...
To treat the problem of growing protoplanetary disc solids across the meter barrier, we consider a v...
Previous work on protoplanetary dust growth shows a halt at centimeter sizes owing to the occurrence...
In interstellar and interplanetary space, the size distribution and composition of dust grains play ...
Presented at: Twenty-first International Colloquium on the Dynamics of Explosions and Reactive Syste...
The cores in molecular clouds are the densest and coldest regions of the interstellar medium (ISM). ...