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REVIEW 3 major objections 5 minor

From Zero to Mega-Gauss Fields: Comprehensive Magnetophotonic Spectroscopy of Graphene Dirac Cones

T0 review · 3 major / 5 minor · reviewed 2026-08-12 · deepseek-v4-flash

Pith's one-line read This paper claims that the anomalously broad infrared absorption of electron-doped graphene at fields up to 560 T is a collective Alfvén wave in a field-created electron-hole plasma, not cyclotron resonance.

desk verdict The ARPES camel-back measurement is the real nugget; the Alfvén-wave story rests on an unconstrained κB coupling and should be treated as speculation until κ is derived or measured. read the letter →

arxiv 2608.10638 v2 pith:DVNOFVYN submitted 2026-08-11 cond-mat.mes-hall

classification cond-mat.mes-hall PACS 71.70.Di73.22.Pr78.20.Ls
keywords ultrahighmagneticfieldsgraphenemagneto-opticalspectroscopyAlfvénwavesLandaulevelcrossingARPESelectron-holeplasmasublatticeasymmetry
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

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

The reading

The paper claims that the infrared absorption of heavily electron-doped epitaxial graphene in ultrahigh magnetic fields — up to 560 T — is not the ordinary cyclotron resonance of individual electrons, but a collective hydromagnetic wave (an Alfvén wave) propagating in an electron-hole plasma that is created when the two zero Landau levels cross near 160–200 T. The argument runs through a distorted Dirac band measured by ARPES: a 'camel-back' dispersion with a ~0.2 eV gap, fitted with a bilayer-style formula whose parameters feed a Landau-level fan chart predicting the level crossing. If the claim is right, megagauss fields turn a 2D solid into a fully compensated, charge-neutral electron-hole plasma that is a tabletop analog of the relativistic electron-positron plasmas of pulsar magnetospheres, and the anomalously broad spectra that earlier work treated as single-particle cyclotron resonance are reinterpreted as a collective mode. The authors fit the extreme-field spectra with a collective Alfvén wave model and read the enlarged sublattice asymmetry (0.10 to 0.12 eV) as a magnetic-field-driven many-body effect.

What carries the argument

The argument is carried by an effective band model and a field-dependent Landau-level Hamiltonian. The band model is a bilayer-graphene dispersion $E_\pm(k) = \pm\sqrt{\Delta_0^2 + \gamma_1^2/2 + (v_F \hbar k)^2} - \sqrt{\gamma_1^4/4 + (v_F\hbar k)^2(\gamma_1^2 + 4\Delta_0^2)}$, used with monolayer parameters ($v_F = 1.06\times10^6\ \mathrm{m/s}$, $\Delta_0 = 0.10\ \mathrm{eV}$, $\gamma_1 = 0.39\ \mathrm{eV}$) to reproduce the camel-back band that ARPES resolves. The Hamiltonian assigns the zero modes diagonal energies $E^0_{n,\mathrm{CB}} = \Delta_0 + \kappa n B$ and $E^0_{n,\mathrm{VB}} = -\Delta_0 - \kappa n B$, i.e., a linear magnetic-field coupling $\kappa B$ that the paper never quantifies and presents as the macroscopic realization of the Berry-curvature orbital magnetic moment of the warped cone; it is this $\kappa B$ term, not the standard inter-level coupling $\beta\sqrt{n}B$ ($\beta = v_F\sqrt{2e\hbar}$), that closes the gap, brings the zero modes to their 160–200 T crossing, and inverts the band order. The absorption spectra are then computed from the collective Alfvén wave dielectric function by summing over Fermi-Dirac-occupied Landau levels with a scattering lifetime $\tau \approx 4$ fs, which turns the fan chart into the fitted line shapes.

What would settle it

Directly measure the field dependence of the two zero Landau levels with a probe that does not assume the Alfvén model — for example, high-field scanning tunnelling spectroscopy of the $N = 0^+$ and $N = 0^-$ states, or magneto-Raman detection of the gap — and check whether they converge and cross near 160–200 T; if the levels do not invert (or if an independent determination shows $\kappa$ is too small or of the wrong sign to close the 0.2 eV gap at that field), the electron-hole plasma and the Alfvén-wave assignment collapse. A cheaper version: measure the shoulder's resonance field at a second photon energy and check whether the same, unadjusted $\kappa$ reproduces it.

