most citedPhenomenology of bubble size distributions in a first-order phase transition

1 citations · 1 across the 3 of their papers we have counts for

collaborators

6 papers

hep-ph20261 cited

Phenomenology of bubble size distributions in a first-order phase transition

Danny Marfatia, Po-Yan Tseng, Yu-Min Yeh

In a cosmological first-order phase transition (FOPT), the true and false vacuum bubble radius distributions are not expected to be monochromatic, as is usually assumed. Consequent…

astro-ph.HE2026

Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts

Chang-Yu Dai, Po-Yan Tseng

Femtolensing of gamma-ray bursts (GRBs) is vastly studied to constrain primordial black holes lighter than solar mass and may close the window for PBH dark matter. In th…

hep-ph2026

Constraining memory-burdened primordial black holes with graviton-photon conversion and binary mergers

Po-Yan Tseng, Yu-Min Yeh

The memory-burden effect stabilizes the evaporating Primordial Black Holes (PBHs) before its complete decay. This also suppresses the evaporation flux via the entropy factor to the…

hep-ph2026

Angular momentum of vacuum bubbles in a first-order phase transition

Jan Tristram Acuña, Danny Marfatia, Po-Yan Tseng

The formation of primordial black holes (PBHs) during a first-order phase transition (FOPT) in a dark sector has been of recent interest. A quantity that characterizes a black hole…

hep-ph2025

Phenomenology of Neutrino-Dark Matter Interaction in DSNB and AGN

Po-Yan Tseng, Yu-Min Yeh

We investigate a neutrino-scalar dark matter (DM) interaction encountering distinctive neutrino sources, namely Diffuse Supernova Neutrino Background (DSNB) and Active Galac…

hep-ph2025

Constraints on extended axion structures from the lensing of fast radio bursts

Jan Tristram Acuña, Kuan-Yen Chou, Po-Yan Tseng

Axions are hypothetical pseudoscalar particles that have been regarded as promising dark matter (DM) candidates. On the other hand, extended compact objects such as axion stars, wh…