Populations of Gravitational Wave Sources

Understanding the population of gravitational wave sources can give insight into astrophysical processes, provide probes of cosmological parameters, and put individual events in context.

I'm interested in using features inferred from the population to inform a wide range of astrophysical phenomena. Some examples include stable mass transfer in binary starts, the supernova mechanism, gamma ray burst jet geometry, and the neutron star equation of state.

Understanding the population of gravitational wave sources can give insight into astrophysical processes, provide probes of cosmological parameters, and put individual events in context.

I'm interested in using features inferred from the population to inform a wide range of astrophysical phenomena. Some examples include stable mass transfer in binary starts, the supernova mechanism, gamma ray burst jet geometry, and the neutron star equation of state.

Understanding the population of gravitational wave sources can give insight into astrophysical processes, provide probes of cosmological parameters, and put individual events in context. I'm interested in using features inferred from the population to place limits on astrophysical phenomena, like the supernova mechanism, gamma ray burst jet geometry, and the neutron star equation of state.

The population of gravitational wave sources can give insight into astrophysical processes like the supernova mechanism, gamma ray burst jet geometry, and the neutron star equation of state. It also provides a direct probe of the cosmic expansion history and helps put individual events in context.

Click through the plots to see some examples of my work on these topics. Clicking on a plot will take you to the publication in which it is featured.