Watch

Extended reading notes

Core claim

On the paper's terms, the central discovery is a field-driven change of regime in a gapped Dirac system. The $N = 0^+$ and $N = 0^-$ Landau levels, separated at zero field by the 0.2 eV sublattice-asymmetry gap, converge and cross near 160–200 T under a linear magnetic-field coupling $\kappa B$ assigned to the zero modes; beyond the crossing the gap is inverted, and the system becomes a dense, fully compensated electron-hole plasma. In this regime the measured absorption under a 0.636 eV thulium-fibre laser — a massive resonance near 400 T with a shoulder near 200 T — is reproduced by a collective Alfvén wave dielectric function, and the fitted field-renormalized asymmetry $\Delta_B = 0.12\ \mathrm{eV}$ exceeds the zero-field value $\Delta_0 = 0.10\ \mathrm{eV}$. The authors state that the magneto-absorption features 'represent absolutely nothing other than the collective Alfvén wave propagation,' making the megagauss graphene a pristine laboratory analog of relativistic electron-positron plasmas.

Load-bearing premise

The load-bearing premise is the unmeasured linear magnetic-field coupling $\kappa B$ placed in the Landau-level Hamiltonian: it is the only mechanism that pulls the $N = 0^+$ and $N = 0^-$ levels into their 160–200 T crossing, yet the paper assigns it no numerical value, derives it from no ARPES band parameter, and concedes in Sec. 3.3 that applying the bilayer-derived model to the monolayer is 'physically inappropriate.'

Editorial extensions

If this is right

  • The STC-regime absorption dips that look like cyclotron resonance are collective electron plasma modes (helicon-like), so reading them with the single-particle $\sqrt{B}$ rule gives systematically wrong assignments — the $0^+\to 2^+$ transition, not $0^+\to 1^+$, is the relevant one at low fields.
  • Near 160–200 T the $N=0^+$ and $N=0^-$ levels cross and invert the gap, driving the doped monolayer into a fully compensated electron-hole plasma whose optical response is a cooperative electron-hole excitation.
  • The field-renormalized sublattice asymmetry exceeds its zero-field value ($\Delta_B = 0.12\ \mathrm{eV} > \Delta_0 = 0.10\ \mathrm{eV}$), evidence that the strong electron-hole interaction amplifies the intrinsic A–B asymmetry rather than merely widening a gap.
  • Because the post-crossing fluid is two-component and charge-neutral, it decouples charge and momentum currents, unlike a single-component Galilean-invariant metal, providing a tabletop analog of relativistic electron-positron and quark-gluon plasmas.
  • The Alfvén resonance survives even though the fitted single-particle scattering lifetime is extremely short ($\tau \approx 4$ fs), because the collective mode outlasts individual particle coherence once the magnetic tension stiffens the plasma.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The paper's own mechanism implies a falsifiable scaling that it does not state: the same unquantified $\kappa$ that fixes the 160–200 T crossing should also fix the resonance field for any other photon energy, so a second laser wavelength would discriminate the Alfvén model from single-particle fits with no free parameters.
  • If the crossing interpretation is correct, the system realizes the reverse of magnetic catalysis — field-induced gap closure and inversion rather than gap opening — which predicts that other substrate-interacting Dirac materials with a comparable zero-field gap would show the same regime change at fields scaled by their gap size.
  • The claim that $\Delta_B$ rises while $v_F$ stays essentially fixed suggests the many-body renormalization is primarily orbital; an independent probe of the gap at ultrahigh fields, such as magneto-Raman scattering or two-colour pump-probe across the camel-back, could measure $\Delta_B$ without relying on the Alfvén line shape.
  • A temperature or gate-density sweep across the crossing should sharpen the shoulder-versus-peak structure if the plasma picture is right, because the degree of electron-hole compensation at the crossing is set by doping and thermal occupation, whereas a single-particle transition would barely respond to either.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 5 minor

Summary. The paper reports infrared magneto-absorption spectra of n-doped epitaxial graphene on 4H-SiC measured in pulsed fields up to 560 T using single-turn coil and electromagnetic flux compression techniques. ARPES measurements reveal a distorted Dirac dispersion with a camel-back structure and a gap of about 0.2 eV, which the authors model with a bilayer-graphene-type dispersion (Eq. 1). From the extracted band parameters they construct Landau-level fan charts using an effective Hamiltonian that includes a linear-in-B coupling κB (Appendix Eq. A1). This term makes the N=0+ and N=0- Landau levels converge and cross near 160-200 T, which is interpreted as a transition into a compensated electron-hole plasma. The broad high-field absorption features are then fitted with a collective Alfvén-wave dielectric function (Eq. S5), yielding parameters vF, ΔB, EF, ΓB, and τ; the extracted ΔB = 0.12 eV is compared with Δ0 = 0.10 eV as evidence of field-enhanced sublattice asymmetry. The paper concludes that the megagauss response is a laboratory analog of relativistic pair plasmas.

