On Acceleration of Highest-energy Cosmic Rays in a Novel Scenario of Magnetar Transients
Transient phenomena in magnetars have been considered as possible acceleration sites of ultra-high-energy cosmic rays (CRs), whose energy reaches ∼200 EeV, such as the Amaterasu particle.
Jiro Shimoda, Tomoki Wada
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Generation of intense magnetic wakes by relativistic laser pulses in plasma. [PDF]
Lamač M +3 more
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Magnetorotational instability in dense electron-positron-ion plasmas. [PDF]
Usman S, Mushtaq A.
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Measurement of the scalar curvature of high-power lasers. [PDF]
Toma A, Postavaru O.
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2 pages, LaTeX (basi.sty), poster presented in the annual meeting of ASI (2003)
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Magnetar formation through a convective dynamo in protoneutron stars. [PDF]
Raynaud R +3 more
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A connection between proto-neutron-star Tayler-Spruit dynamos and low-field magnetars. [PDF]
Igoshev A +5 more
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Repeating fast radio bursts from collapses of the crust of a strange star. [PDF]
Geng J, Li B, Huang Y.
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A highly magnetized long-period radio transient exhibiting unusual emission features. [PDF]
Men Y +4 more
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Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster. [PDF]
Pearlman AB +28 more
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