[2508.15134] Disentangling the Origins of the NANOGrav Signal: Early Universe Models and $ΔN_{eff}$ Bounds Skip to main content We gratefully acknowledge support from the Simons Foundation, member institutions , and all contributors.
We demonstrate that models predicting $\Delta N_{eff}$ above the CMB limit would be firmly excluded, implying that the NANOGrav signal in tension with these bounds must instead arise from astrophysical sources.
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