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Modern Tidal Interaction Models for Rapid Binary Population Synthesis. I. Methods

Authors: Veome Kapil, Ilya Mandel, Evgeni Grishin, Jim Fuller, Jeff Riley, Emanuele Berti

Veome Kapil et al 2026 The Astrophysical Journal 1002 .

Provider: AAS Journals

Caption: Figure 9.

Stellar and tidal evolution for a 3 M_⊙ + 3 M_⊙ binary with P_orb,ZAMS= 5000 days and e_ZAMS = 0.5. The binary is simulated until WD + WD binary formation at ∼458 Myr. The dashed black lines show the boundaries between various stellar phases, and the phases are labeled above each plot.

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