Cosmology 0800-KOSMO
physical cosmology:
* hot big bang model (Friedmann–Lemaître–Robertson–Walker model of spacetime as a family of simplified spacetimes that satisfy the Einstein equation);
* Hubble-Lemaitre expansion (Lemaître 1927) a normalised time derivative of the scale factor and as a key observation, cosmic microwave background (McKellar 1941 + Adams 1941) as a key observation, primordial nucleosynthesis as a key observation);
* derivation of the Friedmann equations;
* the Einstein static solution as an exact solution satisfying mainstream views of the observations of the 1910s;
* the Einstein-de Sitter model as an exact solution with no initial singularity;
* derivation of scale-factor--time--redshift relations;
* geometrically meaningful derivation of the comoving arc length (areal radius), angular diameter distance, and luminosity distance;
* cosmological paradoxes;
* LambdaCDM model versus general-relativistic models and their observational foundations;
* galaxy formation
Total student workload
Learning outcomes - knowledge
Learning outcomes - skills
Learning outcomes - social competencies
Teaching methods
Type of course
Prerequisites
Course coordinators
Assessment criteria
The exam consists of questions randomly chosen from an N-dimensional parameter space of questions where N is much greater than 10. Each student is given rapid feedback and may ask for new questions in order to improve his/her score without limit, apart from the total time available. The expected examination time is about 2-3 hours, but students may continue to a maximum of 6.5 hours. K_W01, K_W03, K_W05, K_W08, K_U04, K_U07, K_K01
Grades are rounded using the "round half to even" algorithm.
Additional information
Additional information (registration calendar, class conductors, localization and schedules of classes), might be available in the USOSweb system: