CORDIS Project
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This project aims to enhance the understanding of common envelope evolution in binary star systems, which is crucial for interpreting gravitational wave observations. It will use advanced simulations to study mass loss and energy dynamics during this phase, linking theoretical predictions with observational data.
One of the crucial formation channels of compact object binaries, including sources of gravitational waves, critically depends on catastrophic binary interactions accompanied by the loss of mass, angular momentum, and energy (""common envelope"" evolution - CEE).
Despite its importance, CEE is perhaps the least understood major phase of binary star evolution and progress in this area is urgently needed to interpret observations from the new facilities (gravitational wave detectors, time-domain s…
UNIVERZITA KARLOVA
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