Neutron Stars and Black Holes Lecture - 5: Radiation from Relativistic Particles
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Radiation from Relativistic Particles
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Maxwell's Equations
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Dipole approximation
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Specific Intensity Iv
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Energy Flux and Intensity of Radiation
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Intensity of Radiation
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LARMOR's Formula
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Angular distribution
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Dipole approximation
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Polarization of the Radiation from a nonrelativistic charge
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Theorem
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Quadrupole and Magnetic Dipole Radiation
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Gravitational radiation
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Spectral Resolution
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Radiation from relativistic particles
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Angular Distribution - Relativistic case
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PULSED radiation from relativistic particles
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Synchrotron Radiation
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Synchrotron Radiation - Spectrum
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A charge gyrating in a magnetic field
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Radiation from an ensemble of particles
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Radio spectrum of a supernova remnant
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Synchrotron Lifetime
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Synchrotron self-absorption
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Landau levels in a magnetic field
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Synchrotron self absorption in compact SUPERLUMINAL SOURCE
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Pulsars, Supernova Remnants and Radio Galaxies
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Next Lecture - Pulsars
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Q&A
Description:
Explore the fifth lecture in a comprehensive series on neutron stars and black holes, focusing on radiation from relativistic particles. Delve into Maxwell's equations, dipole approximation, and specific intensity. Examine energy flux, Larmor's formula, and angular distribution of radiation. Investigate polarization, quadrupole and magnetic dipole radiation, and gravitational radiation. Learn about radiation from relativistic particles, synchrotron radiation, and its spectrum. Discover the physics behind pulsars, supernova remnants, and radio galaxies. Gain insights into synchrotron lifetime, self-absorption, and Landau levels in magnetic fields. Conclude with a brief introduction to the next lecture on pulsars and participate in a Q&A session.
Neutron Stars and Black Holes - Radiation from Relativistic Particles - Lecture 5