TÄHT7035 Galaxies and cosmology 8 ECTS
Organised by
Astronomy
Person in charge
Pekka Heinämäki, Roberto de Propris
Planned organizing times
Period(s) I II III IV
2017–2018 X X
Preceding studies
Bachelor level studies in astronomy

Learning outcomes

Student can describe structural, dynamical, chemical and dark matter differences between elliptical, spiral and dwarf galaxies. Student can describe the significance of the mergers, interactions for the evolution of galaxies. Student can explain relation between black holes and nuclei activity. Student can estimate masses of galaxy clusters.

The student can explain Friedmann's cosmological model as the basis for study of the evolution and matter-energy contents of the universe. She/He can use Friedmann's model as an instrument to make a variety of cosmological calculations. He/She can explain the basic structure formation theory of the universe starting from initial quantum fluctuations through different cosmic epochs. Student can explain formation of the cosmic microwave radiation and it's theoretical and observational significance.

Contents

Stellar contents and morphological and dynamical properties of different galaxy types in Hubble sequence. Inter stellar medium, statistics of galaxies and environments. Dark matter halos of galaxies. Dwarf Galaxies and other low luminosity systems. Mergers and Interactions.
Radio Galaxies and Active Galactic Nuclei. Super massive black holes, galaxy clusters. Observational tests and evidence for galaxy formation and evolution.

Robertson-Walker metric, Mattig's equation and cosmological distances, cosmological tests, the physical nature of the dark energy and dark matter, horizons in cosmology, inflation, primordial spectrum of fluctuations, evolution of the matter power spectrum, quantitative measures of the large-scale structure, physics of cosmic thermal background radiation, linear growth of fluctuations and structure formation, spherical top-hat model, non-linear structure formation and cosmological simulations.

Teaching methods

Teaching method Contact Online
Lectures 40 h 0 h
Exercises 16 h 0 h

Homework

Teaching language

English

Modes of study

Option 1
Available for:
  • Degree Programme Students
  • Other Students
  • Doctoral Students
  • Exchange Students
Written exam
  • In English
Participation in classroom work
  • In English

Minimum 50% of exercises and the final written exam.

Evaluation

Numeric 0-5.

Recommended year of study

4. year spring
5. year spring

MSc-degree students, year 1 or 2

Study materials

Lecture notes,
Additional reading:
Baryshev & Teerikorpi:  Fundamental Questions of Practical Cosmology (Springer, Dordrecht 2012)
Byrd, Chernin, Teerikorpi & Valtonen: Paths to Dark Energy - Theory and Observation (De Gruyter, Berlin 2012)
Scott Dodelson: Modern Cosmology (Academic Press, 2003)
Combes, Boisse Mazure, Blanchard: Galaxies and Cosmology (Springer 2004)  
Mo, van den Bosch, White: Galaxy formation and evolution (Cambridge 2010)

Belongs to following study modules

Department of Physics and Astronomy
Department of Physics and Astronomy
2016–2017
Teaching
Archived Teaching Schedule. Please refer to current Teaching Shedule.
Implementation details are unavailable.
Department of Physics and Astronomy
Degree Programme in Physical Sciences
DP in Physics Education Track
Degree Programme in Physical Sciences
DP in Theoretical Physics
Finnish Study Modules