Measuring dark energy equation of state parameter from the compound lens system DES0408-5354
This is the project of my Master’s thesis carried out during my master studies in astrophysics at EPFL.
- Duration: 6 months (February 2023 - August 2023)
- Supervisor: Joshua Frieman (Department of Astronomy and Astrophysics, UChicago)
Overview
Compound lenses — strong lenses with multiple Einstein rings or arcs from multiple sources at different redshifts — allow measuring the cosmological parameters such as the matter density parameter Omega_m and the dark energy equation of state parameter w. However, such systems are extremely rare, with only one system analyzed so far to constrain the aforementioned parameters. This project will analyze a new compound lens system, DES J0408-5354, and constrain the w parameter for the dark energy. To model this complex system, with multiple source components and one source quasar, we will use the state-of-the-art modeling software lenstronomy.
Gravitational lensing acts as a coordinate transformation that distorts the images of background objects (usually galaxies) near a foreground mass. A gravitational lens is a distribution of matter (such as a cluster of galaxies) between a distant light source and an observer that is capable of bending the light from the source as the light travels toward the observer
References
- STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354 Shajib et al. 20Z0
About this project
- Gravitational lensing
- Cosmology
- Lenstronomy
Links
- Here’s the link to the [report]