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TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane

T0 review · 1 major / 1 minor · reviewed 2026-06-26 · grok-4.3

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Pith's one-line read Diffuse Galactic plane gamma rays split into leptonic and hadronic parts yield neutrinos that match IceCube data even after ISRF variations.

desk verdict The paper applies standard leptonic-hadronic decomposition to LHAASO diffuse data, tests a few alternative ISRF profiles with modest results, and derives neutrino fluxes directly from the hadronic fit normalization. read the letter →

arxiv 2606.23476 v1 pith:FHXFANIH submitted 2026-06-22 astro-ph.HE

Saikat Das , Nayantara Gupta , Siyao Xu This is my paper · ORCID
classification astro-ph.HE
keywords diffusegammaraysneutrinoemissionGalacticplanecosmicinterstellarradiationfieldLHAASOIceCube
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 models LHAASO diffuse TeV-PeV gamma rays in the Galactic plane as the sum of unresolved leptonic emission from pulsar wind nebulae and hadronic emission from supernova-injected cosmic-ray protons. It tests alternative radial profiles for the infrared interstellar radiation field that increase photon density toward the inner Galaxy and measures their effect on gamma-gamma attenuation. Because the fit excludes the Galactic center direction and applies source masks, these profile changes alter the overall normalization only modestly. The hadronic component inferred from the gamma-ray data then produces pp neutrino emission that stays consistent with the IceCube all-sky flux and does not exceed ANTARES or KM3NeT limits on the Galactic Ridge.

What carries the argument

Decomposition of diffuse gamma-ray flux into unresolved leptonic pulsar-wind-nebula emission plus hadronic emission from cosmic-ray protons, with the infrared ISRF radial profile varied to quantify gamma-gamma attenuation changes.

What would settle it

Detection of a Galactic Ridge neutrino flux above the current ANTARES or KM3NeT upper limits, or a clear mismatch between the hadronic gamma-ray normalization and the IceCube all-sky neutrino measurement, would falsify the consistency result.

Watch

Extended reading notes

Core claim

We model the LHAASO observation of diffuse TeV--PeV γ rays in the Galactic plane as the sum of unresolved leptonic emission from pulsar wind nebulae and hadronic emission from supernova-injected cosmic-ray (CR) protons. We investigate uncertainties in the radial distribution of the infrared component of the interstellar radiation field (ISRF), using profiles with enhanced photon densities in the inner Galaxy. The alternative ISRF models affect the LHAASO diffuse fit only modestly, as the analysis excludes the Galactic center direction and applies source masks in the Galactic plane. Using the hadronic normalization inferred from the LHAASO fit for various ISRF models, the associated pp neutri

Load-bearing premise

The observed diffuse gamma-ray emission can be cleanly separated into leptonic pulsar-wind-nebula and hadronic cosmic-ray proton contributions once known sources are masked and the Galactic-center direction is excluded.

Editorial extensions

If this is right

  • The same ISRF variations produce noticeable changes in both hadronic and inverse-Compton gamma-ray emission above 10 TeV from sources near the central molecular zone.
  • Future KM3NeT neutrino observations combined with gamma-ray data on individual sources can constrain the inner-Galaxy cosmic-ray population.
  • Modified infrared profiles alter inverse-Compton emission from point sources near the central molecular zone.

Reading between the lines

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

  • The modest impact of ISRF changes implies that gamma-ray data outside the masked inner region can still anchor the overall hadronic normalization.
  • This approach could be extended to test whether the same cosmic-ray population accounts for both diffuse and point-source emission once better inner-Galaxy ISRF maps become available.
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Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

1 major / 1 minor

Summary. The manuscript models the LHAASO observation of diffuse TeV-PeV gamma rays in the Galactic plane as the sum of unresolved leptonic emission from pulsar wind nebulae and hadronic emission from supernova-injected cosmic-ray protons. It investigates uncertainties arising from alternative interstellar radiation field (ISRF) infrared radial profiles with enhanced inner-Galaxy densities, finding only modest effects on the LHAASO diffuse fit due to source masks and exclusion of the Galactic-center direction. Using the resulting hadronic normalizations, the associated pp neutrino emission is reported to remain consistent with the IceCube all-sky measurement, with the Galactic Ridge flux compatible with ANTARES and KM3NeT constraints. The work also examines impacts on inverse-Compton emission from sources near the central molecular zone and discusses prospects for future KM3NeT observations.

