This shows you the differences between two versions of the page.
| Next revision | Previous revision | ||
|
group5 [2014/06/06 17:32] utama created |
group5 [2014/06/16 13:56] (current) long |
||
|---|---|---|---|
| Line 1: | Line 1: | ||
| - | Group 5 Members : | ||
| - | - Adam Jones (Analysis) | ||
| - | - Alexander Long (Parameter) | ||
| - | - Raditya Utama (Code) | ||
| - | Project Title : | + | ====== HighFive ====== |
| + | ==== X-Ray Burst Simulation on Accreting Neutron Star ==== | ||
| + | (group 5) | ||
| + | **Members:** Alexander Long (Input Person), Adam Jones (Analysis Person), Raditya Utama (Code Person) | ||
| + | ==== Original Goals ==== | ||
| + | - Simulate Bondi accretion on VH1 with appropriate condition | ||
| + | - Run XRB reaction network on xnet | ||
| + | - Link the inputs and outputs between both simulations | ||
| + | - Plot some thermodynamic variables over time | ||
| + | - Study the effect of some parametric changes | ||
| + | |||
| + | ==== 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. | ||
| + | |||
| + | Some important parameters within VH1: | ||
| + | * 1D Spherically Symmetric: ngeom = 2 | ||
| + | * Reflective boundary at surface: nleft = 0 | ||
| + | * Fixed value boundary above neutron star: nright = 2 | ||
| + | * Minimum value of grid: Xmin = 10 km | ||
| + | * Maximum value of grid: Xmax = 50 km | ||
| + | |||
| + | ==== XNet ==== | ||
| + | |||
| + | |||
| + | |||
| + | |||
| + | |||
| + | ==== Presentation ==== | ||
| + | {{:highfive.pdf|Final Presentation for Group 5}} | ||