4
magnetic order of the substrate, so the non-linear part of the transverse signal can be directly
ascribed to SHHE as explained in the following.
As illustrated in Fig. 1(a), with Bz, the spin precession leads to non-zero projection of the
spin polarization of on , which generates a non-zero projection of on (Hall signal) via
ISHE. At low field (weak precession), the effect is linear (Bz) according to Eq. (1) and Fig. 2(b).
At high field (strong precession), the transverse effect is expected to vanish because the projection
of on cancels due to the large precession angle. This overall nonlinear effect is consistent
with the observation in Fig. 1(c).
The observation of the non-quadratic longitudinal and the non-linear transverse field
dependence in Figs. 1(b) and (c) respectively, suggests the strong-precession condition of SHHE
in Eq. (1). In principle, all the parameters contributing to SHHE, i.e., s, SH, and s can be
extracted by fitting the experimental data using the field dependence in Eq. (1). On the other hand,
a scaling rule pointed out by Dyakonov [15] (Sec. S3 within the Supplemental Material [21]) also
needs to be considered, as described below.
Considering the spin-precession nature, the SHHEs are expected to scale with the spin
precession time
. For d/s →∞ (thick film limit),
is limited by the spin relaxation time s, i.e.,
=s, as illustrated in Fig. 1(a). For d/s →0 (thin film limit), spin precession occurs over the
entire film thickness, so
is the same as the spin diffusion time
, where
is the spin diffusion coefficient. Dyakonov then introduced the definition
to describe the dependence of
on both s and [15]. As shown in Fig. 2,
L,SHHE and T,SHHE simulated according to Eq. (1) are normalized with the maximum longitudinal
effect L,SHHE(Bz=∞) and plotted as a function of
. Indeed, the “scaled” field dependence of
SHHE maintains roughly the same curve shape despite that the value of d/s changes over four
orders of magnitude.
The Dyakonov’s scaling rule suggests that it is difficult to unambiguously determine s,
SH, and s altogether by fitting the measured field dependence of SHHE/L0 using Eq. (1)
considering the experimental uncertainty, because it is
instead of s that can be directly extracted.
On the other hand, here we notice that s can be estimated based on the thickness dependence of
SHHE, which can then be used to extract (out of
) and SH. A close look at Eq. (1) reveals that
the low-field SHHE/L0 has a maximum at an intermediate film thickness because it vanishes in
both the thin and thick film limits: For d/s→0 (thin film limit), SHHE approaches zero because
→0 means no precession; for d/s →∞ (thick limit), SHHE/L0 also approaches zero because
the effect of the spin precession that occurs at the boundary is unimportant for thick films. It turns
out that the thickness for reaching maximum low-field SHHE/L0 only depends on s, or d/s4.56
and d/s3.28 for L,SHHE/L0 and T,SHHE/L0 respectively (Sec. S3 within the Supplemental
Material [21]), as also given by Eq. S36 and Eq. S38 in ref. [16].
Considering this property, we measured the thickness dependence of SHHE in the epitaxial
Pt films. The experimental L,SHHE/L0 is calculated by subtracting the OMR contribution, i.e.,
[L(Bz) - L(By)]/L0. Fig. 3 shows the thickness dependence of experimental L,SHHE/L0 at 4
T field. Meanwhile, the experimental T,SHHE/L0 is calculated by subtracting the linear OHE