Numerical simulations of eccentric Proca-star mergers show that relative phase between the stars controls post-merger fate and can generate odd-mode gravitational waves absent from black-hole mergers.
Evolution of rΨ22 4 for models 83B0 (in-phase on top panel) and 83B6 (in-phase on bottom panel), both with ω/µ = 0.83
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Eccentric mergers of binary Proca stars
Numerical simulations of eccentric Proca-star mergers show that relative phase between the stars controls post-merger fate and can generate odd-mode gravitational waves absent from black-hole mergers.