University of Cambridge > Talks.cam > Theoretical Physics Colloquium > Determining the origin of LIGO's merging black holes

Determining the origin of LIGO's merging black holes

Download to your calendar using vCal

If you have a question about this talk, please contact Francesca Chadha-Day .

Although black holes can be the remnants of dead stars, it is also possible that primordial black holes exist, which formed long before stars. Such black holes are a dark matter candidate, and they could also explain some of the unexpected properties of the black hole mergers that LIGO has detected. I will summarise the evidence and challenges behind this claim, and then focus on how current and future data can be used to discriminate between astrophysical and primordial black holes. Finally, I will explain why the QCD transition during the early universe may lead to a large enhancement in the formation rate of primordial black holes with mass below the Chandrasekhar mass limit.

This talk is part of the Theoretical Physics Colloquium series.

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

Š 2006-2025 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity