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Time: AM
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Neutron Stars and Black Holes Lecture - 10: Recycled Pulsars
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Recycled Pulsars
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The HULSE-TAYLOR Pulsar
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Hulse-Taylor Binary Pulsar
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Massive Binary
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Spinning up a neutron star
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What will be the period of rotation of the first-born neutron star after the spin up phase is over?
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The Equilibrium Period
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Alfven Radius
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Accretion disk
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Question: For a given magnetic field, can we spin up a neutron star to arbitrarily small period?
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Eddington Luminosity Limit
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Eddington Limit for the Accretion Rate
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The Minimum Equilibrium Period
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The Hulse-Taylor Binary Pulsar
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Any viable theory of field evolution must explain the following questions
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Origin of magnetic field of neutron stars
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Field decay in Neutron Stars
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Superfluid core
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Type II superconductivity in the core
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Type II proton superconductivity in the core
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Feynman "Vortices" to the rescue!
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The inter-pinning of the fluxoids and vortices
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An important prediction
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Recycled Pulsars
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What determines the degree of field decay?
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A Possible scenario
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The population of Recycled Pulsars
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Next Lecture - Millisecond Pulsars
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Q&A
Description:
Explore the fascinating world of recycled pulsars in this comprehensive lecture from the "Neutron Stars and Black Holes" summer course. Delve into the Hulse-Taylor binary pulsar system, understand the process of spinning up neutron stars, and examine the concept of equilibrium period. Learn about the Alfven radius, accretion disks, and the Eddington luminosity limit. Investigate the origin and evolution of magnetic fields in neutron stars, including field decay mechanisms and the role of superfluidity and superconductivity in the core. Discover the importance of Feynman vortices and their interaction with magnetic flux tubes. Gain insights into the factors determining field decay in recycled pulsars and explore their population distribution. The lecture concludes with a preview of millisecond pulsars and includes a Q&A session, providing a comprehensive understanding of these fascinating astronomical objects.

Neutron Stars and Black Holes - Recycled Pulsars - Lecture 10

International Centre for Theoretical Sciences
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