Under the assumption that occurrence rates reflect gas accretion efficiency, the paper inverts Kepler transit data to infer inner disk gas surface density and magnetic field profiles that switch character at the hot-Jupiter period valley.
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Close-in giant-planet formation via in-situ gas accretion and their natal disk properties
Under the assumption that occurrence rates reflect gas accretion efficiency, the paper inverts Kepler transit data to infer inner disk gas surface density and magnetic field profiles that switch character at the hot-Jupiter period valley.