start-ver=1.4 cd-journal=joma no-vol=94 cd-vols= no-issue=11 article-no= start-page=113801 end-page= dt-received= dt-revised= dt-accepted= dt-pub-year=2025 dt-pub=20251115 dt-online= en-article= kn-article= en-subject= kn-subject= en-title= kn-title=Magnetically Enhanced Thermoelectric Effect Driven by Martensitic Transformation in the Weak Itinerant Ferromagnet Co2NbSn en-subtitle= kn-subtitle= en-abstract= kn-abstract=We investigated the magnetic and thermoelectric properties of the full Heusler alloy Co2NbSn, which exhibits a martensitic transformation at 240 K. Magnetization measurements reveal weak itinerant ferromagnetism in the martensitic phase, which is well described by Takahashi’s spin fluctuation theory. The characteristic spin fluctuation parameters were estimated to be T0 = 1.0 × 103 K and TA = 7.2 × 103 K. Seebeck coefficient measurements under magnetic fields up to 9 T show complex temperature and field dependence, which we decomposed into electron diffusion, spin fluctuation drag, and magnon drag components. A significant magnon-drag contribution was identified in both austenite and martensitic phases. Remarkably, this contribution is strongly enhanced in the martensitic phase compared to the austenite phase, despite a smaller magnetic moment. These findings provide evidence for robust low-energy spin excitations and highlight the potential of martensitic transformation in enhancing the thermoelectric performance of itinerant ferromagnetic alloys. en-copyright= kn-copyright= en-aut-name=KiharaTakumi en-aut-sei=Kihara en-aut-mei=Takumi kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=1 ORCID= en-aut-name=XuXiao en-aut-sei=Xu en-aut-mei=Xiao kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=2 ORCID= en-aut-name=OgiYuki en-aut-sei=Ogi en-aut-mei=Yuki kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=3 ORCID= en-aut-name=AdachiYoshiya en-aut-sei=Adachi en-aut-mei=Yoshiya kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=4 ORCID= en-aut-name=RoyTufan en-aut-sei=Roy en-aut-mei=Tufan kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=5 ORCID= en-aut-name=MatsuuraRyuji en-aut-sei=Matsuura en-aut-mei=Ryuji kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=6 ORCID= en-aut-name=KanomataTakeshi en-aut-sei=Kanomata en-aut-mei=Takeshi kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=7 ORCID= affil-num=1 en-affil=Research Institute for Interdisciplinary Science, Okayama University kn-affil= affil-num=2 en-affil=Department of Materials Science, Tohoku University kn-affil= affil-num=3 en-affil=Graduate School of Science and Engineering, Yamagata University kn-affil= affil-num=4 en-affil=Graduate School of Science and Engineering, Yamagata University kn-affil= affil-num=5 en-affil=Center for Science and Innovation in Spintronics (CSIS), Core Research Cluster (CRC), Tohoku University kn-affil= affil-num=6 en-affil=Faculty of Engineering, Tohoku Gakuin University kn-affil= affil-num=7 en-affil=Research Institute for Engineering and Technology, Tohoku Gakuin University kn-affil= END start-ver=1.4 cd-journal=joma no-vol=89 cd-vols= no-issue=1 article-no= start-page=012001 end-page= dt-received= dt-revised= dt-accepted= dt-pub-year=2019 dt-pub=20191212 dt-online= en-article= kn-article= en-subject= kn-subject= en-title= kn-title=Sparse Modeling in Quantum Many-Body Problems en-subtitle= kn-subtitle= en-abstract= kn-abstract=This review paper describes the basic concept and technical details of sparse modeling and its applications to quantum many-body problems. Sparse modeling refers to methodologies for finding a small number of relevant parameters that well explain a given dataset. This concept reminds us physics, where the goal is to find a small number of physical laws that are hidden behind complicated phenomena. Sparse modeling extends the target of physics from natural phenomena to data, and may be interpreted as “physics for data”. The first half of this review introduces sparse modeling for physicists. It is assumed that readers have physics background but no expertise in data science. The second half reviews applications. Matsubara Green’s function, which plays a central role in descriptions of correlated systems, has been found to be sparse, meaning that it contains little information. This leads to (i) a new method for solving the ill-conditioned inverse problem for analytical continuation, and (ii) a highly compact representation of Matsubara Green’s function, which enables efficient calculations for quantum many-body systems. en-copyright= kn-copyright= en-aut-name=OtsukiJunya en-aut-sei=Otsuki en-aut-mei=Junya kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=1 ORCID= en-aut-name=OhzekiMasayuki en-aut-sei=Ohzeki en-aut-mei=Masayuki kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=2 ORCID= en-aut-name=ShinaokaHiroshi en-aut-sei=Shinaoka en-aut-mei=Hiroshi kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=3 ORCID= en-aut-name=YoshimiKazuyoshi en-aut-sei=Yoshimi en-aut-mei=Kazuyoshi kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=4 ORCID= affil-num=1 en-affil=Research Institute for Interdisciplinary Science, Okayama University kn-affil= affil-num=2 en-affil=Graduate School of Information Sciences, Tohoku University kn-affil= affil-num=3 en-affil=Department of Physics, Saitama University kn-affil= affil-num=4 en-affil=4Institute for Solid State Physics, University of Tokyo kn-affil= END start-ver=1.4 cd-journal=joma no-vol=89 cd-vols= no-issue=6 article-no= start-page=064401 end-page= dt-received= dt-revised= dt-accepted= dt-pub-year=2020 dt-pub=20200519 dt-online= en-article= kn-article= en-subject= kn-subject= en-title= kn-title=Energy Transfer to Resonant Zonal Rossby Modes in Two-Dimensional Turbulence on a Rotating Sphere en-subtitle= kn-subtitle= en-abstract= kn-abstract=The transfer of energy by the nonlinear interaction of Rossby waves in two-dimensional turbulence on a rotating sphere was investigated in this study. Although it has been suggested that three-wave resonant interaction dominates nonlinear interactions when the rotation rate of the sphere is sufficiently high, resonant interactions do not transfer energy to zonal Rossby waves, resulting in the nonresonant interaction of Rossby waves being responsible for the generation of zonal flows [Reznik, Piterbarg, and Kartashova, Dyn. Atmos. Oceans 18, 235 (1993); Obuse and Yamada, Phys. Rev. Fluids 4, 024601 (2019)]. The resonant and nonresonant interactions of Rossby waves were investigated in this study, and it was found that although energy is transferred to the zonal Rossby modes by the nonresonant three-wave interaction of Rossby waves, the target of this nonresonant energy transfer is only the resonant zonal Rossby waves. en-copyright= kn-copyright= en-aut-name=ObuseKiori en-aut-sei=Obuse en-aut-mei=Kiori kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=1 ORCID= en-aut-name=YamadaMichio en-aut-sei=Yamada en-aut-mei=Michio kn-aut-name= kn-aut-sei= kn-aut-mei= aut-affil-num=2 ORCID= affil-num=1 en-affil=Graduate School of Environmental and Life Science, Okayama University kn-affil= affil-num=2 en-affil=Research Institute for Mathematical Sciences, Kyoto University kn-affil= END