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Neutron Stars and Black Holes Lecture - 6: Pulsars
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The remarkable story of the Crab Nebula
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Crab Nebula is expanding with a velocity ~ 1500 km per second
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Continuous emission is strongly polarized
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Expanding wisps near the center of the nebula
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Acceleration of the nebula!
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Radio emission from the Crab!
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A great prediction by Shklovskii
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Radio emission from the Crab Nebula is very strongly linearly polarized.
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X-Ray emission from the nebula!
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The great puzzle!
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The great central engine
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An extraordinary conjecture by Pacini!
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Properties of neutron stars
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Oscillating charge will radiate
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A Rotating Magnet will radiate
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Meanwhile in Cambridge!
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Scintillation, or twinkling' of compact radio sources
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Jocelyn Bell
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An unknown scintillating source
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6 August 1967
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Periodic pulsations discovered from the same source on 28 November 1967
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The great discovery announced!
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Micro structure of individual pulses
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Coherence of the radio radiation
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Brightness temperature limit
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Twinkle, twinkle little star
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A video made with a TV camera showed that Baade's star pulsed with a period of 33 ms!
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The great prediction by Franco Pacini
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Neutron Stars as Pulsars
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Average pulse profiles are unique to each pulsar. They are like their 'finger print'.
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Micro structure of individual pulses
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"Nulling" of pulsars
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Neutron stars are powerful dynamos!
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Pulsar electrodynamics
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Magnetosphere of the neutron star
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Light Cylinder
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Radiation from an accelerated charge
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Radiation from a relativistic charge
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Radio radiation from pulsars
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The Polar Cap Model for pulsars
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A hollow cone of radiation
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Pulsed emission from the CRAB Pulsar.
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Pair creation
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Next Lecture - Physical content of the General Theory of Relativity
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Q&A
Description:
Explore the fascinating world of pulsars in this comprehensive lecture from the "Neutron Stars and Black Holes" summer course. Delve into the remarkable story of the Crab Nebula, understanding its expansion, polarized emission, and the puzzling acceleration of its wisps. Discover the groundbreaking work of scientists like Shklovskii and Pacini, who made crucial predictions about neutron stars. Learn about the serendipitous discovery of pulsars by Jocelyn Bell and the subsequent understanding of their nature as rapidly rotating neutron stars. Examine the unique properties of pulsars, including their periodic pulsations, microstructure of individual pulses, and the phenomenon of "nulling." Gain insights into pulsar electrodynamics, magnetosphere, and the light cylinder concept. Explore various models explaining pulsar radiation, including the Polar Cap Model and pair creation processes. This lecture provides a thorough foundation for understanding pulsars, their emission mechanisms, and their significance in astrophysics. Read more

Neutron Stars and Black Holes - Lecture 6: Pulsars and Their Properties

International Centre for Theoretical Sciences
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