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Core-Collapse Supernova Physics in the Multi-Messenger Era

Citation

Gossan, Sarah Elizabeth (2019) Core-Collapse Supernova Physics in the Multi-Messenger Era. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/ZF1A-6394. https://resolver.caltech.edu/CaltechTHESIS:01312019-123521450

Abstract

Eighty-five years following the historic proposal that core-collapse supernovae accompanied the transition of evolved massive stars to neutron stars [1], the mechanism through which these collapsing stars explode remains uncertain. While supernovae are observed on a daily basis across the electromagnetic spectrum, neutrinos and gravitational waves, emitted from the very heart of the core-collapse supernova central engine, provide a direct glimpse of the dynamics driving the explosion. The joint gravitational wave and electromagnetic observations of a colliding neutron star binary system on 17th August 2017 heralded a new era for multi-messenger astronomy [2]. The next galactic core-collapse supernova presents an unparalleled opportunity to directly probe core-collapse supernova physics and the explosion mechanism.

This thesis explores a number of topics in multi-messenger astronomy and core-collapse supernova physics. First, it tackles the observation problem; detailing an astrophysically motivated search protocol for gravitational waves from core-collapse supernovae triggered by observations of neutrino and/or electromagnetic counterparts. Applying these methods to a number of hypothetical observational scenarios, it presents sensitivity estimates for the second generation of gravitational wave interferometric detectors to both realistic and speculative emission mechanisms associated with core-collapse supernovae. Next, it addresses the prospects for post-detection inference; developing a Bayesian toolkit to interpret gravitational wave observations from core-collapse supernovae and augment current understanding of the explosion mechanism. A proof-of-principle study is also presented, using tailor-made simulations to demonstrate the viability of extracting the angular momentum distribution of nascent millisecond proto-neutron stars from their gravitational wave echoes. Thereafter, it considers the ramifications of failure to accurately capture proto-neutron star hydrodynamics in core-collapse supernova simulations; exploring the influence on the explosion mechanism of gravito-acoustic waves generated by convection in the proto-neutron star mantle. Finally, it ponders the impact of advances in multi-messenger astronomy and source modelling over the next twenty years on the understanding of core-collapse supernova physics.

Item Type:Thesis (Dissertation (Ph.D.))
Subject Keywords:Core-collapse supernovae; Gravitational waves; LIGO; Multi-messenger astronomy
Degree Grantor:California Institute of Technology
Division:Physics, Mathematics and Astronomy
Major Option:Physics
Awards:France A. Córdova Graduate Student Fund, 2016.
Thesis Availability:Public (worldwide access)
Research Advisor(s):
  • Weinstein, Alan Jay
Group:LIGO
Thesis Committee:
  • Fuller, James (chair)
  • Adhikari, Rana
  • Chen, Yanbei
  • Weinstein, Alan Jay
  • Hopkins, Philip F.
Defense Date:22 February 2019
Non-Caltech Author Email:sarah.gossan (AT) gmail.com
Record Number:CaltechTHESIS:01312019-123521450
Persistent URL:https://resolver.caltech.edu/CaltechTHESIS:01312019-123521450
DOI:10.7907/ZF1A-6394
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevD.93.042002DOIArticle adapted for Chapter 4
https://doi.org/10.1103/PhysRevD.94.123012DOIArticle adapted for Chapter 5
https://doi.org/10.1103/PhysRevD.90.044001DOIArticle adapted for Chapter 6
https://arxiv.org/abs/1905.02842arXivArticle adapted for Chapter 8
ORCID:
AuthorORCID
Gossan, Sarah Elizabeth0000-0002-8138-9198
Default Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:11369
Collection:CaltechTHESIS
Deposited By: Sarah Gossan
Deposited On:03 Jun 2019 19:38
Last Modified:04 Oct 2019 00:24

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