activity
20242026
collaborators

10 papers

astro-ph.CO2026

Gravitational Waves from Primordial Black Holes: Connecting Low-Frequency Scalar-Induced Signatures to High-Frequency Binary Mergers

Ashu Kushwaha

Formation of primordial black holes (PBHs) requires a significant enhancement of curvature perturbations. This enhancement generates a twofold gravitational wave (GW) signature: a…

astro-ph.CO2026

Secondary Production of Photons from ALP Dark Matter interacting with a Cosmological Magnetic Field

Abdias Aires, Robert Brandenberger, Ashu Kushwaha

Under the assumption that dark matter is a coherently oscillating pseudoscalar field coupled to electromagnetism by the usual Chern-Simons term, we study the production of secondar…

astro-ph.CO2026

Probing Axion-Photon conversion via circular polarization imprints in the CMB -mode observations

Ashu Kushwaha, Rajeev Kumar Jain

In the presence of a background magnetic field, axions or axion-like particles (ALPs) can be resonantly converted to photons when their mass is nearly equal to the effective photon…

astro-ph.CO2026

Revisiting Constraints on Primordial Curvature Power Spectrum from PBH Abundances

Ashu Kushwaha, Teruaki Suyama

Primordial black holes (PBHs) can form in the early Universe, for instance during radiation domination, from the collapse of large-amplitude density perturbations shortly after hor…

hep-ph2026

An upper limit on cosmological chiral gravitational wave background

Mohammad Ali Gorji, Ashu Kushwaha, Teruaki Suyama

Within the standard framework in which electroweak sphaleron processes relate lepton and baryon number, we derive an upper limit on the amplitude of a chiral gravitational wave bac…

astro-ph.CO2026

Excursion Set Approach to Primordial Black Holes: Cloud-in-Cloud and Mass Function Revisited

Ashu Kushwaha, Teruaki Suyama

The abundance and mass function of primordial black holes (PBHs) are often estimated using the Press-Schechter (PS) formalism. In the case of halo formation, the PS formalism suffe…