Changes between Version 3 and Version 4 of UGT2010


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Timestamp:
Feb 12, 2012 3:00:18 PM (13 years ago)
Author:
nakasato
Comment:

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  • UGT2010

    v3 v4  
    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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     5file:///home/committee/aac/Thesis2010/s1150220 
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    67[[Image(Murakami3.png)]]