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20242026
most citedNumerical simulation of type II primordial black hole formation

23 citations · 30 across the 14 of their papers we have counts for

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gr-qc2026

Refocusing of Wheeler--DeWitt wave functions at inner horizons

Takeshi Chiba, Keiju Murata, Daiki Saito

We study quantum gravitational effects inside hyperbolic black holes with both outer and inner horizons by solving the Wheeler--DeWitt (WDW) equation in the minisuperspace approxim…

gr-qc2026★ 1 cited

COSMOS: A numerical relativity code specialized for PBH formation

Chul-Moon Yoo, Hirotada Okawa, Albert Escrivà +7

Primordial black holes (PBHs) are black holes generated in the early universe without having gone through stellar evolution. In the standard formation process, PBHs are formed from…

gr-qc2026

Rotating wormholes in five dimensions with equal angular momenta: large asymmetry regime

Keiya Uemichi, Yasutaka Koga, Daiki Saito +2

We clarify the relationship between rotation and the energy condition for stationary rotating wormhole solutions of the Einstein equations coupled to a phantom field in five-dimens…

gr-qc2026

Dynamical Formation of Self-Similar Wormholes

Yasutaka Koga, Ryota Maeda, Daiki Saito +1

We study spherically symmetric, self-similar wormhole solutions supported by colliding streams of negative-energy null dust, and their dynamical formation. Under the assumption of…

gr-qc2025

Primordial Black Hole Formation and Spin in Matter Domination Revisited

Weitao Ye, Yungui Gong, Tomohiro Harada +4

In this article, we calculate the mass distribution of primordial black holes (PBHs) formed in the matter-dominated (MD) era by the peak theory. We apply the Zel'dovich approximati…

gr-qc2025★ 3 cited

Dynamical Formation of Charged Wormholes

Yasutaka Koga, Ryota Maeda, Daiki Saito +2

We construct static, spherically symmetric, charged traversable wormhole solutions to the Einstein--Maxwell equations, supported by bidirectional (ingoing and outgoing) null dust w…

gr-qc2025

Primordial black hole formation from a type II perturbation in the absence and presence of pressure

Koichiro Uehara, Albert Escrivà, Tomohiro Harada +2

We investigate primordial black holes (PBHs) formed from extremely large amplitudes of primordial curvature fluctuations, classified as type II. Type II fluctuations differ from ty…

gr-qc2024

Primordial Black Hole Formation from Type II Fluctuations with Primordial Non-Gaussianity

Masaaki Shimada, Albert Escrivá, Daiki Saito +2

This study investigates the formation of primordial black holes (PBHs) resulting from the collapse of adiabatic fluctuations with large amplitudes and non-Gaussianity. Ref. \cite{U…

gr-qc2024

Removing naked singularities in static axially symmetric spacetimes by patching with the flat spacetimes

Daiki Saito, Daisuke Yoshida

We investigate static, axially symmetric spacetimes without naked singularities that are constructed by patching Weyl class spacetimes with the flat spacetimes. Once the exterior g…

gr-qc2024

Revisiting spins of primordial black holes in a matter-dominated era based on peak theory

Daiki Saito, Tomohiro Harada, Yasutaka Koga +1

We estimate the probability distribution for the spins of the primordial black holes (PBHs) that formed during an early matter-dominated era in the Universe. We employ the Zel'dovi…

gr-qc2024★ 23 cited

Numerical simulation of type II primordial black hole formation

Koichiro Uehara, Albert Escrivà, Tomohiro Harada +2

This study investigates the formation of type II primordial black holes (PBHs) resulting from extremely large amplitudes of initial fluctuations in a radiation-dominated universe.…