Significance. If the decomposition of the diffuse emission holds, the analysis supplies a multi-messenger consistency check linking LHAASO gamma-ray data to neutrino observations while quantifying how ISRF variations propagate to attenuation and emission predictions. The explicit variation of ISRF profiles and the modest impact under the adopted masks represent a concrete step toward addressing inner-Galaxy uncertainties.

major comments (1)
  1. [Modeling of diffuse emission and hadronic normalization extraction (abstract and associated fit description)] The hadronic normalization that sets the predicted neutrino flux is extracted only after subtracting an assumed leptonic contribution from unresolved PWNe, using fixed source masks and excluding the Galactic-center direction. The manuscript varies ISRF models but does not vary the PWNe spatial/spectral template or mask boundaries; any systematic error in this decomposition directly rescales the neutrino prediction and therefore underpins the claimed consistency with IceCube, ANTARES, and KM3NeT data.
minor comments (1)
  1. [Abstract] The abstract states that the neutrino flux 'remains consistent' but does not quote the numerical range of hadronic normalizations obtained across the ISRF models; adding this range would clarify the robustness of the consistency statement.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for the constructive feedback on our manuscript. The major comment raises an important point about the fixed nature of the PWNe template in our decomposition of the diffuse emission. We address this below and outline the revisions we will make.

read point-by-point responses

  1. Referee: [Modeling of diffuse emission and hadronic normalization extraction (abstract and associated fit description)] The hadronic normalization that sets the predicted neutrino flux is extracted only after subtracting an assumed leptonic contribution from unresolved PWNe, using fixed source masks and excluding the Galactic-center direction. The manuscript varies ISRF models but does not vary the PWNe spatial/spectral template or mask boundaries; any systematic error in this decomposition directly rescales the neutrino prediction and therefore underpins the claimed consistency with IceCube, ANTARES, and KM3NeT data.

    Authors: We acknowledge that the hadronic normalization is obtained after subtracting a fixed leptonic contribution from unresolved PWNe, with fixed spatial/spectral templates and mask boundaries. These choices are motivated by established pulsar population models and the need to exclude regions (including the Galactic center) where source confusion and modeling uncertainties are highest; the masks follow those used in the LHAASO diffuse analysis itself. The manuscript's primary goal is to quantify the propagation of ISRF uncertainties through the attenuation and emission modeling while holding the decomposition fixed, so that the modest impact of alternative ISRF profiles can be isolated. Because the same PWNe subtraction is applied uniformly across all ISRF cases, the relative changes in the hadronic component (and thus the neutrino predictions) remain robust. We agree, however, that a dedicated sensitivity study varying the PWNe template would further strengthen the multi-messenger consistency claims. We will therefore add an explicit discussion of this systematic in the revised manuscript, including a qualitative assessment of how plausible variations in the PWNe normalization would rescale the neutrino flux while preserving the reported consistency with IceCube, ANTARES, and KM3NeT data. revision: partial

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity; neutrino consistency is an external check on independent data

full rationale

The paper fits a hadronic normalization to LHAASO gamma-ray data after modeling a leptonic PWNe component, then computes the associated pp neutrino flux via standard pion-decay kinematics and compares the result to separate IceCube, ANTARES, and KM3NeT measurements. This constitutes a consistency test between two distinct observables linked by known particle physics, not a reduction of one result to the other by construction. No self-citation chains, uniqueness theorems, or ansatzes imported from prior author work are invoked as load-bearing steps. The derivation remains self-contained against external benchmarks.

Assumptions & free parameters 2 free parameters · 2 assumptions · 0 invented entities

The central claim rests on two fitted quantities (hadronic normalization and choice among ISRF profiles) plus the domain assumption that the observed diffuse emission is the sum of the two specified components. No new particles or forces are introduced.

free parameters (2)
  • hadronic normalization
    Scale factor for the supernova-injected CR proton component, adjusted to reproduce the LHAASO diffuse gamma-ray spectrum.
  • ISRF infrared radial profile parameters
    Alternative functional forms with enhanced inner-Galaxy photon density, selected to bracket uncertainties.
assumptions (2)
  • domain assumption Diffuse TeV-PeV gamma-ray emission is the sum of unresolved leptonic PWNe emission and hadronic emission from SN-injected CR protons
    Explicitly stated as the modeling framework in the abstract.
  • standard math Gamma-gamma attenuation is dominated by the infrared component of the ISRF
    Standard pair-production kinematics applied to the chosen ISRF models.

