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arxiv: 2508.11481 · v2 · submitted 2025-08-15 · ❄️ cond-mat.mes-hall · cond-mat.mtrl-sci

Spin-to-charge-current conversion in altermagnetic candidate RuO₂ probed by terahertz emission spectroscopy

Pith reviewed 2026-05-18 22:51 UTC · model grok-4.3

classification ❄️ cond-mat.mes-hall cond-mat.mtrl-sci
keywords altermagnetismspin Hall effectterahertz emissionRuO2spin-charge conversioninverse spin splitteranisotropic transport
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The pith

In RuO2 the anisotropic inverse spin Hall effect dominates spin-to-charge conversion while any altermagnetic inverse spin-splitter effect is much smaller.

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

The paper uses terahertz emission spectroscopy on epitaxial RuO2 films to measure ultrafast spin-to-charge current conversion. It performs a quantitative breakdown of several competing contributions to the observed anisotropic signals, including the anisotropic inverse spin Hall effect, a possible altermagnetic inverse spin-splitter effect, anisotropic conductivity inside the film, and birefringence in the TiO2 substrate. The analysis finds that the inverse spin Hall effect supplies the largest term, corresponding to an average spin-Hall angle of 2.4 times 10 to the minus 3 at room temperature, while any altermagnetic contribution is only 2 to 4 times 10 to the minus 4. This separation shows that relativistic spin-orbit coupling still produces the main observed effect even in a material proposed as an altermagnet. The work therefore emphasizes that spin-dependent signals in altermagnetic candidates must be carefully isolated from ordinary spin-orbit effects before the altermagnetic order can be claimed as the source.

Core claim

Using THz emission spectroscopy on epitaxial RuO2 thin films, the leading contribution to the measured anisotropic signals is the anisotropic inverse spin Hall effect, which yields an average spin-Hall angle of 2.4 times 10 to the minus 3 at room temperature; a possible contribution from the altermagnetic inverse spin-splitter effect is found to be only 2 to 4 times 10 to the minus 4 after accounting for anisotropic conductivity in RuO2 and birefringence of the TiO2 substrate.

What carries the argument

Quantitative decomposition of THz emission signals into competing spin-to-charge mechanisms (anisotropic inverse spin Hall effect versus altermagnetic inverse spin-splitter effect) plus substrate and film conductivity corrections.

If this is right

  • The spin-Hall angle extracted for RuO2 at room temperature is 2.4 times 10 to the minus 3.
  • Any altermagnetic inverse spin-splitter effect in these films is at most 2 to 4 times 10 to the minus 4 and is not the leading term.
  • Relativistic spin-orbit coupling must still be subtracted before attributing signals to altermagnetic order in similar materials.
  • THz emission spectroscopy combined with multi-effect modeling can separate spin-orbit and altermagnetic contributions in thin films.

Where Pith is reading between the lines

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

  • Similar quantitative separation will be needed for other proposed altermagnets before their spin-splitter effects can be reliably measured.
  • If the smaller altermagnetic term grows at lower temperature or in thicker films, THz spectroscopy could still detect it once the dominant inverse spin Hall background is subtracted.
  • Device designs that rely on altermagnetic spin splitting for charge conversion will require materials where the altermagnetic contribution exceeds ordinary spin-orbit effects.

Load-bearing premise

The model that subtracts anisotropic conductivity and substrate birefringence accurately isolates the spin-dependent contributions without large fitting errors.

What would settle it

An independent electrical measurement of the spin-Hall angle in the same RuO2 films that yields a value far from 2.4 times 10 to the minus 3 would contradict the dominance claim.

read the original abstract

Using the THz emission spectroscopy, we investigate ultrafast spin-to-charge current conversion in epitaxial thin films of the altermagnetic candidate RuO$_2$. We perform a quantitative analysis of competing effects that can contribute to the measured anisotropic THz emission. These include the anisotropic inverse spin splitter and spin Hall effects in RuO$_2$, the anisotropic conductivity of RuO$_2$, and the birefringence of the TiO$_2$ substrate. We observe that the leading contribution to the measured signals comes from the anisotropic inverse spin Hall effect, with an average spin-Hall angle of $2.4\times 10^{-3}$ at room temperature. In comparison, a possible contribution from the altermagnetic inverse spin-splitter effect is found to be approximately $2-4\times 10^{-4}$. Our work stresses the importance of carefully disentangling spin-dependent phenomena that can be generated by the unconventional altermagnetic order, from the effects of the relativistic spin-orbit coupling.

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

2 major / 2 minor

Summary. The manuscript reports terahertz emission spectroscopy experiments on epitaxial RuO2 thin films to investigate ultrafast spin-to-charge current conversion. The authors perform a quantitative multi-component analysis of the anisotropic THz signals, accounting for the anisotropic inverse spin Hall effect (ISHE) and altermagnetic inverse spin-splitter effect (ISS) in RuO2, the material's anisotropic conductivity, and birefringence of the TiO2 substrate. They conclude that the dominant contribution arises from the anisotropic ISHE, yielding an average spin-Hall angle of 2.4×10^{-3} at room temperature, while any altermagnetic ISS contribution is limited to approximately 2-4×10^{-4}.

