Colliding Particles in Granular Material Flows

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Discussion Overview

The discussion revolves around the equations governing colliding particles in granular gas flows, specifically focusing on the calculation of post-collision velocities of identical spherical grains. The scope includes theoretical aspects of particle collisions and the application of conservation laws in different coordinate systems.

Discussion Character

  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant seeks assistance in calculating the change of velocity for colliding particles using a specific equation involving the restitution coefficient.
  • Another participant suggests rewriting velocity vectors in a coordinate system aligned with the collision interface to simplify the analysis, emphasizing that only the normal component of velocity is affected during the collision.
  • The second participant also mentions applying conservation of linear and angular momentum to derive new velocities and suggests consulting a specific textbook for a detailed derivation.
  • A third participant points out that the principles discussed are applicable in both 2D and 3D scenarios, provided the velocity vectors are transformed appropriately.

Areas of Agreement / Disagreement

The discussion does not appear to reach a consensus on the best approach to calculate the change in velocity, as participants offer different methods and references without resolving which is superior.

Contextual Notes

Participants reference specific assumptions about the particles being identical perfect spheres and the use of the restitution coefficient, but do not clarify the implications of these assumptions on the calculations.

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Hello Everyone

I am looking at equations of colliding particles in a granular gas and wondering how to calculate them.

We assume that the grains are identical perfect spheres (in R^3) of diameter D>0, (x,v) and (x-Dn,w) are their states before a collision, where n ε S^2 is the unit vector along the centre of both spheres, and x the position vector of the centre of the first sphere, e is the restitution coefficient which relates the normal components of the particle velocities before and after collision, the post collisional velocities (v*,w*) then are such that

(v*-w*)n = -e((v-w)n)

I was wondering how from this equation do we calculate the change of velocity for the colliding particles:

v* = v- 1/2(1+e)((v-w)n)n,

w* = w+ 1/2(1+e)((v-w)n)n

Many thanks to anyone that can help!
 
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First rewrite the existing velocity vectors (and angular momentum) from their native coordinate system to velocity vectors in the coordinate system connected to the collision interface. In this coordinate system, only the normal component of velocity is changed.
Then apply conservation of linear and angular momentum to get the new velocities and angular momentum and transform them back to the original coordinate system.

Look for instance in the book of Crowe, sommerfeld and Tsiu - multiphase flow with droplets and particles.
They have a nice derivation, including the effect of the angular velocity of the particles and the restitution coefficient.

There is also a result without much explanation on the wiki page for inelastic collision which you could use. This is just the rewritten conservation of momentum.
 
PS: I noticed that the wiki page on momentum has some explanation:
http://en.wikipedia.org/wiki/Momentum

Note that all these 1d equations hold true in 2d and 3d, when you transform the velocity vectors to the coordinate system connected to the collision interface
 
Sorry for the late reply, many thanks for the help!
 

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