Significance. If the central scenario were correct, the paper would report a remarkable collective hydromagnetic response in a two-dimensional Dirac material, with potential implications for analogies between condensed matter and astrophysical pair plasmas. The experimental data themselves, obtained in the megagauss range up to 560 T, are a valuable and unusual resource, and the ARPES measurements clearly document a camel-back dispersion and a large gap in this epitaxial system. The paper is also transparent about the effective nature of its model, explicitly flagging in Sec. 3.3 that the bilayer-derived formulation is not directly applicable to a monolayer. However, the paper's main scientific claim—the zero-mode Landau-level crossing and the Alfvén-wave interpretation—rests entirely on an unconstrained and unexplained linear coupling κB, and the supporting fit to the high-field spectra is circular in its use of the same parameters to confirm the crossing. As presented, the analysis does not establish the proposed physical mechanism.

major comments (3)
  1. [Sec. 3.3 and Appendix Eq. A1] The linear magnetic-field coupling κB introduced in Eq. (A1) is the sole mechanism that makes the N=0+ and N=0- Landau levels converge and cross, yet it is never derived from the ARPES band parameters, never assigned a numerical value, and never constrained by an independent measurement. Section 3.3 itself concedes that applying the bilayer-derived formulation to a monolayer is 'physically inappropriate', and the κB term is then inserted as an ad hoc replacement for the γ1 physics. Because the diagonal zero-mode energies in Eqs. (A2)-(A3) are ±Δ0, the claimed inversion can only arise from the off-diagonal κB coupling; for κ=0, for a smaller value, or for the opposite sign, the gap would instead widen with field (magnetic catalysis) and the 160-200 T crossing would not occur. The fan chart in Fig. 3 is therefore not a prediction of the measured band parameters but an assumption. The authors must provide a microscopic derivation of κ from the distorted band structure or an independent determination of its value and sign before the crossing scenario can be accepted.
  2. [Sec. 3.4, Eq. S5, and Table 2] The Alfvén-wave model of Eq. (S5) is used to fit the same high-field spectra shown in Fig. 4 with five free parameters (vF, ΔB, EF, ΓB, τ; Table 2), and the resulting parameters are then inserted into the fan chart of Fig. 5, which is cited as confirming the zero-mode crossing and the shoulder at roughly 200 T. This is circular: the shoulder is reproduced by a model whose input already includes the renormalized ΔB and the very crossing the model is supposed to validate. The fit quality is presented only as 'excellent', with no residuals, confidence intervals, or comparison to a conventional cyclotron-resonance or other alternative model. The claim in Sec. 3.4 that the features 'represent absolutely nothing other than' Alfvén-wave propagation is therefore not supported by the evidence. The authors should provide quantitative model-comparison statistics (e.g., reduced chi-squared or information criteria), parameter uncertainties, and ideally an out-of-sample test in which one sample is fitted and the other is predicted.
  3. [Sec. 3.4 and Table 2] The reported enhancement ΔB = 0.12 eV > Δ0 = 0.10 eV is read off the same Alfvén-wave fit that defines the post-crossover plasma phase; there is no independent high-field measurement of the sublattice asymmetry. The statement that this difference 'directly signifies' a macroscopic many-body amplification of the sublattice asymmetry is thus an interpretation of a fit parameter rather than an observed quantity. An independent test would be, for example, a prediction of the field dependence of individual Landau-level transition energies or a separate probe of the gap in the plasma phase; without such a test, the ΔB enhancement does not provide independent support for the Alfvén scenario.
minor comments (5)
  1. [Eqs. S1-S2 and Table 2] In Eqs. (S1) and (S2), τ is treated as a dimensionless broadening parameter, but Table 2 lists τ in femtoseconds; the relationship between these two quantities should be clarified.
  2. [Fig. 4 and Sec. 3.4] The text and figure mark fields above about 500 T as potentially contaminated by stray infrared radiation, yet the Alfvén fit and the fan chart in Fig. 5 extend to 560-800 T; the manuscript should state explicitly how the fit treats the potentially contaminated region.
  3. [Sec. 3.4] The phrase 'Alfv’en' should be corrected to 'Alfvén'.
  4. [Sec. 3.3] The interpretation of the low-field features as collective helicon waves is mentioned qualitatively, but no helicon dispersion, model, or fitting procedure is provided; either add the model or clearly label this part as a qualitative suggestion.
  5. [Tables 1 and 2] Table 2 lists E_F = 40 meV for Sample A and 100 meV for Sample B, whereas Table 1 lists 50 meV and 90 meV; the discrepancies and their origin should be explained.

