DEUTERIUM BURNING IN MASSIVE GIANT PLANETS AND LOW-MASS BROWN DWARFS FORMED BY CORE-NUCLEATED ACCRETION

@article{Bodenheimer2013DEUTERIUMBI,
  title={DEUTERIUM BURNING IN MASSIVE GIANT PLANETS AND LOW-MASS BROWN DWARFS FORMED BY CORE-NUCLEATED ACCRETION},
  author={Peter H. Bodenheimer and Gennaro D’Angelo and Jack J. Lissauer and Jonathan J. Fortney and Didier Saumon},
  journal={The Astrophysical Journal},
  year={2013},
  volume={770}
}
Using detailed numerical simulations, we study the formation of bodies near the deuterium-burning limit according to the core-nucleated giant planet accretion scenario. The objects, with heavy-element cores in the range 5–30 M⊕, are assumed to accrete gas up to final masses of 10–15 Jupiter masses (MJup). After the formation process, which lasts 1–5 Myr and which ends with a “cold-start,” low-entropy configuration, the bodies evolve at constant mass up to an age of several Gyr. Deuterium… 
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