Creep tide model for the three-body problem - The rotational evolution of a circumbinary planet

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Table 1

Initial conditions of our reference numerical simulation, representing a Kepler-38-like system (Orosz et al. 2012a).

Body	m₀	m₁	m₂
Mass	0.95 m_⊙	0.25 m_⊙(*)	10 m_⊕
Radius
a_i [AU]		0.15	0.45(*)
e_i		0.15	0.05(*)
Ω_i	5 n₁	5 n₁	5 n₂

Notes. Orbital elements are given in a Jacobi reference frame. The parameters highlighted with an asterisk were varied in different simulations as is indicated in the text.

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