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Angle-dependent in Situ Fast Flavor Transformations in Post-neutron-star-merger Disks

  • Authors: Kelsey A. Lund, Payel Mukhopadhyay, Jonah M. Miller, G. C. McLaughlin

Kelsey A. Lund et al 2025 The Astrophysical Journal Letters 985 .

  • Provider: AAS Journals

Caption: Figure 5.

Top: total mass of each element produced, as a function of mass number. Bottom: mass-weighted relative abundances of each element produced, with solar abundances shown as gray diamonds. In each case, we plot both the yields from the outflows with (pink) and without (teal) oscillations. We show the results considering all ejecta (solid lines) as well as nonequatorial ejecta (dashed), as described in Section 3.

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