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arxiv: 2512.19065 · v2 · submitted 2025-12-22 · ❄️ cond-mat.mes-hall · cond-mat.other

Signature of inverse orbital Hall effect in silicon studied using time-resolved terahertz polarimetry

Pith reviewed 2026-05-16 20:49 UTC · model grok-4.3

classification ❄️ cond-mat.mes-hall cond-mat.other
keywords inverse orbital Hall effectsiliconanomalous Hall conductivityterahertz spectroscopyphotocarriersorbitronicscircularly polarized lightroom temperature
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The pith

Circularly polarized light induces a long-lived helicity-dependent anomalous Hall conductivity in silicon at room temperature.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper examines the anomalous Hall conductivity generated in silicon by circularly polarized near-infrared light at room temperature through pump-probe terahertz spectroscopy. By using time-resolved detection, it isolates a long-lived conductivity that varies with the light's helicity. This conductivity has a size similar to gallium arsenide even though silicon has much weaker spin-orbit coupling, and it stays steady across different photon energies unlike spin-related effects tied to the bandgap. The findings point to an orbital mechanism known as the inverse orbital Hall effect, which could enable practical orbitronic devices based on silicon.

Core claim

Using near-infrared pump and terahertz probe spectroscopy, we detect a long-lived anomalous Hall conductivity in silicon photocarriers at room temperature that depends on the helicity of the pump light. The conductivity magnitude is comparable to that observed in GaAs, and remains robust against changes in near-infrared photon energy. These features indicate that the effect arises from the inverse orbital Hall effect rather than spin polarization, since silicon's spin-orbit coupling is weak and spin effects are energy-dependent near the gap.

What carries the argument

Time-resolved terahertz polarimetry that isolates the helicity-dependent anomalous Hall conductivity of photocarriers from short-lived nonlinear currents, revealing the inverse orbital Hall effect.

If this is right

  • The inverse orbital Hall effect operates in silicon at room temperature without needing strong spin-orbit coupling.
  • Orbital angular momentum transport produces measurable transverse conductivity in photocarriers.
  • Silicon becomes viable for orbitronic applications that integrate with existing semiconductor technology.
  • Helicity-dependent Hall signals can be used to study orbital currents separately from spin currents.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Similar orbital Hall signatures may appear in other weak spin-orbit semiconductors such as germanium.
  • Light-controlled orbital currents could enable low-dissipation logic elements compatible with silicon electronics.
  • Varying carrier density and magnetic field strength would allow quantitative extraction of orbital Hall conductivity values.
  • The method provides a template for detecting orbital effects in other centrosymmetric materials.

Load-bearing premise

The assumption that robustness against photon energy and magnitude comparable to GaAs sufficiently rules out spin-polarization mechanisms and other non-orbital contributions.

What would settle it

A strong variation of the anomalous Hall conductivity with photon energy near the silicon bandgap, or the absence of the effect in silicon samples where orbital angular momentum is suppressed, would challenge the orbital interpretation.

Figures

Figures reproduced from arXiv: 2512.19065 by Ami Mi Shirai, Changsu Kim, Hidefumi Akiyama, Jun Yoshinobu, Kota Aikyo, Ryusuke Matsunaga, Shinji Miwa, Tomohiro Fujimoto, Yuta Murotani.

Figure 1
Figure 1. Figure 1: FIG. 1 [PITH_FULL_IMAGE:figures/full_fig_p010_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. (a) [PITH_FULL_IMAGE:figures/full_fig_p011_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. (a) [PITH_FULL_IMAGE:figures/full_fig_p012_3.png] view at source ↗
read the original abstract

We investigated the anomalous Hall conductivity induced in silicon by circularly polarized light at room temperature using near-infrared (NIR) pump-terahertz (THz) probe spectroscopy. The time-resolved detection scheme eliminates the large nonlinear current generated by the field-induced circular photogalvanic effect, allowing exclusive observation of a long-lived anomalous Hall conductivity of photocarriers that depends on the helicity of NIR light. The magnitude of this conductivity is comparable to that of GaAs despite silicon's much weaker spin-orbit coupling, and its robustness against NIR photon energy rules out a spin-polarization-based origin, which occurs only in the vicinity of the bandgap. These results suggest the emergence of the inverse orbital Hall effect, paving the way for silicon-based orbitronics.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

3 major / 2 minor

Summary. The paper reports an experimental investigation of helicity-dependent anomalous Hall conductivity in silicon photocarriers at room temperature using near-infrared pump and time-resolved terahertz probe spectroscopy. The time-resolved scheme is used to suppress the circular photogalvanic effect, isolating a long-lived conductivity signal that depends on NIR light helicity. The authors note that the signal magnitude is comparable to GaAs despite silicon's weaker spin-orbit coupling and that it persists across a range of NIR photon energies, leading them to attribute the effect to the inverse orbital Hall effect rather than spin-polarization mechanisms.

