activity
19992023
most citedPhysics Interplay of the LHC and the ILC

408 citations · 5.6k across the 109 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

hep-ph2022★ 12 cited

Probing New Physics in the Vector-like Lepton Model by Lepton Electric Dipole Moments

Koichi Hamaguchi, Natsumi Nagata, Genta Osaki +1

We examine the lepton dipole moments in an extension of the Standard Model (SM), which contains vector-like leptons that couple only to the second-generation SM leptons. The model…

hep-ph2022

Report of the Topical Group on Physics Beyond the Standard Model at Energy Frontier for Snowmass 2021

Tulika Bose, Antonio Boveia, Caterina Doglioni +318

This is the Snowmass2021 Energy Frontier (EF) Beyond the Standard Model (BSM) report. It combines the EF topical group reports of EF08 (Model-specific explorations), EF09 (More gen…

hep-ph2022★ 3 cited

Minimal Nambu-Goldstone Higgs Model in Supersymmetric SU(5) Revisited

Koichi Hamaguchi, Shihwen Hor, Natsumi Nagata

We revisit the minimal Nambu-Goldstone (NG) Higgs supersymmetric (SUSY) SU(5) grand unified model and study its phenomenological implications. The Higgs sector of the model possess…

hep-th2022★ 7 cited

Axion Quality Problem and Non-Minimal Gravitational Coupling in the Palatini Formulation

Dhong Yeon Cheong, Koichi Hamaguchi, Yoshiki Kanazawa +3

In axion models, the global U(1) Peccei-Quinn (PQ) symmetry is explicitly broken by non-perturbative effects of gravity, such as axionic wormholes. The gravitational violation of t…

hep-ph2022★ 2 cited

Neutron Star Heating in Dark Matter Models for the Muon Discrepancy

Koichi Hamaguchi, Natsumi Nagata, Maura E. Ramirez-Quezada

The observed value of the muon magnetic dipole moment, which deviates from the Standard Model prediction by , can be explained in models with weakly-interacting massive parti…

hep-ph2022★ 30 cited

Capture of Electroweak Multiplet Dark Matter in Neutron Stars

Motoko Fujiwara, Koichi Hamaguchi, Natsumi Nagata +1

If dark matter has a sizable scattering cross section with nucleons, it can efficiently be captured by a neutron star. Its energy is then transferred to the neutron star as heat th…