Astrophysics

An in-depth exploration of the physical processes governing celestial objects and phenomena throughout the universe. From stellar structure and evolution to compact objects, gravitational waves, and cosmological observations.

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New to Astrophysics?

Check out our beginner-friendly course designed for undergraduate students! Learn about stars, galaxies, black holes, and cosmology with accessible explanations, real-world examples, and links to advanced topics when you're ready.

Start with Astrophysics for Beginners →

Advanced Course Overview

This comprehensive astrophysics course covers the fundamental physics of stars, galaxies, compact objects, and large-scale structure. We explore stellar evolution, nuclear processes, gravitational dynamics, and observational techniques that have revolutionized our understanding of the cosmos.

8 Parts

Comprehensive coverage from stellar physics to cosmological observations

48+ Chapters

Detailed topics with derivations and observational data

Video Lectures

Curated lecture series from leading institutions

Course Structure

Part I: Stellar Structure and Evolution

Equations of stellar structure, energy generation via nuclear fusion, stellar evolution from main sequence to compact remnants. Hertzsprung-Russell diagram, stellar populations, and nucleosynthesis.

Stellar StructureNuclear FusionHR Diagram

Part II: Compact Objects

White dwarfs, neutron stars, and black holes. Degeneracy pressure, Chandrasekhar limit, neutron star equation of state, pulsar physics, accretion disks, and X-ray binaries.

White DwarfsNeutron StarsPulsars

Part III: Galactic Dynamics

Gravitational potentials, orbital dynamics, disk stability, rotation curves, dark matter distribution, spiral structure, and the Milky Way's structure and kinematics.

Rotation CurvesDark MatterSpiral Structure

Part IV: High-Energy Astrophysics

Particle acceleration, synchrotron radiation, Compton scattering, jets and blazars, gamma-ray bursts, cosmic rays, and multi-messenger astrophysics.

Synchrotron RadiationCosmic RaysGRBs

Part V: Gravitational Waves

Generation and detection of gravitational waves, LIGO/Virgo observations, binary inspiral and merger, waveform analysis, multi-messenger astronomy, and future detectors.

LIGO DetectionsBinary MergersMulti-Messenger

Part VI: Extragalactic Astronomy

Galaxy classification and evolution, active galactic nuclei, quasars, supermassive black holes, galaxy clusters, large-scale structure, and the cosmic web.

AGN & QuasarsGalaxy ClustersLarge-Scale Structure

Part VII: Observational Techniques

Telescopes and instruments across the electromagnetic spectrum, photometry, spectroscopy, interferometry, adaptive optics, space missions, and data analysis methods.

SpectroscopyInterferometrySpace Missions

Part VIII: Planetary Systems and Exoplanets

Solar system formation, planet formation and migration, exoplanet detection methods, habitability, atmospheres, and the search for life beyond Earth.

Exoplanet DetectionPlanet FormationHabitability

Featured Lecture Series

Prerequisites

Recommended Background:

Mathematical Tools:

  • • Vector calculus and differential equations
  • • Basic numerical methods
  • • Statistical analysis
  • • Fourier analysis
  • • Some tensor calculus (for GR topics)

Key Topics Covered

Fundamental Physics:

  • • Radiative transfer and opacity
  • • Nuclear reaction networks
  • • Equation of state for extreme matter
  • • Magnetic field dynamics
  • • Plasma physics in astrophysical contexts

Observational:

  • • Multi-wavelength astronomy
  • • Gravitational wave detections
  • • Neutrino astronomy
  • • Time-domain astronomy
  • • Survey science and big data