Significance. If the modeling and separation of contributions prove robust, the result is significant for spintronics and altermagnetism research. It provides concrete evidence that relativistic spin-orbit coupling effects dominate over unconventional altermagnetic order in this candidate material, offering a cautionary benchmark for interpreting THz emission data in similar systems and stressing the need for careful disentanglement of competing mechanisms.

major comments (2)
  1. [§4] §4 (Quantitative analysis and modeling): The central claim that anisotropic ISHE dominates with spin-Hall angle 2.4×10^{-3} while altermagnetic ISS is only 2-4×10^{-4} rests on a multi-component subtraction that includes RuO2 conductivity anisotropy and TiO2 birefringence. The manuscript provides insufficient detail on the fitting procedure, assumed frequency dependence, phase factors, or error propagation/sensitivity analysis; small systematic uncertainties in these inputs could re-attribute signal strength between the larger ISHE and smaller ISS channels given their factor-of-5–10 magnitude difference.
  2. [Methods] Methods section (data acquisition and processing): No explicit description is given of how raw THz waveforms are processed to extract polarization-dependent amplitudes, nor of the statistical or systematic uncertainties entering the extracted spin-Hall angle and ISS values. This information is load-bearing for assessing whether the reported quantitative separation is reliable.
minor comments (2)
  1. [Figure 2] Figure 2 or equivalent (THz emission traces): The polarization rotation angles and substrate contributions should be labeled more clearly to allow readers to follow the subtraction steps without ambiguity.
  2. [Abstract] Abstract and introduction: The phrase 'altermagnetic candidate' is used consistently, but a brief statement on the current experimental status of altermagnetic order in RuO2 (e.g., recent neutron or ARPES results) would help contextualize the claim.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the careful reading of our manuscript and the constructive comments. We appreciate the recognition that the work provides a cautionary benchmark for interpreting THz emission data in altermagnetic candidates. We address the major comments below and agree that additional details on the analysis and methods will strengthen the paper. We will incorporate these clarifications in the revised version.

read point-by-point responses
  1. Referee: [§4] §4 (Quantitative analysis and modeling): The central claim that anisotropic ISHE dominates with spin-Hall angle 2.4×10^{-3} while altermagnetic ISS is only 2-4×10^{-4} rests on a multi-component subtraction that includes RuO2 conductivity anisotropy and TiO2 birefringence. The manuscript provides insufficient detail on the fitting procedure, assumed frequency dependence, phase factors, or error propagation/sensitivity analysis; small systematic uncertainties in these inputs could re-attribute signal strength between the larger ISHE and smaller ISS channels given their factor-of-5–10 magnitude difference.

    Authors: We agree that the description of the quantitative analysis in §4 would benefit from greater detail to allow full assessment of robustness. In the revised manuscript we will expand this section to explicitly describe the multi-component fitting procedure, the functional forms and frequency dependence assumed for each contribution (anisotropic ISHE, ISS, conductivity anisotropy, and substrate birefringence), the handling of phase factors between the emitted THz fields, and a sensitivity analysis with error propagation. This will include quantitative tests showing how variations in the input parameters affect the extracted spin-Hall angle and ISS amplitude, thereby confirming that the factor-of-5–10 separation remains stable. revision: yes

  2. Referee: [Methods] Methods section (data acquisition and processing): No explicit description is given of how raw THz waveforms are processed to extract polarization-dependent amplitudes, nor of the statistical or systematic uncertainties entering the extracted spin-Hall angle and ISS values. This information is load-bearing for assessing whether the reported quantitative separation is reliable.

    Authors: We acknowledge that the current Methods section does not provide a sufficiently explicit account of waveform processing. In the revised manuscript we will add a dedicated subsection detailing the steps from raw THz time-domain waveforms to polarization-dependent amplitudes. This will include the Fourier-transform procedure, polarization decomposition, background subtraction, and the evaluation and propagation of both statistical (shot-to-shot) and systematic (alignment, substrate effects) uncertainties into the final spin-Hall angle and ISS values. revision: yes

Circularity Check

0 steps flagged

No significant circularity in experimental separation of spin-to-charge conversion mechanisms

full rationale

The paper reports THz emission measurements on RuO2 films and performs a multi-component quantitative model to isolate contributions from anisotropic inverse spin Hall effect, possible altermagnetic inverse spin-splitter effect, RuO2 conductivity anisotropy, and TiO2 substrate birefringence. The extracted spin-Hall angle and upper bound on the ISS effect are obtained by fitting the model to the measured anisotropic signals rather than by any self-definitional loop, fitted-input-renamed-as-prediction, or load-bearing self-citation chain. All load-bearing steps rely on independent physical models and external calibration data; the final numerical values are not equivalent to the inputs by construction.

Axiom & Free-Parameter Ledger

1 free parameters · 1 axioms · 0 invented entities

The claim depends on the accuracy of the model separating conventional spin-orbit effects from potential altermagnetic ones, with the spin-Hall angle as a fitted parameter.

free parameters (1)
  • spin-Hall angle = 2.4e-3
    Average value extracted from THz emission data at room temperature.
axioms (1)
  • domain assumption Competing effects can be quantitatively modeled and separated using the described analysis
    Invoked in the quantitative analysis of THz signals.

pith-pipeline@v0.9.0 · 5843 in / 1211 out tokens · 47289 ms · 2026-05-18T22:51:28.088900+00:00 · methodology

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