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Kautsar et al. Energy Mater. 2025, 5, 500129  https://dx.doi.org/10.20517/energymater.2025.26  Page 7 of 14

               Figure 4A summarizes the σ  of the studied magnets, showing a slight increase after HD and subsequent
                                       xx
               GBDP. No notable differences in σ  were observed among the RE-Cu (RE = Dy-Nd, Nd, Pr) GBDP
                                               xx
               magnets. Figure 4B presents the κ and the lattice contribution to thermal conductivity (κ ) of the studied
                                                                                            lat
               magnets. The κ  is extracted by subtracting the electronic contribution (κ ) from the total κ : = κ - κ . The κ e
                                                                             e
                            lat
                                                                                                   e
                                                                                            lat
               is estimated using the Wiedemann-Franz Law  κ  = Lσ T, where L represents the Lorenz number
                                                            e
                                                                  xx
               (2.44 × 10  WΩK ) and T is the absolute temperature . Figure 4B shows that the  κ  exhibits a slight
                       -8
                              -2
                                                               [30]
                                                                                         lat
               increase after HD but rises significantly following GBDP. This contributes to the increase in κ in the HD
               and GBDP magnets compared to the HP magnet. The κ  values of the studied magnets are presented in
                                                                e
               Supplementary Figure 3; κ  shows only a slight increase after HD and GBDP.
                                     e
               The observed increase in σ  and κ following HD and GBDP can be attributed to the grain growth [53,54] .
                                       xx
               However, the substantial rise in κ  after GBDP suggests the involvement of an additional mechanism. To
                                            lat
               investigate this, microstructural analyses comparing the IGP of HP, HD and GBDP magnets-represented by
               the Dy-Nd-Cu GBDP magnet-were conducted, as illustrated in Figure 5A-C. The HP magnet exhibits a thin
               amorphous IGP [Figure 5A], which is retained in the HD magnet [Figure 5B]. However, this phase
               transforms into a thick crystalline IGP after GBDP [Figure 5C and D]. This crystallization of the IGP after
               GBDP is likely a key factor driving the pronounced increase in κ , as crystalline IGPs typically exhibit
                                                                         lat
               higher phonon mean free paths and reduced phonon scattering compared to their amorphous counterparts,
                                [30,55,56]
               thereby improving κ   . Additionally, the prolonged heat treatment during GBDP may also contribute to
               the increase in κ  by reducing point defect scattering. The reduced content of ferromagnetic elements
                              lat
               (Fe + Co) in the IGP after GBDP contributes to the enhanced coercivity [Figure 1B] by reducing the M of
               the IGP [39-41,57] . However, the impact of this compositional change on σ  and  κ still requires further
                                                                               xx
               investigation. The mechanism of IGP thickening and crystallization can be described as follows. During
               GBDP, the diffusion source, consisting of eutectic alloys, melts and infiltrates the magnet through the grain
               boundaries. This process increases the thickness and volume fraction of the RE-rich phase in the IGP and
               modifies its composition. The thickening of the IGP during GBDP, combined with prolonged annealing,
               likely explains the observed crystallization.
               Here we show the transverse thermoelectric conversion properties of the studied magnets. Figure 6A
               presents the A  and ϕ  images of the studied magnets at f = 1.0 Hz and J  = 1.0 A, measured in the M  state
                                                                             c
                                                                                                     r
                                  odd
                           odd
               under zero H. Uniform current-induced temperature modulation is clearly observed across the entire
               surface of the magnet slabs. To quantitatively estimate the anomalous Ettingshausen coefficient
               Π  (=S T), the A  per unit charge current density j , i.e., A /j , was measured at different f ranging from
                AEE
                                                                   odd c
                                odd
                      ANE
                                                             c
               1.0 Hz to 10.0 Hz, as shown in Figure 6B. The A  values at each f were obtained by averaging the A odd
                                                          odd
               values over the marked rectangular area (1.2 × 4.5 mm ) in Figure 6A. A clear decrease in A /j  with
                                                                2
                                                                                                 odd c
               increasing f was observed, which is well replicated by considering thermal diffusion in the sample using the
               one-dimensional heat diffusion equation in the frequency domain (solid lines in Figure 6B) . Finally, the
                                                                                             [27]
               steady-state value of A /j , corresponding to f → 0 Hz (A , /j ), was calculated from fitting the curve in
                                                                 odd 0Hz c
                                  odd c
               Figure 6B. The signal with  ϕ  approximately 180º indicates that the bottom surface of the sample
                                         odd
               (-y direction) is being heated, as illustrated in Figure 6C.
               The Π  and S  values were calculated using Π  = S T =            , where L is the sample thickness and
                                                         AEE
                    AEE
                            ANE
                                                              ANE
               ∆T  represents the temperature difference between the top and bottom surfaces of the sample induced by
                  AEE
                                                                                   [45]
               AEE. This temperature difference is determined as ∆T  = 2A ,  (M /M ) . An M /M  correction is
                                                                                           s
                                                               AEE
                                                                                              r
                                                                              s
                                                                                 r
                                                                       odd 0Hz
               applied to address the incomplete saturation of the studied magnets’ M during the AEE measurements. To
               ensure accurate determination of the M /M  values for the LIT sample slabs, their magnetic hysteresis loops
                                                 s
                                                    r
               were measured using a pulse B-H tracer [Supplementary Figure 4], and the results are summarized in
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