This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision | |||
| 
                    group5 [2014/06/16 13:21] long  | 
                
                    group5 [2014/06/16 13:56] (current) long  | 
            ||
|---|---|---|---|
| Line 6: | Line 6: | ||
| **Members:** Alexander Long (Input Person), Adam Jones (Analysis Person), Raditya Utama (Code Person) | **Members:** Alexander Long (Input Person), Adam Jones (Analysis Person), Raditya Utama (Code Person) | ||
| - | ==== Starting Procedure ==== | + | ==== Original Goals ==== | 
| - Simulate Bondi accretion on VH1 with appropriate condition | - Simulate Bondi accretion on VH1 with appropriate condition | ||
| - Run XRB reaction network on xnet | - Run XRB reaction network on xnet | ||
| - | - Link the inputs and outputs between both simulations with | + | - Link the inputs and outputs between both simulations  | 
| - Plot some thermodynamic variables over time | - Plot some thermodynamic variables over time | ||
| - Study the effect of some parametric changes  | - Study the effect of some parametric changes  | ||
| - | ==== Bondi Accretion Model ==== | + | ==== VH1 and Bondi Accretion Model ==== | 
| To simulate the accretion of matter onto the surface of a neutron star in a binary system we decided to use VH1 setup with a Bondi accretion model.  | To simulate the accretion of matter onto the surface of a neutron star in a binary system we decided to use VH1 setup with a Bondi accretion model.  | ||
| Line 24: | Line 24: | ||
| * Maximum value of grid: Xmax = 50 km | * Maximum value of grid: Xmax = 50 km | ||
| + | ==== XNet ==== | ||
| + | |||