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Title: On the Role of Dynamical Cooling in the Dynamics of Circumbinary Disks
Abstract

Hydrodynamical interactions between binaries and circumbinary disks (CBDs) play an important role in a variety of astrophysical systems, from young stellar binaries to supermassive black hole binaries. Previous simulations of CBDs have mostly employed locally isothermal equations of state. We carry out 2D viscous hydrodynamic simulations of CBDs around equal-mass, circular binaries, treating the gas thermodynamics by thermal relaxation toward equilibrium temperature (the constant-βcooling ansatz, whereβis the cooling time in units of the local Keplerian time). As an initial study, we use the grid-based codeAthena++on a polar grid, covering an extended disk outside the binary co-orbital region. We find that with a longer cooling time, the accretion variability is gradually suppressed, and the morphology of the CBD becomes more symmetric. The disk also shows evidence of hysteresis behavior depending on the initial conditions. Gas cooling also affects the rate of angular momentum transfer between the binary and the CBD, where given our adopted disk thickness and viscosity (H/r∼ 0.1 andα∼ 0.1), the binary orbit expands while undergoing accretion for mostβvalues between 0 and 4.0 except over a narrow range of intermediateβvalues. The validity of using a polar grid excising the central domain is also discussed.

 
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NSF-PAR ID:
10395882
Author(s) / Creator(s):
; ;
Publisher / Repository:
DOI PREFIX: 10.3847
Date Published:
Journal Name:
The Astrophysical Journal
Volume:
943
Issue:
2
ISSN:
0004-637X
Format(s):
Medium: X Size: Article No. 175
Size(s):
["Article No. 175"]
Sponsoring Org:
National Science Foundation
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