Circularity Check

3 steps flagged · score 8.0 of 10

The N=0+/0− crossing is generated by the κB term introduced to produce it, and the ΔB>Δ0 enhancement is a free fit to the same spectra it is then used to explain.

  1. self definitional [Appendix Eq. A1–A3; Sec. 3.3 'Landau Level Fan Chart and Optical Transitions']
    "To accurately capture these complex behaviors—particularly the anomalous level-crossing driven by the giant orbital magnetic moment associated with the gapped Dirac topology—we explicitly introduce a linear magnetic field term κB into the effective model. ... Crucially, it is the presence of this linear term κB that overcomes the initial energy gap 2∆0 and dictates the anomalous energy evolution of the zero-mode Landau levels. As a direct consequence, this term induces the critical level crossover between the 0+ and 0− states observed in the ultrahigh-field regime."

    The central prediction—that N=0+ and N=0− cross near 160–200 T and create the electron-hole plasma—is produced entirely by κB, a term the paper explicitly introduces 'to accurately capture' the level-crossing. No numerical value or independent derivation of κ is given. In Eqs. A2–A3 the diagonal zero-mode energies are ±Δ0 with no κ·n·B shift (n=0), so the crossing arises only from the unconstrained off-diagonal κB coupling. The claimed prediction is therefore equivalent to the assumption that κB exists and has the right sign and magnitude. Section 3.3 further concedes that directly applying the bilayer-derived Hamiltonian to the monolayer is 'physically inappropriate,' making κ an ad hoc replacement for the bilayer γ1 physics rather than a parameter with independent support.

  2. fitted input called prediction [Sec. 3.4, Table 2 and discussion of ΔB > Δ0]
    "The experimental waveforms are reproduced by the physical parameters extracted from the fitting, and the results are listed in Table 2. ... Once the N=0 levels invert and the system enters the collective Alfvén wave regime (200–560 T), our analysis reveals a dynamically enhanced parameter ΔB > Δ0. ... this remarkable increase in ΔB indicates that the strong interactions between the coexisting electrons and holes strictly amplify the fundamental sublattice potential asymmetry of the system."

    The claimed magnetic-field-induced enhancement of the sublattice asymmetry (ΔB = 0.12 eV > Δ0 = 0.10 eV) is obtained by fitting ΔB to the very high-field absorption spectra that the model is then used to explain. Table 2 lists ΔB as a fitting parameter together with vF, EF, ΓB, and τ. The 'evidence' for the many-body enhancement is therefore a restatement of the fitted value, not an independent observation or prediction. The comparison with the ARPES value Δ0 is a comparison between two separate fits, which does not test the claim that the magnetic field dynamically amplifies the sublattice asymmetry.

1 more flagged steps
  1. self definitional [Sec. 3.4, paragraphs discussing Fig. 4 and Fig. 5]
    "The solid green and dashed blue arrows indicate resonant optical transitions that quantitatively match the 0.636 eV photon energy of the thulium fiber laser. ... The transitions at 440 T and 220 T directly correspond to the main absorption peak and its shoulder structure, respectively, as visualized in Fig. 4."

    The shoulder near 200 T is presented as the experimental confirmation of the 0+/0− crossing, but the fan chart that produces the 220 T transition is computed with the parameters fitted to those same spectra (Table 2) and with the κB term that was introduced to force the crossing. Observing a spectral feature and assigning it to a model element that was put in by hand does not independently validate the crossing. The agreement is a consequence of the model inputs, not a test of them.

