Review examines gravitational-wave generation in a unified dark sector model, suggesting detectable outcomes.
In this work, we review gravitational-wave generation in a two-scalar-field cosmological model. The framework relies on a two-field scenario in which warm inflation is unified with the dark sector within a single theoretical description. It has recently been shown that this setup leads to a gravitational-wave spectrum potentially detectable by future experiments. Here we also demonstrate that the resulting spectrum is largely independent of the 𝜙 field initial condition, thereby extending previous findings.
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Tommaso Mengoni (2026) studied this question.
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