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Constrained Gaussian-process-bridge Prior for Neutron-star Equation-of-state Inference

  • Authors: Tyler Gorda, Oleg Komoltsev, Aleksi Kurkela, Eirik Sunde

Tyler Gorda et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 7.

Posterior of dc(n), Δ(n), and p/pfree(μ) (see main text for definitions) from the hierarchical model discussed in Section 4 with the correlation length taken from a uniform distribution σ/n ∈ [0.2, 0.4].  The dotted vertical lines and the associated bars correspond to the mean and 1σ credible interval for densities reached in the centers of 1.4 M, 2 M, and MTOV stars.

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