Temporal evolution of isolated pulsars; Age-Tau problem

DOI10.1142/S0218271814500837zbMath1310.83009MaRDI QIDQ5176248

Pinar Kutukcu, Aşkin Ankay

Publication date: 3 March 2015

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

zbMATH Keywords

magneto-dipole radiationsupernova remnantsevolution of pulsarsisolated neutron stars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Radiative transfer in astronomy and astrophysics (85A25)

Cites Work

• 1E 1207.4–5209-LIKE RADIO-QUIET NEUTRON STARS
• THE STRONG MAGNETIC FIELD DECAY AND EVOLUTION OF RADIO PULSARS ON THE P–Ṗ DIAGRAM
• TESTING THE FALL-BACK DISK MODEL FOR RADIO PULSARS USING NEW DATA
• POSSIBLE EVOLUTION OF DIM RADIO-QUIET NEUTRON STAR 1E 1207.4-5209 BASED ON A B-DECAY MODEL
• MAGNETOSPHERIC PARTICLE ACCELERATION AND X-RAY EMISSION OF PULSARS
• DEPENDENCE OF THE X-RAY LUMINOSITY AND PULSAR WIND NEBULA ON DIFFERENT PARAMETERS OF PULSARS AND THE EVOLUTIONARY EFFECTS
• INFLUENCES OF PHYSICAL PARAMETERS OF NEUTRON STARS ON THE IR POSITIONS ON THE P-Ṗ DIAGRAM

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