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
International Centre for Theoretical Sciences via YouTube
Overview
Syllabus
Time: AM
Neutron Stars and Black Holes Lecture - 5: Radiation from Relativistic Particles
Radiation from Relativistic Particles
Maxwell's Equations
Dipole approximation
Specific Intensity Iv
Energy Flux and Intensity of Radiation
Intensity of Radiation
LARMOR's Formula
Angular distribution
Dipole approximation
Polarization of the Radiation from a nonrelativistic charge
Theorem
Quadrupole and Magnetic Dipole Radiation
Gravitational radiation
Spectral Resolution
Radiation from relativistic particles
Angular Distribution - Relativistic case
PULSED radiation from relativistic particles
Synchrotron Radiation
Synchrotron Radiation - Spectrum
A charge gyrating in a magnetic field
Radiation from an ensemble of particles
Radio spectrum of a supernova remnant
Synchrotron Lifetime
Synchrotron self-absorption
Landau levels in a magnetic field
Synchrotron self absorption in compact SUPERLUMINAL SOURCE
Pulsars, Supernova Remnants and Radio Galaxies
Next Lecture - Pulsars
Q&A
Taught by
International Centre for Theoretical Sciences
