activity
20242026
most citedThermalization and hotspot formation around small primordial black holes

7 citations · 10 across the 17 of their papers we have counts for

collaborators

18 papers

gr-qc2026

Simulation of PBH formation in a matter-dominated universe

Chul-Moon Yoo, Albert Escrivà, Tomohiro Harada +1

We investigate primordial black hole (PBH) formation during an early matter-dominated era using fully nonlinear numerical relativity. The initial condition is set by a functional f…

astro-ph.CO2026

Higher-Order Analytical Expansion of Thawing Dark Energy with an Exponential Potential

Naoto Maki, Kazunori Kohri

Motivated by recent DESI results suggesting dynamical dark energy, we investigate the thawing scenario in quintessence with an exponential potential, …

astro-ph.CO2026

X-ray signals converted from high-frequency gravitational waves emitted by spinning light primordial black hole dark matter

Asuka Ito, Kazunori Kohri

We investigate the detectability of high-frequency gravitational waves from the superradiance of light primordial black hole dark matter through photons converted in the Galactic m…

astro-ph.CO2026

A cross-calibration approach for polarisation-sensitive detectors in CMB experiments: application to LiteBIRD's polarisation angle calibration

A. Novelli, F. Piacentini, S. Micheli +102

We present a cross-calibration algorithm that determines the relative calibration of detectors within the same frequency band of a CMB experiment. The method iteratively compares s…

gr-qc2026

Graviton Floor

Himeka Matsuo, Asuka Ito, Kazunori Kohri +2

It has been observed that the Universe is permeated by the cosmic photon background, ranging from radio waves to gamma rays. We investigate the conversion of the photon background…

gr-qc2026

Natural Inflation with a negative cosmological constant

Chia-Min Lin, Naoto Maki, Kazunori Kohri

In this work, we investigate a cosmic inflation model based on a cosine-type potential with a negative cosmological constant. This model originates from a classical solution of the…

astro-ph.CO2026

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations

Albert Escrivà, Tomohiro Harada, Kazunori Kohri +2

We study the dynamics of the collapse of a nonspherical overdense patch during an early matter-dominated era and the associated production of gravitational waves (GWs) using a semi…

astro-ph.CO2026

Blue-tilted spectral running and the JWST early galaxy tension

Mikage U. Kobayashi, Gen Chiaki, Kazutaka Kimura +4

Recently, the James Webb Space Telescope (JWST) collaboration has found the unexpectedly large abundance of massive galaxies with stellar masses of at high…

astro-ph.CO2026

Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter

Naoto Maki, Kazunori Kohri

Motivated by the indications of time-varying dark energy equation of state reported from DESI, we investigate a quintessence model with an exponential potential $V_0 e^{-λϕ/m_{\mat…

hep-th2026

Simple Analytical Solutions of the Wheeler-DeWitt Equation in the Classical Hamilton-Jacobi Limit

Naoto Maki, Chia-Min Lin, Kazunori Kohri

We investigate the Wheeler-DeWitt equation for a flat, homogeneous, and isotropic Universe containing a canonical scalar field with a potential. We show that under the constraint $…

hep-ph2026

CMB signatures of gravity-mediated dark radiation in

Anish Ghoshal, Sk Jeesun, Kazunori Kohri

Measurement of in the CMB (Cosmic Microwave Background) observations, like Planck 2018 and BBN (Big Bang Nucleosynthesis) has already set stringent constraints on the…

astro-ph.CO2026

Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy

Naoto Maki, Kazunori Kohri

In this paper, we investigate a quintessence field with an exponential potential motivated by the suggestion of time-varying dark energy from the DESI galaxy survey. Assuming a kin…

astro-ph.CO2025

NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes, and implications for the origins of Little Red Dots

Mikage U. Kobayashi, Kazunori Kohri

In this paper, we explain the recently reported a nHz-band gravitational-wave background from NANOGrav 15-year through the merger of binary super-massive black holes with masses 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…

astro-ph.CO2025★ 1 cited

Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order

Jun-Peng Li, Sai Wang, Zhi-Chao Zhao +1

Produced nonlinearly by the enhanced linear cosmological curvature perturbations, the scalar-induced gravitational waves (SIGWs) can serve as a potentially powerful probe of primor…

hep-ph2025

General relativistic effects on photon spectrum emitted from dark matter halos around primordial black holes

Toya Suzuki, Takahisa Igata, Kazunori Kohri +1

We investigate general relativistic effects on the photon spectrum emitted from decaying (or annihilating) particle dark matter in the halo surrounding a primordial black hole. The…

astro-ph.CO2024★ 2 cited

Study of primordial non-Gaussianity and with the cross-correlations between the scalar-induced gravitational waves and the cosmic microwave background

Zhi-Chao Zhao, Sai Wang, Jun-Peng Li +1

The stochastic gravitational-wave background originating from cosmic sources contains vital information about the early universe. In this work, we comprehensively study the cross-c…

hep-ph2024★ 7 cited

Thermalization and hotspot formation around small primordial black holes

Minxi He, Kazunori Kohri, Kyohei Mukaida +1

We quantitatively analyze a basic question: what is the stationary solution of the background plasma temperature profile around a black hole (BH)? One may naively expect that the t…