activity
20162020
most citedSelf-interacting dark matter and muon in a gauged U model

111 citations · 472 across the 11 of their papers we have counts for

collaborators

11 papers

hep-ph2020★ 2 cited

Thermal Evolution of Neutron Stars as a Probe of Physics beyond the Standard Model

Keisuke Yanagi

Thermal evolution of neutron stars (NSs) is studied as a probe of physics beyond the standard model. We first review the standard cooling theory of NSs in detail, with an emphasis…

hep-ph2019★ 36 cited

Constraining FIMP from the structure formation of the Universe: analytic mapping from

Ayuki Kamada, Keisuke Yanagi

A feebly interacting massive particle (FIMP), contrasting with a weakly interacting massive particle (WIMP), is an intriguing dark matter (DM) candidate. Light (keV-scale) FIMP DM…

astro-ph.CO2019★ 4 cited

Fingerprint matching of beyond-WIMP dark matter: neural network approach

Kyu Jung Bae, Ryusuke Jinno, Ayuki Kamada +1

Galactic-scale structure is of particular interest since it provides important clues to dark matter properties and its observation is improving. Weakly interacting massive particle…

hep-ph2019★ 70 cited

Dark Matter Heating vs. Rotochemical Heating in Old Neutron Stars

Koichi Hamaguchi, Natsumi Nagata, Keisuke Yanagi

Dark matter (DM) particles in the Universe accumulate in neutron stars (NSs) through their interactions with ordinary matter. It has been known that their annihilation inside the N…

astro-ph.HE2019★ 31 cited

Cooling Theory Faced with Old Warm Neutron Stars: Role of Non-Equilibrium Processes with Proton and Neutron Gaps

Keisuke Yanagi, Natsumi Nagata, Koichi Hamaguchi

Recent observations have found several candidates for old warm neutron stars whose surface temperatures are above the prediction of the standard neutron star cooling scenario, and…

hep-ph2018★ 110 cited

Limit on the Axion Decay Constant from the Cooling Neutron Star in Cassiopeia A

Koichi Hamaguchi, Natsumi Nagata, Keisuke Yanagi +1

The observed rapid cooling of the neutron star (NS) located at the center of the supernova remnant Cassiopeia A (Cas A) can be explained in the minimal NS cooling scenario. This co…