activity
20162023
most citedThe Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest

66 citations · 374 across the 16 of their papers we have counts for

collaborators

16 papers

hep-ph2023★ 9 cited

Multipole vector dark matter below the GeV-scale

Xiaoyong Chu, Junji Hisano, Alejandro Ibarra +2

We consider electrically neutral complex vector particles below the GeV mass scale that, from a low energy perspective, couple to the photon via higher dimensional form factor…

astro-ph.CO2022★ 3 cited

Early or phantom dark energy, self-interacting, extra, or massive neutrinos, primordial magnetic fields, or a curved universe: An exploration of possible solutions to the and problems

Helena García Escudero, Jui-Lin Kuo, Ryan E. Keeley +1

In this paper we explore the existing tensions in the local cosmological expansion rate, , and amplitude of the clustering of large-scale structure at …

hep-ph2022★ 13 cited

Atmospheric axion-like particles at Super-Kamiokande

Kingman Cheung, Jui-Lin Kuo, Po-Yan Tseng +1

We consider a muonphilic axion-like-particle (ALP), denoted as , lighter than twice the muon mass. ALPs of this mass range dominantly decay into a pair of photons, induced by a…

hep-ph2022★ 2 cited

Shining Light on Cosmogenic Axions with Neutrino Experiments

Yanou Cui, Jui-Lin Kuo, Josef Pradler +1

While most searches for cosmic axions so far focused on their cold relics as (a component of) dark matter, various well-motivated cosmological sources can produce "boosted" axions…

hep-ph2022★ 30 cited

FLArE up dark sectors with EM form factors at the LHC Forward Physics Facility

Felix Kling, Jui-Lin Kuo, Sebastian Trojanowski +1

Despite being mostly secluded, dark sector particles may feebly interact with photons via a small mass-dimension 4 millicharge, a mass-dimension 5 magnetic and electric dipole mome…

hep-ph2022★ 22 cited

Towards a full description of MeV dark matter decoupling: a self-consistent determination of relic abundance and

Xiaoyong Chu, Jui-Lin Kuo, Josef Pradler

Thermal dark matter at the MeV mass-scale has its abundance set during the highly non-trivial epochs of neutrino decoupling and electron annihilation. The technical obstacles attac…