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.
040 Re(rΨl=m=3 4 /µ ) uµ (retarded time) 0 1.5 3 4.5 0 400 800 1200 1600 2000 2400 2800 Proca mass Proca angular momentum Mass tµ Figure 19
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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.