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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 8.

The distribution of likelihoods for the best-fit parameters derived from 100 synthetic datasets constructed in the p-value procedure (blue histogram) compared to the likelihood of the actual data’s best-fit parameters (red vertical line), for the single power-law mass–radius relation (left) and the modified mass–radius relation (right). The likelihood of the observed data is better than the likelihood obtained in 15% of the synthetic datasets for the single power-law model and is better than obtained in 67% of the synthetic datasets for the modified mass–radius relation.

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