MATERIALS MODEL- ING VIA MASSIVELY PARALLEL MOLECU- LAR DYNAMICS At Los Alamos, we have embarked upon a program to study the behavior of materials under the influence of external stresses and heat flow, using the method of molecular dynamics (MD), where the motion of millions of strongly interacting atoms or molecules is followed on a computer. Because the complex flow phenomena occur on much larger distance scales than do molecular sizes and spacings, and because the time scales of interest are much longer than are vibrational peri- ods or mean collision times, we are using the massively parallel CM-5 at the ACL for these simulations. On the earlier version of this machine (CM-2), we were able to carry out preliminary simulations of 106 atoms for over 1000 vibrational periods, using some 50 hours of cpu time. For these 2D calcula- tions, the linear dimension is 0.3 micrometers, and the physical time duration is a nanosecond. In fact, we have shown that 8 x 106 atoms are feasi- ble on the CM-2, and 3 x 107 atoms can be simulated on the CM-5, which is estimated to be capable of 10 times the clock speed of the CM-2 by the end of 1992. This order of magnitude increase in both size and speed of the CM-5 rela- tive to the CM-2 is comparable to the relative advantages of the CM-2 over the single-processor Cray Y-MP. On the CM-5, we may be able to extend the physical time simulated to 0.1 ms, for cpu times of less than 200 hours. The Fortran 90 MD code on the Con- nection Machines has been written in such a way that a variety of geometries (initial conditions) and external driving forces (boundary conditions) are easily implemented. For bulk materials, where periodic boundary conditions are appropriate, three distinct kinds of dynamics are available: (1) the usual Newtonian equations of motion (micro- canonical ensemble - NVE - constant number of particles N, constant volume V, constant total energy E, as well as constant total linear momentum); (2) isothermal Nose'-Hoover MD (canoni- cal ensemble - NVT - where T is the temperature of the heat bath); and (3) isothermal-isobaric Nose'-Hoover MD (NPT - where P is the diagonal of the pressure tensor). In addition to these special ensemble dynamics, the peri- odic boundaries under Newtonian mechanics can be moved at constant independent velocities. If correspond- ing velocity gradients are imposed upon the peculiar momenta of the atoms, homogeneous adiabatic expan- sion can be simulated; otherwise, inho- mogeneous shock waves can be generated. Moreover, boundary-driven flows, such as either Couette shear flow or heat flow between hot and cold walls, can be simulated. Simple geo- metric objects (e.g., free surfaces, spheres, and plates) can be generated and given body velocities. Input to the code at setup time and for restarts is uncomplicated, and modifications of the MD code to do more complicated initial and boundary conditions is not difficult. The particle positions and momenta are updated by integrating the equa- tions of motion via the Stoermer (or Verlet) method of finite central differ- ences. In the case of Nose'-Hoover dynamics, the handful of global control variables for coupling of the thermostat and barostat are also easily handled by the Stoermer method. In addition to being time-reversible and very robust (e.g., energy and linear momentum are well conserved over long trajectory times), Stoermer integration minimizes memory requirements to arrays for the phase (particle coordinates and momenta) and forces, plus the few sca- lars for the Nose'-Hoover coupling variables. We have applied this parallel MD code to shock-wave propagation, annealing of polycrystalline materials, and spalla- tion phenomena (fracture). Shock-wave simulations revealed similar induced plasticity for ductile materials, whose atoms interact via a many-body embed- ded-atom method (EAM) potential appropriate for metals, compared with brittle pair-potential materials - at least in 2D, where dislocations are more eas- ily formed than in 3D. The annealing calculations demonstrate that coarsen- ing of grains proceeds by the motion of grain boundaries in the direction of concavity (big grains gobble up little ones), so that the average linear dimen- sion grows with time t like t0.3. Spalla- tion occurs when a thin plate of material hits a thicker target at suffi- cient velocity. The shock waves gener- ated on impact are relieved by rarefaction waves at the free surfaces opposite the impact plane. When the rarefactions meet at the spall plane, the material is put into tension; if the impact is hard enough, the material expands until it breaks. Our MD simu- lations showed that homogeneous uniaxial adiabatic expansion (linear velocity profile about the spall plane) is an excellent approximation. Moreover, a simple dislocation-motion model accounts well for the stress at failure, as a function of the imposed strain rate. We are planning to apply this versatile MD code (in both 2D and 3D) to a wide variety of interesting phenomena, including fracture under various exter- nal driving forces, dislocation genera- tion at crack tips, shock-wave-induced plasticity in granular (polycrystalline) solids, ablation of surfaces by radiation (in collaboration with 3M), chemically reactive flow (as in detonation waves, in collaboration with the Naval Research Laboratory), and polymer dynamics problems, including simula- tion of the flow of colloidal suspensions (in collaboration with du Pont). Many of these applications directly impact the development and manufacturing of novel materials by American industry. The first sequence (TXY) shows a MD simula- tion of shock wave in a 2D Lennard- Jones solid. Particle velocities are col- ored by a rainbow ranging from -up (deep blue) to 0 (blue-green) to +up (bright red), where up is the piston velocity. The shock front moves to the right at the shock velocity (us) which is greater than the speed of sound; the piston is at the far left. An elastic pre- cursor has almost reached the right- hand edge of the window, which includes about 1/3 of the total number of atoms (65K). The plastic wave is near the midpoint of the window. The second sequence (V) shows a MD shock- wave simulation. Local crystal orienta- tion for each particle (hexagonal sym- metry is assumed) is colored by a rainbow ranging from -30 deg. relative to the horizontal (deep blue) to 0 deg. (blue- green) to + 30 deg. (bright red). Shock- induced dislocation generation is apparent near the midpoint of the window (plastic wave front); disloca- tion cores appear as localized spots. Acknowledgement: Brad Holian, LANL, T-12