Free Course Image Cosmology Fundamentals: Hubble’s Law, FLRW Models, Inflationand Structure Formation

Free online courseCosmology Fundamentals: Hubble’s Law, FLRW Models, Inflationand Structure Formation

Duration of the online course: 19 hours and 52 minutes

New

Free astronomy course on Hubble’s law, FLRW cosmology, horizons, redshift, inflation, and structure formation with observational and GR foundations.

In this free course, learn about

  • Course Introduction and Hubble’s Law Basics
  • Foundations of Cosmological Models: Newtonian to Relativistic
  • Relativistic Cosmology and Cosmic Components
  • Observational Cosmology: Redshift, Distances, and Counts
  • Inflationary Cosmology
  • Beyond Standard Cosmology: Modified Gravity
  • Structure Formation and Gravitational Instability

Course Description

Cosmology Fundamentals: Hubble’s Law, FLRW Models, Inflation and Structure Formation is a free online astronomy course from Zewail City that builds a clear pathway from the basic language of cosmology to the modern picture of an expanding universe. It begins by sharpening essential tools such as units and dimensions, then moves into the observational foundations that reveal cosmic expansion through Hubble’s law.

You will connect intuitive Newtonian ideas with relativistic cosmology, developing the concepts needed to describe a homogeneous and isotropic universe. Along the way, you will work with the FLRW metric, compare matter- and radiation-dominated eras, and explore illustrative cases such as the Milne universe. Key spacetime concepts are developed through horizons and conformal diagrams, helping you interpret what can and cannot be observed across cosmic history.

The course then focuses on how we measure the universe: redshift, distance measures, angular size, luminosity relations, and number counts, tying theory to observational cosmology. You will also examine the universe’s composition and thermal history, building context for major transitions in the early cosmos.

Finally, the course dives into inflation and its role in explaining large-scale structure, followed by an introduction to modified gravity through f(R) models. The closing sections develop structure formation via gravitational instability, starting with Newtonian treatments and extending to general relativity, giving you a coherent framework for understanding how small perturbations evolve into the cosmic web seen today.

Course content

  • Video class: Introduction to the course 40m
  • Video class: Units, Dimensions 1h15m
  • Exercise: في صيغة قانون هابل للتمدد الكوني، ما هي العلاقة بين سرعة ابتعاد المجرات والمسافة؟
  • Video class: Cont. Hubble’s Law 1h00m
  • Video class: Newtonian Cosmology for a Dust Universe (Continued): Cosmology #4 | ZC OCW 45m
  • Video class: Review of General Relativity 1h13m
  • Video class: FLRW Metric 1h09m
  • Video class: Cont. Relativistic Cosmology 1h13m
  • Video class: Matter vs. Radiation, Milne Universe 54m
  • Video class: Horizons 1h00m
  • Video class: Cont. Conformal Diagrams, Redshifts and Observational Cosmology: Cosmology #10 | ZC OCW 1h11m
  • Video class: Cont. Redshift, Angular Size and Luminosity: Cosmology #11 | ZC OCW 1h06m
  • Video class: Number Counts, Composition and Thermal History of the Universe: Cosmology #12 | ZC OCW 44m
  • Video class: Inflation (Part 1): Cosmology #13 | ZC OCW 51m
  • Video class: Inflation (Part 2): Cosmology #14 | ZC OCW 50m
  • Video class: Inflation (Part 3): Cosmology #15 | ZC OCW 1h04m
  • Video class: f(R) Modified Gravity: Cosmology #16 | ZC OCW 31m
  • Video class: Newtonian Gravitational Instability (Part 1): Cosmology #17 | ZC OCW 1h07m
  • Video class: Newtonian Gravitational Instability (Part 2): Cosmology #18 | ZC OCW 1h08m
  • Video class: Newtonian Gravitational Instability (Part 3): Cosmology #19 | ZC OCW 1h08m
  • Video class: Gravitational Instability in General Relativity: Cosmology #20 | ZC OCW 53m

This free course includes:

19 hours and 52 minutes of online video course

Digital certificate of course completion (Free)

Exercises to train your knowledge

100% free, from content to certificate

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