group5

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 group5 [2014/06/13 10:59]long group5 [2014/06/16 13:56] (current)long Both sides previous revision Previous revision 2014/06/16 13:56 long 2014/06/16 13:21 long 2014/06/13 10:59 long 2014/06/09 14:15 utama 2014/06/09 14:13 utama 2014/06/06 17:32 utama created Next revision Previous revision 2014/06/16 13:56 long 2014/06/16 13:21 long 2014/06/13 10:59 long 2014/06/09 14:15 utama 2014/06/09 14:13 utama 2014/06/06 17:32 utama created 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) - ==== 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  ​ + ==== 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}}
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