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- W4312866986 abstract "AbstractIn the previous chapter, we analyzed the cosmic ray (CR) production at the terminal shocks of starburst superwinds. We found that the maximum energies are (sim 10^{17}) eV, limited mainly by the mass loading factor of the wind and the magnetic field strength. The large amount of energy injected by the powerful star formation, along with their metal-rich environments, make starburst galaxies favorable places for the production of ultra-high energy cosmic rays (UHECRs). This idea is particularly motivated by the increasing mass composition for CRs at the highest energies observed by the Pierre Auger Observatory (Auger), along with the correlation between arrival directions and the positions of these galaxies [1, 37, 38]. The superwind is an excellent region in starbursts where particles with large Larmor radii and heavy composition can be confined and accelerated without suffering photo-disintegration [7]. Observationally, the presence of relativistic particles in starburst galaxies has been proved by the gamma emission detected from nearby objects [2,3,4,5, 30]." @default.
- W4312866986 created "2023-01-05" @default.
- W4312866986 creator A5048415692 @default.
- W4312866986 date "2022-01-01" @default.
- W4312866986 modified "2023-09-27" @default.
- W4312866986 title "Particle Acceleration in the Superwind of Starburst Galaxies. Part II: Small-Scale Processes" @default.
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- W4312866986 doi "https://doi.org/10.1007/978-3-031-10306-3_5" @default.
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