Cosmos

Structure and evolution of the Cosmos

Explores the vast complexities of the cosmos, focusing on the formation and interaction of galaxies, the early universe, dark matter, and cosmic expansion, contributing to groundbreaking discoveries like the accelerating expansion of the universe, a phenomenon pivotal to our understanding of cosmic evolution.

About

On the largest and most distant scales, astrophysicists and cosmologists at RSAA study many types of distant galaxies, investigate the nature of the early universe, and measure the expansion of space itself. Areas of study in these fields include:

  • understanding how galaxies form and interact with each other and their environments
  • observing how interactions between galaxies affect their development
  • the effects of internal processes, such as star formation and central supermassive black holes, on the growth of a galaxy
  • the role and nature of dark matter in the formation of structure in the universe
  • measuring the rate of acceleration of the expansion of the universe and understanding the implications for cosmological models
  • modelling and observing enigmatic phenomena such as gamma ray bursts, supernovae and other transients to understand the physical processes that cause them.

Research led by cosmologists at ANU led to the discovery that the Universe is expanding at an ever-increasing rate; work for which the 2011 Nobel Prize in Physics was awarded. RSAA astronomers continue to investigate what this means for theoretical models of the Universe, to understand the role of dark energy or the cosmological constant that drives this accelearation. They are also improving measurements of distance to the exploding stars, or supernovae, that are used as beacons in mapping the expansion rate to refine the results that constrain these models. One of the major goals for the SkyMapper Telescope's Southern Sky Survey is to discover tens of thousands of new supernova occurring in distant galaxies. This will significantly increase the sample of observed events and enable astronomers to make detailed follow-up observations to help improve understanding of the physical processes that occur during these stellar explosions.

Projects

In this project you will use a new cosmic ray propagation code, CRIPTIC, to model the injection, transport, and final annihilation of positrons in the interstellar medium of the inner Galaxy.

Student intake

Open for Honours, PhD students

People

We aim to build a novel framework to study supermassive black holes via their unique gravitational wave signatures providing a multi-messenger tool to constrain galaxy formation in the early universe.

Student intake

Open for Honours, Master, PhD students

People

  • Dr Lilli (Ling) Sun

In this project you will use some combination of theoretical population synthesis calculations and/or analysis of public data from the Fermi telescope to examine the question: what is the real origin of the Galactic Centre Gamma-Ray Excess?

Student intake

Open for Honours, PhD students

People

Members

Faculty

Christoph Federrath

Associate Director HDR
Former ARC Future and Stromlo Fellow
Research School of Astronomy and Astrophysics

Academic

Christoph Federrath

Associate Director HDR
Former ARC Future and Stromlo Fellow
Research School of Astronomy and Astrophysics

News

A PhD student at the ANU Research School of Astronomy and Astrophysics, Catherine Farage, is studying massive ellipticals in galaxy clusters, to look for clues that could help to explain the mechanisms behind the formation of large galaxies.

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A team of Australian astronomers is looking for the trigger of a cosmic explosion discovered by Dutch astronomer Tycho Brahe in 1572. It is still unclear why events like this, which are refered to as supernovae, occur. 

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Nobel winner Professor Brian Schmidt's press conference at Parliament House

Professor Brian Schmidt from the Research School of Astronomy and Astrophysics has won the 2011 Nobel Prize for Physics.

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Events

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Tuesday, 15 Jul 2025, 11am

Resolving the subgrid physics of galactic winds.

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Tuesday, 29 Jul 2025, 11am

In pursuit of realistic star formation histories from SED fitting.

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