Critical behavior and ultraviolet scaling of induced gravitational waves (GWs) from an early matter-dominated (eMD) era are studied in the context of primordial black hole evaporation. The depth of the eMD is characterized by the minimum parameter of the equation of state ${\omega }_{\min }$ that the Universe can attain during this phase. We identify a critical value ${\omega }_c\sim 7.3\times {10}^{-3}$ that separates two regimes. For ${\omega }_{\min }<{\omega }_c$, the GW peak lies at the nonlinear cutoff point and requires nonlinear dynamics. For ${\omega }_{\min }>{\omega }_c$, the peak originates from modes that reenter near the matter-radiation equality, and the ultraviolet tail follows a distinct scaling $k^{-3/2}$. This critical behavior provides a clear definition of deep versus shallow eMD and a robust spectral signature for future GW observations.

Close

PrevNext

View figure in article

• Gravitational waves