Pith. sign in

REVIEW 5 cited by

Parameterization of Gamma, e^+/- and Neutrino Spectra Produced by p-p Interaction in Astronomical Environment

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0605581 v3 pith:C6HF2OIE submitted 2006-05-23 astro-ph

Tuneyoshi Kamae , Niklas Karlsson , Tsunefumi Mizuno , Toshinori Abe , Tatsumi Koi This is my paper · ORCID
classification astro-ph
keywords interactionformulaespectraastronomicalfeynmangammanubarscaling
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present the yield and spectra of stable secondary particles (gamma, e^+/-, nu_e, nubar_e, nu_mu, and nubar_mu) of p-p interaction in parameterized formulae to facilitate calculations involving them in astronomical environments. The formulae are derived on the up-to-date p-p interaction model by [Kamae05] which incorporates the logarithmically rising inelastic cross-section, the diffraction dissociation process, and the Feynman scaling violation. To improve fidelity to experimental data in lower energies, two baryon resonance contributions have been added: one representing Delta(1232) and the other multiple resonances around 1600MeV/c^2. The parametrized formulae predict that all secondary particle spectra be harder by about 0.05 in power-law indices than that of the incident proton and their inclusive cross-sections be larger than those predicted by p-p interaction models based on the Feynman scaling.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Galactic Neutrino Sky: Predictions from Gamma-ray Source Populations

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    A template of resolved and unresolved gamma-ray sources, added to an unmodified diffuse model, reproduces the shape and spectrum of IceCube's inner-Galaxy neutrino excess.

  2. Galactic Center Neutrinos from Cosmic Ray-Dark Matter Interactions

    hep-ph 2026-07 conditional novelty 6.0 of 10

    ANTARES Galactic Ridge neutrino observations constrain DM-nucleon elastic scattering cross sections down to keV-scale DM masses via cosmic ray–dark matter deep inelastic scattering.

  3. Relativistic ions with power-law spectra explain radio phoenixes

    astro-ph.HE 2025-03 unverdicted novelty 5.0 of 10

    Relativistic ions with power-law spectra produce secondary e± that explain the curved radio spectra of phoenixes in galaxy clusters, fitting data better than aged-electron models with three parameters.

  4. Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation

    hep-ph 2026-06 unverdicted novelty 4.0 of 10

    Monte Carlo simulations of nuclear cascades in NGC 1068 demonstrate that injected nuclear composition imprints on neutrino and gamma-ray spectra, supported by a re-analysis of archival COMPTEL observations.

  5. IceCube Results and Perspective for Neutrinos from LHAASO Sources

    astro-ph.HE 2024-04 unverdicted novelty 2.0 of 10

    Reviews IceCube neutrino results, models Galactic plane flux from cosmic ray interactions with the interstellar medium, and discusses prospects for identifying PeVatrons via LHAASO sources.

Pith tools