Significance. If the orbital origin is rigorously established, the result would be significant for demonstrating orbitronic phenomena in elemental silicon, a technologically dominant material with weak spin-orbit coupling, thereby supporting the development of silicon-based orbitronics. The experimental isolation of a long-lived helicity-dependent Hall signal via time-resolved THz polarimetry is a technically interesting approach, but the current evidence remains suggestive rather than conclusive due to the absence of quantitative modeling that excludes alternative spin or scattering contributions.

major comments (3)
  1. [Abstract] Abstract and interpretation section: The claim that photon-energy independence across the NIR range definitively rules out spin-polarization mechanisms is not supported by any quantitative estimate or referenced calculation of the expected spin-Hall conductivity arising from indirect transitions, photo-induced scattering, or valley mixing in silicon under the specific experimental conditions (pump fluence, wavelength range, and room-temperature carrier dynamics).
  2. [Results] Results section: The statement that the observed conductivity magnitude is comparable to that in GaAs is presented without error bars, uncertainty quantification, or details on how the values were extracted from the THz polarimetry data, which weakens the cross-material comparison used to argue against spin-orbit-coupling scaling.
  3. [Discussion] Discussion: No explicit comparison is made to a spin-Hall model or prior calculation for silicon in the indirect-gap regime that would show the expected spin-derived signal to be orders of magnitude smaller than the measured conductivity; this leaves the orbital attribution as an interpretation rather than a demonstrated exclusion of spin-based alternatives.
minor comments (2)
  1. [Methods] The manuscript would benefit from a figure or schematic illustrating the time-resolved detection geometry and how it temporally separates the instantaneous circular photogalvanic current from the long-lived anomalous Hall response.
  2. [Abstract] Notation for the anomalous Hall conductivity (e.g., units and normalization to carrier density) should be clarified consistently between the abstract, figures, and text to avoid ambiguity in magnitude comparisons.

Simulated Author's Rebuttal

3 responses · 0 unresolved

We thank the referee for the careful and constructive review of our manuscript. The comments have helped us strengthen the presentation of our results and the supporting arguments. We address each major comment below and have revised the manuscript to incorporate additional details, references, and clarifications as appropriate.

read point-by-point responses
  1. Referee: [Abstract] Abstract and interpretation section: The claim that photon-energy independence across the NIR range definitively rules out spin-polarization mechanisms is not supported by any quantitative estimate or referenced calculation of the expected spin-Hall conductivity arising from indirect transitions, photo-induced scattering, or valley mixing in silicon under the specific experimental conditions (pump fluence, wavelength range, and room-temperature carrier dynamics).

    Authors: We appreciate this point and agree that a more explicit quantitative anchor would strengthen the interpretation. Our original reasoning rested on the well-established energy dependence of spin-related effects being confined near the direct gap, while our data span the indirect regime. In the revised manuscript we now cite prior calculations of spin Hall conductivity in silicon for indirect transitions and room-temperature conditions, and we include a brief order-of-magnitude estimate (based on literature spin-orbit parameters and carrier densities) showing that any spin-derived contribution remains at least an order of magnitude below the measured signal under our fluence and wavelength range. This addition makes the exclusion of spin mechanisms more quantitative while preserving the original conclusion. revision: yes

  2. Referee: [Results] Results section: The statement that the observed conductivity magnitude is comparable to that in GaAs is presented without error bars, uncertainty quantification, or details on how the values were extracted from the THz polarimetry data, which weakens the cross-material comparison used to argue against spin-orbit-coupling scaling.

    Authors: We thank the referee for highlighting this presentational gap. The conductivity values were obtained from the imaginary part of the THz conductivity spectra via standard Drude-Lorentz fitting after Fourier transformation of the time-domain traces, with uncertainties propagated from the signal-to-noise ratio and fitting residuals. In the revised version we have added error bars to the relevant figures, included a concise description of the extraction procedure in the methods section, and reported the numerical values with their uncertainties to support the GaAs comparison. revision: yes

  3. Referee: [Discussion] Discussion: No explicit comparison is made to a spin-Hall model or prior calculation for silicon in the indirect-gap regime that would show the expected spin-derived signal to be orders of magnitude smaller than the measured conductivity; this leaves the orbital attribution as an interpretation rather than a demonstrated exclusion of spin-based alternatives.

    Authors: We agree that an explicit side-by-side comparison improves rigor. The revised discussion now directly references existing spin-Hall calculations for silicon in the indirect-gap regime at room temperature and contrasts them with our measured conductivity. These models predict spin-derived signals that are suppressed by at least one to two orders of magnitude relative to our observations, consistent with silicon’s weak spin-orbit coupling. This addition converts the orbital attribution from an interpretation into a more substantiated exclusion of the dominant spin-based alternatives. revision: yes

Circularity Check

0 steps flagged

No circularity; experimental controls support interpretation without reduction to inputs

full rationale

The paper reports time-resolved THz measurements of helicity-dependent anomalous Hall conductivity in photoexcited silicon. The claim of inverse orbital Hall effect rests on (i) elimination of instantaneous photogalvanic currents via the detection scheme, (ii) persistence of the signal across NIR photon energies above the indirect gap, and (iii) magnitude comparison to GaAs despite weaker SOC. These are independent experimental observations and known band-structure facts, not a derivation that reduces to a fitted parameter or self-citation by construction. No equations or ansatzes are presented that equate the observed conductivity to an orbital Hall term via definition. The interpretation is falsifiable by future spin-Hall calculations or controls, satisfying the criterion for non-circularity.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The claim rests on standard semiconductor transport models and the assumption that photon-energy independence excludes spin-based mechanisms; no new free parameters or invented entities are introduced in the abstract.

axioms (1)
  • standard math Standard models of photogalvanic effects and Hall conductivity in semiconductors apply to the observed signals.
    The separation of nonlinear currents from the anomalous Hall conductivity relies on established time-resolved transport physics.

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