Understand
The possibility that long tidal tails formed during compact object mergers may power optical transients through the decay of freshly synthesized r-process material is investigated.
- Precise modeling of the merger dynamics allows for a realistic determination of the thermodynamic conditions in the ejected debris.
- The results of hydrodynamic and full nuclear network calculations are combined to calculate the resultant r-process abundances and the heating of the material by their decays.
- The subsequent homologous structure is mapped into a radiative transfer code to synthesize emergent model light curves and determine how their properties (variability and color evolution) depend on the mass ratio and orientation of the merging binary.
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Zemp, M., Ramirez-Ruiz, E., & Diemand, J. 2009, ApJ, 705, L186
2009
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