A TOY MODEL FOR SCALARS IN TRANSIENT MAGNETIC FIELDS

DOI10.1142/S0217732311035808zbMath1274.85006OpenAlexW2084021897MaRDI QIDQ2861204

Marina-Aura Dariescu, Ciprian Dariescu

Publication date: 12 November 2013

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732311035808

zbMATH Keywords

Mathieu's equationneutron starscoupled modes and recurrent methodsKlein-Gordon and Maxwell equations

Mathematics Subject Classification ID

Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Galactic and stellar structure (85A15) Electromagnetic theory (general) (78A25) Special ordinary differential equations (Mathieu, Hill, Bessel, etc.) (34B30)

Related Items (4)

Coherent planar symmetric spacetimes generated by progressive waves of Nambu-Goldstone bosons ⋮ Approximative analytic study of fermions in magnetar's crust; ultra-relativistic plane waves, Heun and Mathieu solutions and beyond ⋮ FERMIONS IN MAGNETAR'S CRUST IN TERMS OF HEUN DOUBLE CONFLUENT FUNCTIONS ⋮ ON THE MATHIEU EQUATION DESCRIBING ULTRA-RELATIVISTIC FERMIONS EVOLVING IN A TIME-HARMONIC ELECTRIC FIELD PARALLEL TO A STATIC MAGNETIC INDUCTION

Cites Work

• Unnamed Item
• Hall cascades versus instabilities in neutron star magnetic fields
• Magnetic field dissipation in neutron star crusts: from magnetars to isolated neutron stars
• Stable magnetic fields in stellar interiors
• Evolution of the magnetic field in magnetars

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