Changes between Version 1 and Version 2 of UGT2010


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Timestamp:
Feb 12, 2012 2:42:30 PM (13 years ago)
Author:
nakasato
Comment:

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  • UGT2010

    v1 v2  
    1 = M.Murakami = 
     1= 村上真理 = 
    22== Simulations of Merging White Dwarf Stars by Smoothed Particle Hydrodynamics Method == 
    33I simulate merging white dwarf stars by smoothed par- ticle hydrodynamics. A purpose of my study is to ex- amine what will happen by merging white dwarf. I use Smoothed Particle Hydrodynamics method for the sim- ulation, and simulate 10 models in total. Similar simu- lation had been performed, but the treated particle num- ber was a little. I increase the number of the particles for simulation. In addition I calculate the gravitational wave. Therefore, the result are different by the mass ratio. 
     4 
     5[[Image(Murakami1.png)]]  
     6 
     7[[Image(Murakami2.png)]]  
     8 
     9[[Image(Murakami3.png)]]