Changes between Initial Version and Version 1 of UGT2010


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Timestamp:
Feb 12, 2012 2:21:20 PM (13 years ago)
Author:
nakasato
Comment:

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  • UGT2010

    v1 v1  
     1= M.Murakami = 
     2== Simulations of Merging White Dwarf Stars by Smoothed Particle Hydrodynamics Method == 
     3I 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.