Bayesian methods for cosmological parameter estimation from cosmic microwave background measurements

DOI10.1088/0264-9381/18/14/306zbMath0990.83014arXivastro-ph/0006401OpenAlexW3105564333WikidataQ123417537 ScholiaQ123417537MaRDI QIDQ2752484

Lloyd Knox, Ben Luey, Renate Meyer, Nelson Christensen

Publication date: 13 March 2002

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0006401

zbMATH Keywords

Monte Carlo methodscosmological parameterscosmic microwave backgroundanisotropies

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items

Physical parameter space of bimetric theory and SN1a constraints ⋮ Effects of rainfall on \textit{Culex} mosquito population dynamics ⋮ Cosmic microwave background constraints on coupled dark matter ⋮ Laplace based Bayesian inference for ordinary differential equation models using regularized artificial neural networks ⋮ Statistical inference for dynamical systems: a review ⋮ DARK ENERGY FROM FIFTH-DIMENSIONAL BRANS–DICKE THEORY

This page was built for publication: Bayesian methods for cosmological parameter estimation from cosmic microwave background measurements