activity
20172021
most citedQuasi-periodic oscillations in flares and coronal mass ejections associated with magnetic reconnection

56 citations · 126 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc202125 cited

Axion clouds may survive the perturbative tidal interaction over the early inspiral phase of black hole binaries

Takuya Takahashi, Takahiro Tanaka

Gravitational wave observation has the potential of probing ultralight bosonic fields such as axion. Axion forms a cloud around a rotating black hole (BH) by superradiant instabili…

gr-qc20201 cited

Renormalization group analysis of superradiant growth of self-interacting axion cloud

Hidetoshi Omiya, Takuya Takahashi, Takahiro Tanaka

There are strong interests in considering ultra-light scalar fields (especially axion) around a rapidly rotating black hole because of the possibility of observing gravitational wa…

cond-mat.str-el201713 cited

Symmetry Preservation and Critical Fluctuations in a Pseudospin Crossover Perovskite LaCoO

Yasuhiro Shimizu, Takuya Takahashi, Syunpei Yamada +3

Spin-state crossover beyond a conventional ligand-field theory has been a fundamental issue in condensed matter physics. Here, we report microscopic observations of spin states and…

astro-ph.SR201756 cited

Quasi-periodic oscillations in flares and coronal mass ejections associated with magnetic reconnection

Takuya Takahashi, Jiong Qiu, Kazunari Shibata

We propose a mechanism for quasi-periodic oscillations of both coronal mass ejections (CMEs) and flare loops as related to magnetic reconnection in eruptive solar flares. We perfor…

astro-ph.SR201729 cited

Sheath-Accumulating Propagation of Interplanetary Coronal Mass Ejection

Takuya Takahashi, Kazunari Shibata

Fast interplanetary coronal mass ejections (interplanetary CMEs, or ICMEs) are the drivers of strongest space weather storms such as solar energetic particle events and geomagnetic…

astro-ph.SR20172 cited

Shock-Cloud Interaction in the Solar Corona

Takuya Takahashi

Flare associated coronal shock waves sometimes interact with solar prominences leading to large amplitude prominence oscillations. Such prominence activation gives us unique opport…