Computes neutrino template maps from the Galactic Plane including star cluster emission, finding the cluster contribution may be non-negligible and consistent with IceCube best-fit templates.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 3years
2026 3representative citing papers
A time-dependent model of stellar evolution and wind shocks shows collective winds of massive star clusters dominate the PeV knee and explain the common spectral break in protons and helium.
SAETASS solves the time-dependent astroparticle transport equation in spherical symmetry using a conservative finite-volume, operator-splitting framework, validated against analytical solutions and applied to cosmic-ray proton transport in a stellar-wind bubble.
citing papers explorer
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Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays
Computes neutrino template maps from the Galactic Plane including star cluster emission, finding the cluster contribution may be non-negligible and consistent with IceCube best-fit templates.
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Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays
A time-dependent model of stellar evolution and wind shocks shows collective winds of massive star clusters dominate the PeV knee and explain the common spectral break in protons and helium.
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SAETASS: Solver for Astroparticle Equation of Transport Analysis in Spherical Symmetry
SAETASS solves the time-dependent astroparticle transport equation in spherical symmetry using a conservative finite-volume, operator-splitting framework, validated against analytical solutions and applied to cosmic-ray proton transport in a stellar-wind bubble.