 | Computational Physics (Pioneer Batch of CHEP 2004-08 Spring) BSc(Hons) Computational Physics at Centre for High Energy Physics University of the Punjab Lahore Pakistan |
 | Computational Physics (CHEP's first Annual Dinner 22-Dec-05) Centre for High Energy Physics University of the Punjab Lahore Pakistan |
 | Liquid nitrogen in a puddle of water We pour some liquid nitrogen in a puddle of water that formed on the roof right outside of the Computational Physics Lab that was being used neither for computation nor for physics. Well, I guess physics was happening. Although it's a little difficult to tell when watching, the liquid nitrogen formed lots of small, twirling bubbles and moved through out the water, looking pretty nifty. Some of these bubbles were mercilessly slaughtered by Monica with the knife. |
 | Two fluid jets www.matyka.pl - Simulations in Physics. Incompressible free surface flow done with SIMPLE based method. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Driven Cavity www.matyka.pl - Simulations in Physics. Flow in driven cavity simulation done with my SIMPLE based solver. Visualization made using massless tracers. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Tunnel SIMPLE flow (Navier--Stokes) www.matyka.pl - Incompressible fluid flow done with one of my fluid solvers. This one created with SIMPLE (Semi Implicit Method for Pressure Linked Equations). Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Broken Dam Simulation www.matyka.pl - Simulations in Physics. Free surface broken dam simulation done with my SIMPLE based solver. Visualization made using massless tracers. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Star formation by collapse of molecular clouds Simulation by SPH of the collapse and fragmentation of a molecular cloud presented in "The Formation of Stars and Brown Dwarfs and the Truncation of Protoplanetary Discs in a Star Cluster" by Matthew R. Bate, Ian A. Bonnell, and Volker Bromm (http://www.ukaff.ac.uk/starcluster/). The calculation models the collapse and fragmentation of a molecular cloud with a mass 50 times that of our Sun. The cloud is initially 1.2 light-years (9.5 million million kilometres) in diameter, with a temperature of 10 Kelvin (-263 degrees Celsius). |
 | Shroedinger Wave Packets www.matyka.pl - Simulations in Physics. I've done it to test some numerical methods for partial differential equations of Shroedinger type. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Knee Flow Re=200 www.matyka.pl - Simulations in Physics. Flow trough knee shaped tunnel simulation done with my SIMPLE based solver. Visualization made using massless tracers. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Flow trough pipes Re=149 www.matyka.pl - Simulations in Physics. Flow trough a set of pipes done with my SIMPLE based solver. Visualization made using massless tracers. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
 | Knee Flow Re=200 www.matyka.pl - Simulations in Physics. Flow trough knee shaped tunnel simulation done with my SIMPLE based solver. Visualization made using massless tracers. Written in C++ by Maciej Matyka: maciej.matyka [] gmail.com |
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