User Tools

Site Tools


group5

Differences

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

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
group5 [2014/06/09 14:13]
utama
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+==== 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 
group5.1402337589.txt.gz · Last modified: 2014/06/09 14:13 by utama