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| Title: |
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| Speaker: |
Dr. Ashley J. Ruiter (Senior Lecturer)
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| Affiliation: |
The University of New South Wales, Canberra |
| Datetime: |
Oct.16,Monday, AM10:20-11:20 |
| Venue: |
Room 427,Buld 1# |
| Abstract: |
It is well known that neutron stars are born during the death of massive stars in iron core-collapse supernovae. However, they can also form via more exotic formation scenarios like the accretion-induced collapse of a white dwarf star in a binary system. I will show some results of formation scenarios of neutron stars formed via the collapse of a heavy white dwarf, and comment on their potential detectability with gravitational radiation. While the implementation of a sophisticated method to deal with the common envelope phase in binary population synthesis is still a work in progress, preliminary results show that we may be able to constrain common envelope physics with accretion-induced collapse (and also Type Ia supernova) progenitors using future space-based gravitational wave detectors.
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