Luna Zagorac

Luna Zagorac's picture
Postdoctoral Fellow
Perimeter Institute of Theoretical Physics
Research Areas: 
Research : 

My research interests tend to lie at the intersection of theoretical cosmology, particle astrophysics, and high-powered computing (HPC). I am moved by questions of cosmic archaeology, encapsulating phenomena in the early universe including inflation, dark matter production, primordial black holes, and large scale structure evolution. At the same time, I am passionate about questions of archaeoastronomy and cosmogony, particularly in the case of using primary hieroglyphic sources to map Ancient Egyptian constellations and understand relevant notions of  universal creation. 

Ph.D. 2022, Yale University
Honors & Awards: 
  • 2021 - Leigh Page Award for Excellence in Graduate Student Teaching
  • 2020 - Loyde and William C. G. Ortel Fellowship in Physics from Yale University
  • 2020 - Future Investigators in NASA Earth and Space Science and Technology (FINESST)
  • 2019 - Franke Graduate Student Fellowship
Selected Publications: 
Zagorac, Sands, Padmanabhan, and Easther. “Schrödinger-Poisson solitons: Perturbation theory.” Physical Review D 105.10 (2022): 103506.
Padmanabhan, Ronaghan, Zagorac, and Easther. “Simulating Ultralight Dark Matter with Chapel: An Experience Report.” In SC19 Proceedings (2019).
Zagorac, Easther, and Padmanabhan. “GUT-scale primordial black holes: mergers and gravitational waves.” Journal of Cosmology and Astroparticle Physics 2019.06(2019): 052 .
Thesis Advisor: 
Nikhil Padmanabhan & Richard Easther (University of Auckland)
Dissertation Title: 
A Light in the Dark: UltraLight Dark matter Phenomenology in Simulation
Dissertation Abstract: 

Of the outstanding problems in astronomy, the nature of dark matter is certainly one of the most mysterious. Containing five times more energy density than its luminous counterpart, dark matter has been shaping the large-scale structure of our Universe for billions of years. The expansion of accessible and accurate cosmological simulations has revolutionized how we visualize the imprint of dark matter in the structure of our Universe. In my Ph.D., I contributed to this revolution through the development and implementation of a new code, CHPLULTRA: a parallel, portable, and efficient tool for HPC simulations of a promising dark matter candidate, Fuzzy or UltraLight Dark Matter (ULDM). ULDM is a well-motivated axion-like dark matter candidate whose incredibly small mass results in naturally cored profiles, thus ameliorating many of the small-scale problems of cold dark matter (CDM) while maintaining the same robust large-scale results. When unperturbed, the lowest energy solution of the ULDM system is a spherical “soliton” structure with a known mass density profile. A ULDM dark matter halo is formed through collisions of these solitons and has two characteristic parts: a central soliton core, and an NFW “skirt” surrounding it. In order to investigate ULDM dynamics, I calculated the full spectrum of eigenstates for ULDM systems with approximately stationary potentials, thus allowing me to 1) link the qualitative behavior of soliton cores in ULDM simulations with superpositions of specific modes and 2) decompose CHPLULTRA simulations of ULDM halos into individual eigenstates. Using this formalism, I investigated the formation of halos through soliton collisions and the dependence of the final halo product on initial parameters. Crucially, this allowed me to explore how halo cores form and explain discrepancies in the literature surrounding the core-halo mass relation: a key prediction of ULDM. I was also able to comment on the composition of the halos’ skirts, including their qualitative behavior and eigenstate makeup, as a function of initial binary parameters. Finally, I sketched out some of the exciting future directions for understanding ULDM through the language of its eigenstates; these include combining my work on ULDM with my previous work on primordial black holes, which is included as part of this dissertation.