Мақола

Particle acceleration in the polar cap region of an oscillating neutron star

O. ZanottiLaboratory of Applied Mathematics, University of Trento, via Mesiano 77, 38100 Trento, ItalyV. MorozovaInstitute of Nuclear Physics, Ulughbek, 100214 Tashkent, UzbekistanB. AhmedovInstitute of Nuclear Physics, Ulughbek, 100214 Tashkent, Uzbekistan

Astronomy and Astrophysicsjournal2012en

ABI

Аннотация

Aims. We revisit particle acceleration in the polar cap region of a neutron star by taking into account both general relativistic effects and the presence of toroidal oscillations at the star surface. In particular, we address the question of whether toroidal oscillations at the stellar surface can affect the acceleration properties in the polar cap.

Мавзулар

Pulsars and Gravitational Waves Research Astrophysical Phenomena and Observations Dust and Plasma Wave Phenomena

Идентификаторлар

DOI: 10.1051/0004-6361/201118380

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