Project Overview
Astrophysical objects as Dark Matter probes
Department(s)
Physics and Astronomy
Abstract
One of the most profound mysteries of the Universe is the nature of the elusive component we call Dark Matter. We know of its existence based on its gravitational effects that range from the smallest of scales to the largest (super galactic cluster) scales. In fact, one Dark Matter provides the scaffolding upon which regular matter (i.e. matter forms us, stars, galaxies, clusters, etc.) distributes itself. One strategy to hut for dark matter is looking into its potential observable signatures in astrophysical objects such as stars, planets, brown dwarfs, white dwarfs, etc. Our group does just that: predicting the observable signatures of dark matter trapped inside celestial bodies. Now, we are at the stage where predictions can finally meet reality or data, if you want. This is because the James Webb Space Telescope, that is currently operational and providing publicly available data that is very relevant to this project. Depending on the interest (and strengths) of the student your role could be to further develop theoretical models (and make observable predictions) or to contrast existing models against existing data and infer what dark matter can or cannot be. Either way, you would be contributing to solving one of the deepest puzzles nature has posed for us: the nature of Dark Matter.
Student Qualifications
Students need to be highly proficient in numerical methods, preferably well versed in Python. Fortran knowledge would be a plus, although it is not necessary. A solid background in Astrophysics is needed, as well as familiarity with basic concepts of Cosmology.
Number of Student Researchers
3 students
Project Length
8 weeks