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Large Scale Structure and Galaxy Formation

Vak
2024-2025

Admission requirements

Familiarity with basic concepts of cosmology is assumed. The student is assumed to have basic knowledge of the thermal history of the universe, recombination, the cosmic microwave background, cosmic distances, horizons, and to be able to work with the Friedmann equation. In terms of the Leiden curriculum, the Astronomy master's course Origin and Evolution of the Universe provides the ideal preparation.

Description

How galaxies and the large-scale structures in which they are embedded form is a fundamental question in extra-galactic astronomy. It is an area that has seen tremendous progress, but is still constantly challenged by ever-improving observational data. This course introduces you to this fascinating subject and the underlying physics, starting from how small density perturbations grow into dark matter haloes, to how baryons cool and form the galaxy population we observe today.

Physical concepts are derived from basic principles where possible. The emphasis is on intuitive rather than mathematically rigorous derivations.

Topics that will be covered include:

  • Statistical cosmological principle

  • Linear growth of density perturbations

  • Free streaming

  • Jeans smoothing

  • Radiation drag

  • The linear growth of potential fluctuations

  • The linear growth of peculiar velocities

  • Transfer functions and the matter power spectrum

  • Correlation functions

  • Redshift space distortions

  • The cosmic web

  • Non-linear spherical collapse

  • Scaling laws and virial relations

  • Halo mass functions and Press-Schechter theory

  • Biasing

  • Halo density profiles, shapes, and spins

  • The halo model

  • Semi-empirical models for galaxy clustering

  • Radiative cooling

  • Gas accretion

  • Angular momentum and galaxy sizes

  • Stellar and AGN feedback

  • Self-regulated galaxy formation

  • The epoch of reionization

  • The Gunn-Peterson effect and quasar absorbers

  • The thermal history of the intergalactic medium

Course objectives

Upon completion of this course you will be able to explain how (we think that) large-scale structures and galaxies form and evolve and you will be able to carry out calculations of the formation of structures in the universe.

Upon completion of the course you will be able to:

  • Understand the concepts covered in the course, including those listed above

  • Be able to explain the current picture of the origin and evolution of large-scale structure and galaxies

  • Make quantitative but approximate models for the evolution of large-scale structure, dark matter haloes, the circumgalactic medium, galaxies and the intergalactic medium

  • Understand the main limitations of the models and know some of the unanswered questions

  • Be able to read the literature and follow talks on the topics covered

Timetable

See Astronomy master schedule

In MyTimetable, you can find all course and programme schedules, allowing you to create your personal timetable. Activities for which you have enrolled via MyStudyMap will automatically appear in your timetable.

Additionally, you can easily link MyTimetable to a calendar app on your phone, and schedule changes will be automatically updated in your calendar. You can also choose to receive email notifications about schedule changes. You can enable notifications in Settings after logging in.

Questions? Watch the video, read the instructions, or contact the ISSC helpdesk.

Note: Joint Degree students from Leiden/Delft need to combine information from both the Leiden and Delft MyTimetables to see a complete schedule. This video explains how to do it.

Mode of instruction

  • Lectures

  • Exercise classes

Assessment method

  • Written exam (75%)

  • Four homework assignments: 25% (if higher than the result of the written exam)

Reading list

Lecture notes

Registration

As a student, you are responsible for enrolling on time through MyStudyMap.

In this short video, you can see step-by-step how to enrol for courses in MyStudyMap.
Extensive information about the operation of MyStudyMap can be found here.

There are two enrolment periods per year:

  • Enrolment for the fall opens in July

  • Enrolment for the spring opens in December

See this page for more information about deadlines and enrolling for courses and exams.

Note:

  • It is mandatory to enrol for all activities of a course that you are going to follow.

  • Your enrolment is only complete when you submit your course planning in the ‘Ready for enrolment’ tab by clicking ‘Send’.

  • Not being enrolled for an exam/resit means that you are not allowed to participate in the exam/resit.

Contact

Lecturer: Prof.dr. J. Schaye

Remarks

Software
Starting from the 2024/2025 academic year, the Faculty of Science will use the software distribution platform Academic Software. Through this platform, you can access the software needed for specific courses in your studies. For some software, your laptop must meet certain system requirements, which will be specified with the software. It is important to install the software before the start of the course. More information about the laptop requirements can be found on the student website.