Prelude to a double degenerate merger: the onset of mass transfer and its impact on gravitational waves and surface detonations
arXiv:1101.5132 · doi:10.1088/0004-637X/737/2/89
Abstract
We present the results of a systematic numerical study of the onset of mass transfer in double degenerate binary systems and its impact on the subsequent evolution. All investigated systems belong to the regime of direct impact, unstable mass transfer. In all of the investigated cases, even those considered unstable by conventional stability analysis, we find a long-lived mass transfer phase continuing for as many as several dozen orbital periods. This settles a recent debate sparked by a discrepancy between earlier SPH calculations that showed disruptions after a few orbital periods and newer grid-based studies in which mass transfer continued for tens of orbits. As we show that these binaries can survive at small separation for hundreds of orbital periods, their associated gravitational wave signal should be included when calculating the gravitational wave foreground (although expected to below LISA's sensitivity at these high frequencies). We also show that the inclusion of the entropy increase associated with shock-heating of the accreted material reduces the number of orbits a binary survives given the same initial conditions, although the effect is not as pronounced when using the appropriate initial conditions. The use of accurate initial conditions and a correct treatment of shock heating allows for a reliable time evolution of the temperature, density, and angular momentum, which are important when considering thermonuclear events that may occur during the mass transfer phase and/or after merger. Our treatment allows us to accurately identify when surface detonations may occur in the lead-up to the merger, as well as the properties of final merger products.
20 pages, 25 figures, submitted to ApJ. Movies available at http://teamwork.jacobs-university.de:8080/confluence/display/~mdan/Prelude+to+a+double+degenerate+merger
References in corpus (10)
- The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star
- Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?
- The Luminous and Carbon-Rich Supernova 2006gz: A Double Degenerate Merger?
- Double-detonation supernovae of sub-Chandrasekhar mass white dwarfs
- Fallback accretion in the aftermath of a compact binary merger
- Astrophysical Smooth Particle Hydrodynamics
- The ELM Survey. II. Twelve Binary White Dwarf Merger Systems
- The Stability of Double White Dwarf Binaries Undergoing Direct Impact Accretion
- Simulating Black Hole White Dwarf Encounters
- The galactic population of white dwarfs
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