◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

T. Usui

19 papers hereh-index 292.6k citations244 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author12
  • last author4

Across the 18 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP10
  • cond-mat.supr-con8
  • cond-mat.str-el1
same name
  • T. Usui — 7 papers, h 27
  • T. Usui — 3 papers, h 14
  • T. Usui — 2 papers, h 1
  • T. Usui — 2 papers, h 4
  • T. Usui — 1 paper, h 1
  • T. Usui — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20142026
most citedEvolution of Water Reservoirs on Mars: Constraints from Hydrogen Isotopes in Martian Meteorites

119 citations · 466 across the 19 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

cond-mat.supr-con2014★ 13 cited

Unscaling Superconducting Parameters with Tc​ for Bi-2212 and Bi-2223: A Magnetotransport Study in the Superconductive Fluctuation Regime

Shintaro Adachi, Tomohiro Usui, Hironobu Kudo +12

To investigate the origin of the enhanced Tc​ (≈ 110 K) of the trilayer cuprate superconductor Bi2​Sr2​Ca2​Cu3​O10+δ​ (Bi-2223), we have performed sys…

cond-mat.supr-con2014★ 15 cited

Doping Dependencies of Onset Temperatures for the Pseudogap and Superconductive Fluctuation in Bi2​Sr2​CaCu2​O8+δ​, Studied from both In-Plane and Out-of-Plane Magnetoresistance Measurements

Tomohiro Usui, Daiki Fujiwara, Shintaro Adachi +12

To investigate the relationship between the pseudogap and superconductivity, we measured both the in-plane (ρab​) and out-of-plane (ρc​) resistivity for oxygen-controlled Bi$…

astro-ph.EP2014★ 119 cited

Evolution of Water Reservoirs on Mars: Constraints from Hydrogen Isotopes in Martian Meteorites

Hiroyuki Kurokawa, Masahiko Sato, Masashi Ushioda +4

Martian surface morphology implies that Mars was once warm enough to maintain persistent liquid water on its surface. While the high D/H ratios (~6 times the Earth's ocean water) o…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.