Cosmological parameter estimation using Particle Swarm Optimization (PSO)
Jayanti Prasad, Tarun Souradeep (Inter-University Centre for, Astronomy, Astrophysics (IUCAA), Pune (India))

TL;DR
This paper explores the use of Particle Swarm Optimization (PSO), a stochastic method from engineering, for estimating cosmological parameters from WMAP data, comparing its performance with traditional MCMC techniques.
Contribution
It demonstrates the application of PSO to cosmological parameter estimation and discusses its advantages for extensive searches in high-dimensional spaces.
Findings
PSO yields parameter estimates consistent with MCMC results.
Error bars differ due to different computation methods.
PSO shows promise for efficient high-dimensional searches.
Abstract
Obtaining the set of cosmological parameters consistent with observational data is an important exercise in current cosmological research. It involves finding the global maximum of the likelihood function in the multi-dimensional parameter space. Currently sampling based methods, which are in general stochastic in nature, like Markov-Chain Monte Carlo(MCMC), are being commonly used for parameter estimation. The beauty of stochastic methods is that the computational cost grows, at the most, linearly in place of exponentially (as in grid based approaches) with the dimensionality of the search space. MCMC methods sample the full joint probability distribution (posterior) from which one and two dimensional probability distributions, best fit (average) values of parameters and then error bars can be computed. In the present work we demonstrate the application of another stochastic method,…
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