f(Q) Theory and its Application in Gravitation Course
This course provides a comprehensive introduction to f(Q) theory in symmetric teleparallel gravity, focusing on its cosmological applications. Participants will learn to derive key equations, model dark energy, analyze universe evolution, and effectively communicate findings.

from 4 to 360h flexible workload
valid certificate in your country
What will I learn?
This concise f(Q) Theory and Its Application in Gravitation Course equips you with practical tools to handle symmetric teleparallel gravity, starting from defining the nonmetricity scalar, deriving f(Q) field equations, and modified Friedmann relations. You will examine simple late-time acceleration models, grasp semi-analytical methods for H(a) and w_eff(a), and receive clear guidance on presenting results, plots, and citations in a polished report.
Elevify advantages
Develop skills
- Master f(Q) gravity basics: nonmetricity, action, and field equations for cosmology.
- Derive modified Friedmann equations and extract H(a) and w_eff(a) fast and cleanly.
- Build and test simple f(Q) dark-energy models against ΛCDM and stability limits.
- Use semi-analytical tools to sketch background evolution and identify attractors.
- Present f(Q) results clearly with focused plots, tables, and concise citations.
Suggested summary
Before starting, you can change the chapters and workload. Choose which chapter to start with. Add or remove chapters. Increase or decrease the course workload.What our students say
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