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group5 [2014/06/09 14:13] utama |
group5 [2014/06/16 13:56] long |
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- | Group 5 Members : | ||
- | - Adam Jones (Analysis) | ||
- | - Alexander Long (Parameter) | ||
- | - Raditya Utama (Code) | ||
- | Project Title : | + | ====== HighFive ====== |
- | X-Ray Burst Simulation on Accreting Neutron Star | + | ==== X-Ray Burst Simulation on Accreting Neutron Star ==== |
+ | (group 5) | ||
- | Step : | + | **Members:** Alexander Long (Input Person), Adam Jones (Analysis Person), Raditya Utama (Code Person) |
- | - Simulate Bondi accretion on VH1 with appropriate condition | + | |
- | - Run XRB reaction network on xnet | + | ==== Original Goals ==== |
- | - Link the inputs and outputs between both simulations with | + | - Simulate Bondi accretion on VH1 with appropriate condition |
- | - Plot some thermodynamic variables over time | + | - Run XRB reaction network on xnet |
- | - Study the effect of some parametric changes | + | - 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}} | ||
- | 06/09/2014 |