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The TDE Population from First-principles Models of Stellar Disruption and Debris Dynamics

  • Authors: Tsvi Piran, Julian Krolik, Taeho Ryu

Tsvi Piran et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

The total (full + partial) event rate density in the ﹩\mathrm{log}{M}_{{\rm{BH}}}\times \mathrm{log}{L}_{{\rm{peak}}}﹩ plane for flux-limited samples. Both plots have αBH = 0, but the one in the left panel utilizes a Salpeter IMF mass function, cut off at 1 M, i.e., α1 = 2.35, α2 = 4, and Mb = 1 M, whereas the one in the right panel has no cutoff: α1 = α2 = 2.35. Rates (arbitrary units) are shown on a linear scale calibrated by the color bar.

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