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2023

Constraints on neutrino natal kicks from black-hole binary VFTS 243

Vigna-Gómez, Alejandro, Willcox, Reinhold, Tamborra, Irene et al.

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The recently reported observation of VFTS 243 is the first example of a massive black-hole binary system with negligible binary interaction following black-hole formation.

The black-hole mass ($\approx 10\ M_{\odot}$) and near-circular orbit ($e\approx 0.02$) of VFTS 243 suggest that the progenitor star experienced complete collapse, with energy-momentum being lost predominantly through neutrinos.
VFTS 243 enables us to constrain the natal kick and neutrino-emission asymmetry during black-hole formation.
At 68% C.L., the natal kick velocity (mass decrement) is $\lesssim 10$ km/s ($\lesssim 1.0\ M_{\odot}$), with a full probability distribution that peaks when $\approx 0.3\ M_{\odot}$ were ejected, presumably in neutrinos, and the black hole experienced a natal kick of $4$ km/s.

Constraints on neutrino natal kicks from black-hole binary VFTS 243 · Around

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