Changes between Version 2 and Version 3 of UGT2010


Ignore:
Timestamp:
Feb 12, 2012 2:43:00 PM (13 years ago)
Author:
nakasato
Comment:

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  • UGT2010

    v2 v3  
    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. 
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    5 [[Image(Murakami1.png)]]  
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    7 [[Image(Murakami2.png)]]  
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    96[[Image(Murakami3.png)]]  
     7[[Image(Murakami1.png)]]  
     8[[Image(Murakami2.png)]]