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Multimodality in the Search for New Physics in Pulsar Timing Data and the Case of Kination-amplified Gravitational-wave Background from Inflation

  • Authors: Bohua Li, Joel Meyers, Paul R. Shapiro

Bohua Li et al 2025 The Astrophysical Journal 985 .

  • Provider: AAS Journals

Caption: Figure 4.

3D scatterplot with the NGmock sample (left panels) and the EPTAmock sample (right panels). The color bar indicates the value of ΔNeff,GW for each point. The stars and the triangles in the lower panels denote the KA and the no-KA best fits to the mock spectra, respectively. The dashed lines in the upper panels also denote these best fits (same as in the lower figure of Figure 2), specified in Table 1. The dashed lines in the lower panels indicate the various physical constraints on the KA and the no-KA modes, described by Equations (5), (6), and (7).

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