Noah Sennett - December 13, 2019 

Dissertation Title: Probing fundamental physics with gravitational waves from inspiraling binary systems

Date and Time: Friday, December 13, 2:30 pm 

Location: PSC 3150

Dissertation Committee Chair: Prof. Alessandra Buonanno

Committee: 

Prof. Theodore Jacobson
Prof. Julie McEnery
Prof. Peter Shawhan
Prof. Raman Sundrum
Prof. Massimo Ricotti, Dean’s Representative

Abstract: 

The first observations of gravitational waves from the mergers of black holes and/or neutron stars with Advanced LIGO and Virgo have opened a new window to the cosmos. This thesis examines how the gravitational-wave signal produced during the inspiral---the earliest phase of a binary system’s coalescence---can better inform our understanding of the highly dynamical, strong-curvature regime of gravity.

My work addressing this topic is comprised of two major components. First, I examine the behavior of binary black-hole and neutron-star systems in various possible extensions of General Relativity, constructing analytic models of their orbital motion and gravitational-wave production during their inspiral. Particular attention is devoted to alternative theories that admit scalarization, a second-order phase transition that occurs in compact bodies or binary systems that can manifest as non-perturbative phenomenology in a gravitational-wave signal.

The other component of this thesis is the development of a statistical infrastructure suitable for testing General Relativity using gravitational-wave observations. This framework is more flexible and modular approach than existing alternatives, allowing this infrastructure to be immediately employed with a wide range of waveform models. In work done in conjunction with the LIGO Scientific and Virgo Collaborations, I use this statistical framework to place bounds on phenomenological deviations from General Relativity using the binary black-hole and neutron-star events detected during LIGO's first and second observing runs. I also use this infrastructure to constrain certain specific alternative theories of gravity, including Brans-Dicke gravity.