THE STRONG MAGNETIC FIELD DECAY AND EVOLUTION OF RADIO PULSARS ON THE P–Ṗ DIAGRAM

DOI10.1142/S0218271804005122zbMath1064.85504arXivastro-ph/0408477OpenAlexW3104644122MaRDI QIDQ4662696

Sevinç O. Tagieva, Aşkin Ankay, Oktay H. Guseinov

Publication date: 30 March 2005

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0408477

zbMATH Keywords

pulsarmagnetic fieldevolution

Mathematics Subject Classification ID

Electromagnetic fields in general relativity and gravitational theory (83C50) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

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