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- W4385291878 abstract "Recently, pulsar timing array (PTA) collaborations announced evidence for an isotropic stochastic gravitational wave (GW) background. The origin of the PTA signal can be astrophysical or cosmological. In the latter case, the so-called secondary scalar-induced GW scenario is one of the viable explanations, but it has a potentially serious issue of the overproduction of primordial black holes (PBHs) due to the enhanced curvature perturbation. In this letter, we present a new interpretation of the PTA signal. Namely, it is originated from an extra spectator tensor field that exists on top of the metric tensor perturbation. As the energy density of the extra tensor field is always subdominant, it cannot lead to the formation of PBHs. Thus our primordial-tensor-induced scenario is free from the PBH overproduction issue." @default.
- W4385291878 created "2023-07-27" @default.
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- W4385291878 date "2023-07-24" @default.
- W4385291878 modified "2023-10-06" @default.
- W4385291878 title "Extra-tensor-induced origin for the PTA signal: No primordial black hole production" @default.
- W4385291878 doi "https://doi.org/10.48550/arxiv.2307.13109" @default.
- W4385291878 hasPublicationYear "2023" @default.
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