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Astron. Astrophys. 325, 857-865 (1997) 4. Modified bulk viscosityA smoothed quantity can be calculated at any point in the fluid by
Eq. (1). The smoothed velocity at If this point coincides with a position for a particle, the smoothed and the particle's individual velocity will be different in general. This difference is used to construct a modified bulk viscosity. Benz (1990) suggests that this quantity could be used when integrating the position to prevent interparticle penetration. It is true that it prevents interparticle penetration, but it unfortunately introduces conservation problems when the particles are not moved at their individal velocity. If the contribution from particle i subtracted, it does however say something about the fluid around the particle. The smoothed velocity at r can then be redefined as where In the standard formulation of the bulk artificial viscosity particle i interacts with each neighbour separately, where the acceleration and time derivative of the internal energy is added to the particle as described in Sect. 2. This introduces problems described in Sect. 3. The individual velocity of particle i can then be seen as a deviation from the smoothed value at the particle's position and the artificial viscosity as a correction to the individual velocity. I propose a modified bulk viscosity to replace the standard bulk viscosity, where the fluid around the particle is considered from a collective contribution from the neighbours in one single interaction. This modified bulk artificial viscosity is defined as where Now consider the integration of the velocitites and internal energy
density from time which gives the change in kinetic energy for particle i: If to conserve the total energy. The artificial also must prevent particle penetration. The modified
artificial viscosity is calculated with respect to an integrated mean
of the neighbours. Therefore a particle will move less than
If the particles i and j are each others neighbours and that their other neighbours give the same contribution to their respective velocities, one concludes from Eq. (15) and (16) that the impulse is conserved. Their other neighbours do, however, not give the same contribution, due to the limited resolution. Tests of self gravitating rotating disks show that the angular momentum and impulse are well conserved. ![]() ![]() ![]() ![]() © European Southern Observatory (ESO) 1997 Online publication: April 28, 1998 ![]() |