Even after including inflated young radii, overlooked inner planets, and non-zero initial offsets, eccentricity tides still cannot fully explain the observed period-ratio deviations of near-resonant exoplanets.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Non-zero Initial $\Delta$
Even after including inflated young radii, overlooked inner planets, and non-zero initial offsets, eccentricity tides still cannot fully explain the observed period-ratio deviations of near-resonant exoplanets.