Differences

This shows you the differences between two versions of the page.

--- group5 [2014/06/13 10:59]
long
+++ group5 [2014/06/16 13:56]
long
@@ Line 6: / Line 6: @@
 **Members:** Alexander Long (Input Person), Adam Jones (Analysis Person), Raditya Utama (Code Person)
-==== Procedure ====
+==== Original Goals ====
   - Simulate Bondi accretion on VH1 with appropriate condition
   - 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
   - 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}}

Talent