Fabian Schneider To Lead Stellar Evolution Theory In HITS


Fabian Schneider leads the new research group “Stellar Evolution Theory” (SET) at the Heidelberg Institute for Theoretical Studies (HITS). The astrophysicist explores the turbulent life of massive binary stars and their explosive deaths in supernovae. He was awarded an ERC Starting Grant of about € 1.5 million by the European Research Council (ERC). He will use the funds to establish his own junior research group at HITS.

Stars are the basic building blocks of the visible Universe. Astrophysicists are particularly interested in massive stars. They are cosmic powerhouses, exploding in spectacular supernovae and leaving behind some of the most exotic forms of matter: neutron stars and black holes. Mergers of neutron stars and black holes are now routinely observed thanks to gravitational wave observatories. But there are still a lot of questions that remain unanswered.

.Since 1 January 2021, Fabian has been the leader of Stellar Evolution Theory

at the Heidelberg Institute for Theoretical Studies (HITS). He had successfully applied for an ERC Starting Grant from the European Research Council (ERC), and he is now establishing his own junior research group. HITS now consists of 13 research groups, four of them in the field of astronomy Fabian Schneider studied physics at the University of Bonn and completed his Ph.D. in astrophysics at the Argelander-Institute for Astronomy in 2015. He then joined the Department of Physics of the University of Oxford as a “Hintze Fellow”, where he did research on massive stars, their magnetic fields and supernovae.

The new SET group focuses on massive binary stars, which make up the majority of massive stars. During their lifetime, they can reach a stage where their outer layers are transferred onto their companion. The mass transfer profoundly changes the evolution of both stars. For example, if a star loses its envelope in a mass-transfer phase, it may explode in a supernova and produce a neutron star rather than collapsing into a black hole at the end of its life. In about 25% of massive stars, this mass-transfer even leads to a merger of both binary components.