full rationale

The paper's central narrative has two load-bearing steps, and both reduce to their own inputs. First, the zero-mode level crossing near 160–200 T—the event that converts the system into a compensated electron-hole plasma and motivates the Alfvén-wave interpretation—is not derived from the ARPES band parameters. It is generated by the linear coupling κB in Eq. A1, which the Appendix says is introduced 'to accurately capture' the level-crossing; the diagonal zero-mode energies (Eqs. A2–A3 with n=0) are ±Δ0 with no κ·n·B shift, so the crossing comes entirely from the unconstrained off-diagonal κB coupling. Section 3.3 concedes that the bilayer-derived Hamiltonian is 'physically inappropriate' for the monolayer, making κ an ad hoc patch rather than a parameter with independent support. Second, the field-induced enhancement ΔB = 0.12 eV > Δ0 = 0.10 eV is a free fitting parameter in Table 2, adjusted to reproduce the same high-field absorption spectra that are then offered as evidence of the many-body enhancement. The 'outstanding agreement' with ARPES is an agreement between two fitting exercises, not an independent prediction. The shoulder at ~200 T is likewise labeled as the crossing, but the fan chart that produces the 220 T transition uses the fitted parameters and the κB term. The ARPES dispersion and gap do provide some independent input (vF, Δ0), which prevents a score of 10, but the core magneto-optical reinterpretation—the crossing, the plasma phase, and the apparent ΔB enhancement—is forced by construction.

Assumptions & free parameters 9 free parameters · 6 assumptions · 1 invented entities

The central scenario rests on one unconstrained parameter (kappa) and several fitted parameters (vF, Delta_B, EF, Gamma_B, tau) within a model that the authors themselves say is physically inappropriate for a monolayer. The claimed Delta_B > Delta_0 effect is the difference between two fits, not an independent measurement.

free parameters (9)
  • kappa (linear field coupling) = not reported
    Introduced in Appendix Eq. A1 to produce the N=0+/0- level crossing near 160 to 200 T; no microscopic derivation or magnitude is given.
  • Delta_0 (ARPES fit) = 0.10 eV
    Fitted to the ARPES intensity map using Eq. (1).
  • v_F (ARPES fit) = 1.06 x 10^6 m/s
    Fitted to the ARPES intensity map.
  • gamma_1 (effective interlayer coupling) = 0.39 eV
    Taken from bilayer graphene literature and used as an effective parameter to reproduce band warping; not independently measured for this monolayer.
  • Delta_B (renormalized sublattice asymmetry) = 0.12 eV
    Fitted in the Alfvén wave model for both samples (Table 2); the claimed field-induced enhancement over Delta_0 is this fitted difference.
  • v_F (Alfvén model) = 0.97 / 0.86 x 10^6 m/s
    Fitted per sample in the Alfvén model (Table 2).
  • E_F (Alfvén model) = 40 / 100 meV
    Fitted per sample; consistent with transport values but not fixed by them.
  • Gamma_B (total broadening) = 0.14 / 0.13 eV
    Fitted per sample in the Alfvén model.
  • tau (scattering lifetime) = 4 fs
    Fitted and interpreted as a new scattering regime; differs from the roughly 12 fs implied by the mobility.
assumptions (6)
  • ad hoc to paper Eq. (1), the bilayer-graphene dispersion, is a valid effective description of the distorted monolayer Dirac cone.
    Sec. 3.2 uses gamma1 = 0.39 eV from bilayer graphene to model monolayer epitaxial graphene, while Sec. 3.3 admits applying the bilayer Hamiltonian to the monolayer is physically inappropriate.
  • domain assumption The ARPES-measured band structure on an annealed surface is representative of the unannealed optical samples.
    Samples were annealed at 500 C for ARPES; the magneto-optical samples were not, and no direct correlation is established.
  • domain assumption Valley splitting is negligible at these fields.
    Stated in Sec. S4: LL valley splitting of less than 10 meV is smaller than the experimental broadening.
  • ad hoc to paper The linear kappa B term captures the orbital-momentum effect of the distorted band.
    Appendix: no derivation from the band parameters is provided; the term is asserted to originate from band warping.
  • domain assumption The dielectric function Eq. (S5) describes the collective Alfvén response of the 2D electron-hole plasma.
    This is a standard linear response formula, but its application to a strongly damped, short-lifetime (tau = 4 fs) plasma is assumed rather than justified.
  • domain assumption 70 to 80% monolayer coverage is sufficient to treat the sample as a uniform monolayer.
    From Ref. [7], the remaining 20 to 30% multilayer or buffer-layer regions are ignored in the analysis.
invented entities (1)
  • Linear magnetic-field coupling term kappa B on zero-mode Landau levels
    purpose: To drive the N=0+/0- level crossing and gap inversion at 160 to 200 T
    Appears in Appendix Eq. A1 with no microscopic derivation and no reported value, and its main observational consequence is the crossing it is designed to create.