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Cite this review

Pith. "Pith review of TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane." pith.science (2026). https://pith.science/paper/FHXFANIH

@misc{pith2026260623476,
  author       = {Pith},
  title        = {Pith review of: TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/FHXFANIH}},
  note         = {Machine review of arXiv:2606.23476}
}
abstract

We model the LHAASO observation of diffuse TeV--PeV $\gamma$ rays in the Galactic plane as the sum of unresolved leptonic emission from pulsar wind nebulae and hadronic emission from supernova-injected cosmic-ray (CR) protons. We investigate uncertainties in the radial distribution of the infrared component of the interstellar radiation field (ISRF), using profiles with enhanced photon densities in the inner Galaxy. We quantify their effects on $\gamma\gamma$ attenuation of the diffuse $\gamma$-ray emission. The alternative ISRF models affect the LHAASO diffuse fit only modestly, as the analysis excludes the Galactic center direction and applies source masks in the Galactic plane. Using the hadronic normalization inferred from the LHAASO fit for various ISRF models, the associated $pp$ neutrino emission remains consistent with the IceCube all-sky measurement, while the flux from the Galactic Ridge region remains compatible with current ANTARES and KM3NeT constraints. Since the modified infrared profiles differ most strongly toward the inner Galaxy, we also examine their impact on inverse-Compton emission from point sources near the central molecular zone. These same models can noticeably modify the hadronic and inverse-Compton $\gamma$-ray emission above $\sim\!10$ TeV from sources in the central region. Future KM3NeT observations, combined with $\gamma$-ray measurements of individual sources, can probe the inner-Galaxy CR population and constrain the radial distribution of the ISRF near the Galactic Center.

Figures

Figures reproduced from arXiv: 2606.23476 by the authors.

Figure 1
Figure 1. Axisymmetric density distribution of (a) molecular H2 and (b) atomic H I in Galactocentric coordinates, obtained by az￾imuthally averaging the 3D interstellar medium reconstruction of Soding et al. ¨ (2025). 2016; Gupta 2025), we consider IR profiles with enhanced photon densities in the inner Galaxy. We evaluate their im￾pact on the γγ optical depth and hence on the fit to the ob￾served diffuse γ-ray spectrum. The … view at source ↗
Figure 2
Figure 2. Galactic pulsar distribution, generated from the observed ATNF pulsar distribution in a 60◦ Galactocentric azimuthal sector centered on the Sun–Galactic-center line. The distribution corre￾sponds to one random realization with an aligned-pulsar fraction of unity. The red dashed line marks ℓ = 15◦ ; the LHAASO region of interest extends anticlockwise to the green dashed line at ℓ = 235◦ . ∂Np/∂t = 0. We solve Eq. 7 n… view at source ↗
Figure 3
Figure 3. Diffuse integrated γ-ray emission at > 10 TeV in the Galactic plane from PWNe for one random realization of the Galaxy. The emission from the white regions are masked out to match the LHAASO analysis (Cao et al. 2023). The upper and lower panels correspond to the LHAASO inner (15◦ < ℓ < 125◦ , |b| < 5 ◦ ) and outer (125◦ < ℓ < 235◦ , |b| < 5 ◦ ) regions. & Manchester 1998), the 737 pulsars selected in the reliable s… view at source ↗
Figures from the paper (4 more)
Figure 4
Figure 4. Figure 4: LHAASO inner-region (15◦ < ℓ < 125◦ , |b| < 5 ◦ ) diffuse γ-ray spectrum for the baseline model. The blue band shows the 3σ confidence interval from the fitted hadronic normalization, while the green band shows the 1σ spread of the unresolved PWN component. The γ-ray f…
Figure 5
Figure 5. Figure 5: Diffuse γ-ray flux for the LHAASO inner (15◦ < ℓ < 125◦ , |b| < 5 ◦ ) and outer (125◦ < ℓ < 235◦ , |b| < 5 ◦ ) region of interest. The shaded region indicates the variation due to uncertainties in the IR model stemming from alternate dust density profiles assumed in […
Figure 6
Figure 6. Figure 6: Left: Neutrino flux obtained in our baseline model (blue line) and other IR distribution profiles (blue shaded), using the best-fit normalizations obtained in [PITH_FULL_IMAGE:figures/full_fig_p007_6.png]
Figure 7
Figure 7. Figure 7: Flux of inverse-Compton γ-ray emission from a steady-state electron spectrum, shown in arbitrary units. The source is placed near the CMZ at R = 0.2 kpc. The left panel shows the relative contributions of the different ISRF photon fields in the baseline model. The righ…

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Pith tools

Reviewed June 26, 2026 · model on record in the stance chip above.