Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/8262
Title: Between the Cosmic-Ray “Knee” and the “Ankle”: Contribution from Star Clusters
Authors: Bhadra, Sourav
Thoudam, Satyendra
Nath, Biman
Sharma, Prateek
Keywords: Cosmic rays
Particle astrophysics
High energy astrophysics
Galactic cosmic rays
Young star clusters
Issue Date: 1-Feb-2024
Publisher: American Astronomical Society
Citation: The Astrophysical Journal, 2024, Vol.961, p215
Abstract: We show that massive, young star clusters may be possible candidates that can accelerate Galactic cosmic rays (CRs) in the range of 107–109 GeV (between the “knee” and “ankle”). Various plausible scenarios, such as acceleration at the wind termination shock and supernova shocks inside these young star clusters, have been proposed, since it is difficult to accelerate particles up to the 107–109 GeV range in the standard paradigm of CR acceleration in supernova remnants. We consider a model for the production of different nuclei in CRs from massive stellar winds using the observed distribution of young star clusters in the Galactic plane. We present a detailed calculation of CR transport in the Galaxy, taking into account the effect of diffusion, interaction losses during propagation, and particle reacceleration by old supernova remnants to determine the all-particle CR spectrum. Using the maximum energy estimate from the Hillas criterion, we argue that a young, massive star cluster can accelerate protons up to a few tens of PeV. Upon comparison with the observed data, our model requires a CR source spectrum with an exponential cutoff of 5 × 107Z GeV (50 Z PeV) from these clusters, together with a CR injection fraction of ∼5% of the wind kinetic energy. We discuss the possibility of achieving these requirements in star clusters, as well as the associated uncertainties, in the context of considering star clusters as the natural accelerator of the “second component” of Galactic CRs.
Description: Open Access
URI: http://hdl.handle.net/2289/8262
Alternative Location: https://ui.adsabs.harvard.edu/abs/2024ApJ...961..215B/abstract
https://arxiv.org/abs/2312.06992
https://doi.org/10.3847/1538-4357/ad1605
Copyright: 2024, The Author(s)
Appears in Collections:Research Papers (A&A)

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