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Cite this review

Pith. "Pith review of From Zero to Mega-Gauss Fields: Comprehensive Magnetophotonic Spectroscopy of Graphene Dirac Cones." pith.science (2026). https://pith.science/paper/DVNOFVYN

@misc{pith2026260810638,
  author       = {Pith},
  title        = {Pith review of: From Zero to Mega-Gauss Fields: Comprehensive Magnetophotonic Spectroscopy of Graphene Dirac Cones},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/DVNOFVYN}},
  note         = {Machine review of arXiv:2608.10638}
}
abstract

We investigate the infrared magneto-optical response of n-doped epitaxial graphene on 4H-SiC in ultrahigh magnetic fields up to 560~T, utilizing single-turn coil and electromagnetic flux compression techniques. The measured absorption spectra are anomalously broad, strongly deviating from conventional cyclotron resonance. Angle-resolved photoemission spectroscopy (ARPES) reveals a distorted Dirac dispersion featuring a ``camel-back" structure with an energy gap of $E_g \sim 0.2$~eV. Using the band parameters extracted via a generalized bilayer graphene model, we construct a Landau level (LL) fan chart that dictates a critical level crossing between the $N=0^+$ and $N=0^-$ states near 160--200~T. At this threshold, the optical transition mechanism undergoes a dramatic shift from an electron-dominated collective mode to a cooperative electron-hole collective excitation. Furthermore, the extreme-field absorption spectra under thulium fiber laser excitation ($\hbar\omega_0 = 0.636$~eV)---culminating in a massive resonance near 400~T with a shoulder at 200~T---are excellently reproduced by a collective Alfv\'en wave model. This analysis also evidences a magnetic-field-induced enhancement of the sublattice potential asymmetry parameter (from 0.10~eV to 0.12~eV). This directly signifies that the macroscopic electron-hole band asymmetry is further amplified by the applied magnetic field. Ultimately, the field-induced energy inversion generates a strongly interacting, fully compensated electron-hole plasma. The resonant excitation of Alfv\'en waves in this regime demonstrates that a pristine tabletop analog to the relativistic electron-positron plasmas found in astrophysical extremes can be elegantly realized within a 2D graphene system.

Figures

Figures reproduced from arXiv: 2608.10638 by the authors.

Figure 1
Figure 1. displays the infrared magneto-transmission spectra obtained from the STC experiments. Here, the results for both Sample A and Sample B are plotted for three different incident light wavelengths: CO2 (9.55 µm), CO (5.7 µm), and He-Ne (3.38 µm). These weak absorption profiles stand in stark contrast to standard two-dimensional electron gases (2DEGs) hosted in semiconductor heterostructures, such as InAs/AlSb single qu… view at source ↗
Figure 2
Figure 2. Two-dimensional ARPES energy-momentum intensity map captured along the ky direction across the K (K′ ) high-symmetry points. The red solid line denotes the best-fit curve calculated from the model, Eq. (1), which cleanly traces the distorted dispersion Dirac band. The center of the energy gap (the yellow dashed line) is positioned approximately 0.18 eV below the Fermi energy (EF ), indicated by the sky blue dashed l… view at source ↗
Figure 3
Figure 3. Calculated Landau-level (LL) fan chart up to 200 T based on the distorted Dirac dispersion model, using parameters extracted from our ARPES analysis (vF = 1.06×106 m/s, ∆ = 0.1 eV). The red and blue curves represent the LLs for the conduction and valence bands, respectively. The solid vertical arrows (black, blue, and orange) indicate the optical transition energies corresponding to the STC experiments shown in [PI… view at source ↗
Figures from the paper (2 more)
Figure 4
Figure 4. Figure 4: Magneto-infrared absorption spectra for A: Sample A and B: Sample B in ultrahigh magnetic fields up to 560 T, measured at room temperature using a thulium fiber laser (photon energy: 0.636 eV). The solid curves represent the optical absorption spectra calculated via th…
Figure 5
Figure 5. Figure 5: Landau-level (LL) fan chart calculated up to 800 T. The upper and lower manifolds [PITH_FULL_IMAGE:figures/full_fig_p011_5.png]

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Reviewed August 12, 2026 · model on record in the stance chip above.