This workshop is intended for undergraduate/graduate students and researchers interested in learning cosmology and numerical computations using CLASS and MontePython. During this workshop, participants will learn:
- Basic cosmology including cosmological perturbation theory.
- Bayesian statistics and Markov Chain Monte Carlo (MCMC) technique for analysing parameter constraints for data.
- MontePython and CLASS application in cosmology.
Organizing Committee
- Piyabut Burikham, Chulalongkorn University, Thailand
- Kamphee Karwan, Institute for Fundamental Study, Naresuan University, Thailand
- Pitayuth Wongjun, Institute for Fundamental Study, Naresuan University, Thailand
- Teeraparb Chantavat, Institute for Fundamental Study, Naresuan University, Thailand
- Nandan Roy, Centre for Theoretical Physics and Natural Philosophy, Mahidol University, Thailand
- Chakkrit Kaeonikhom, Chiang Mai Rajabhat University, Chiang Mai, Thailand
- Utane Sawangwit, National Astronomical Research Institute of Thailand, Thailand
- Poom Kumam, King Mongkut's University of Technology Thonburi, Thailand
**Limited availability up to 30 participants. The attending participants will be announced at later time. The participants must bring his/her own computer/laptop to the workshop.
Deadline for Registration 22 November 2024
CLASS
CLASS (Cosmic Linear Anisotropy Solving System) is a powerful and widely used cosmological Boltzmann code that computes the evolution of perturbations in the universe. It is employed to solve the coupled Einstein-Boltzmann equations, which describe the dynamics of different components of the universe—such as dark matter, baryons, photons, neutrinos, and dark energy—at linear scales. CLASS is designed to handle a wide range of cosmological models and provides accurate predictions for various cosmological observables.
MontePython
MontePython is a software tool used in the field of cosmology for conducting Bayesian parameter estimation from cosmological data. It is similar in function to CosmoMC, which I mentioned earlier. MontePython uses Markov Chain Monte Carlo (MCMC) techniques to sample the parameter space of cosmological models and estimate the likelihood of these models given observed data.
Researchers in cosmology and astrophysics use MontePython to analyze a wide range of cosmological data, such as data from cosmic microwave background (CMB) experiments, large-scale structure surveys, and other astrophysical observations. The tool allows for the exploration and constraints of various cosmological parameters, helping researchers to determine the best-fitting models that describe the universe's properties and evolution.
MontePython is a flexible and customizable software package that can be adapted to different cosmological models and datasets. It provides a framework for performing advanced statistical analyses and comparing theoretical models to observational data, contributing to our understanding of the cosmos and the fundamental parameters that describe it.