Stockholm university

Research project Explorations of the Epoch of Reionization

The Epoch of Reionization is the period when the first stars and galaxies formed, some 13 billion years ago. During this period ionizing light produced in these galaxies escaped into the medium inbetween the galaxies. This resulted in a gradual ionization and heating of the entire Universe.

Radiative transfer simulations
Radiative transfer simulations of the progress of reionization. Blue regions have been ionized, black regions are still neutral. Bright regions have higher density. In this model the image of the left is half ionized and corresponds to redshift 7.5, the image on the left is 70% ionized and corresponds to redshifts 6.5. Credit: K.Dixon/G. Mellema/I. Iliev

Much remains unclear about how events developed during this time and this project is investigating how we can learn more for example from observations of the 21-cm line of neutral hydrogen using for example LOFAR and the future Square Kilometre Array.


The period of is of fundamental importance for understanding our Universe as the oldest stars, the first black holes and the `seeds' of modern day galaxies formed during this era. However, this entire period remains poorly understood. Basic facts such as when it started, when it ended and what were sources of ionizing photons, remain unknown.
The key to a better exploration is the 21cm signal produced by neutral hydrogen in the intergalactic medium. The Low Frequency Array (LOFAR) EoR collaboration of which I am a core member is attempting to detect this signal in a statistical sense. The much more powerful Square Kilometre Array (SKA https://skao.int ), currently under construction, will revolutionize the field by producing actual images of the distribution of the signal.
In this project we will interpret the next LOFAR-EoR data releases using the new inference framework we have been developing. We are also participating in the preparations for SKA and  lastly we will investigate the poorly understood final stages of reionization using world leading computer simulations.

Project members

Project managers

Garrelt Mellema

Head of the department

Department of Astronomy
Picture of Garrelt Mellema

Members

Garrelt Mellema

Head of the department

Department of Astronomy
Picture of Garrelt Mellema

Ivelin Georgiev

PhD student

Department of Astronomy
ivelin-g

Olof Petter Nils Axel Nebrin

Doktorand

Department of Astronomy

Sambit Kumar Giri

Guest researcher

Nordic Institute for Theoretical Physics (NORDITA)
sambit_image