Neutron Stars and Black Holes - Recycled Pulsars - Lecture 10

Neutron Stars and Black Holes - Recycled Pulsars - Lecture 10

International Centre for Theoretical Sciences via YouTube Direct link

The HULSE-TAYLOR Pulsar

4 of 31

4 of 31

The HULSE-TAYLOR Pulsar

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Classroom Contents

Neutron Stars and Black Holes - Recycled Pulsars - Lecture 10

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  1. 1 Time: AM
  2. 2 Neutron Stars and Black Holes Lecture - 10: Recycled Pulsars
  3. 3 Recycled Pulsars
  4. 4 The HULSE-TAYLOR Pulsar
  5. 5 Hulse-Taylor Binary Pulsar
  6. 6 Massive Binary
  7. 7 Spinning up a neutron star
  8. 8 What will be the period of rotation of the first-born neutron star after the spin up phase is over?
  9. 9 The Equilibrium Period
  10. 10 Alfven Radius
  11. 11 Accretion disk
  12. 12 Question: For a given magnetic field, can we spin up a neutron star to arbitrarily small period?
  13. 13 Eddington Luminosity Limit
  14. 14 Eddington Limit for the Accretion Rate
  15. 15 The Minimum Equilibrium Period
  16. 16 The Hulse-Taylor Binary Pulsar
  17. 17 Any viable theory of field evolution must explain the following questions
  18. 18 Origin of magnetic field of neutron stars
  19. 19 Field decay in Neutron Stars
  20. 20 Superfluid core
  21. 21 Type II superconductivity in the core
  22. 22 Type II proton superconductivity in the core
  23. 23 Feynman "Vortices" to the rescue!
  24. 24 The inter-pinning of the fluxoids and vortices
  25. 25 An important prediction
  26. 26 Recycled Pulsars
  27. 27 What determines the degree of field decay?
  28. 28 A Possible scenario
  29. 29 The population of Recycled Pulsars
  30. 30 Next Lecture - Millisecond Pulsars
  31. 31 Q&A

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