Constraining dark matter properties with self-annihilating dark matter admixed white dwarfs
• Aug 2023 — Present
Supervisors: Prof. M.-C. Chu, Dr. L.-M. Lin
- Derive framework for white dwarfs partially-sustained by photon pressure sourcing from dark matter self-annihilation in hydrostatic balance
- Study the stable structure configuration of white dwarfs with self-annihilating dark matter admixed
- Constrain the dark matter interaction rate and particle mass by comparing the observed white dwarf mass-radius relationship with the simulated one
Testing stability and asteroseismology of bosonic dark matter admixed white dwarfs with variable scattering length
• May 2022 — Oct 2023
Final Year Project Report
Supervisor: Prof. M.-C. Chu
- Demonstrated admixing bosonic dark matter can possibly explain specific mass-radius relationships in white dwarfs
- Illustrated the instability of white dwarfs partially hosting attractive bosonic dark matter lead to black holes
- Probed the asteroseismology of white dwarfs containing bosonic dark matter of density-dependent scattering length
- Tested stability and hydrodynamics of admixed white dwarfs under general relativity and approximated rotation
Addressing Missing Satellite Problem by decyaing dark matter halo
• May — Jul 2021
Poster
Supervisor: Prof. M.-C. Chu
- Modified the model to be more realistic by transforming initial circular orbits to elliptical orbits with a range of eccentricity
- Simulated decaying dark matter halo density profile time evolution to account for Missing Satellite Problem
- Constrained decaying dark matter nature with lowered expected amount of satellite galaxies in line with observed amount
Programming
Experienced in Python, C, Fortran, Julia and SQL
Languages
Fluent in English, Cantonese and Mandarin Chinese