The Merging of Black Hole Binary in Gas Sphere: Effects of the Equation of State

Details The Merging of Black Hole Binary in Gas Sphere: Effects of the Equation of State The Merging of Black Hole Binary in Gas Sphere: Effects of the Equation of State

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.9002l&link_type=abstract

American Astronomical Society Meeting 207, #90.02; Bulletin of the American Astronomical Society, Vol. 37, p.1318

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I will present high resolution SPH simulations of the merging of black hole binary in three polytropic gas spheres: adiabatic, γ =1.2, and isothermal. Our results show that the separation of the binary decreases quickly in an isothermal sphere, less fast when γ =1.2, and slowly in an adiabatic sphere, suggesting that the equation of state of the gas plays an important role in the merging process.

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