f(Q) Theory and its Application in Gravitation Course
Gain expertise in f(Q) gravity, progressing from core concepts like nonmetricity and field equations to cosmological applications including altered Friedmann dynamics and benchmarks against ΛCDM. Construct straightforward f(Q) models to account for late-time cosmic acceleration, analyse background evolution using semi-analytic approaches, and interpret observational datasets with precise plots, tables, and citations for impactful presentations.

flexible workload of 4 to 360h
valid certificate in your country
What will I learn?
This focused course on f(Q) theory and its role in gravitation equips you with essential tools for symmetric teleparallel gravity, covering nonmetricity scalar definition, f(Q) field equations derivation, and adapted Friedmann equations. Participants will study basic late-universe acceleration scenarios, apply semi-analytic techniques for Hubble parameter H(a) and effective equation of state w_eff(a), and receive tips for effectively showcasing findings, graphs, and references in professional reports.
Elevify advantages
Develop skills
- Master fundamentals of f(Q) gravity: nonmetricity concepts, action principles, and cosmological field equations.
- Derive adapted Friedmann equations efficiently to obtain H(a) and w_eff(a) behaviours.
- Develop and validate basic f(Q) dark energy models relative to ΛCDM and stability criteria.
- Apply semi-analytic methods to model cosmic background evolution and detect attractor solutions.
- Communicate f(Q) findings effectively using targeted plots, tables, and succinct references.
Suggested summary
Before starting, you can change the chapters and the 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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