CosmoSIS: a system for MC parameter estimation

被引:0
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作者
Bridle, S. [1 ]
Dodelson, S. [2 ,3 ,6 ]
Jennings, E. [3 ,4 ]
Kowalkowski, J. [2 ]
Manzotti, A. [3 ,6 ]
Paterno, M. [2 ]
Rudd, D. [3 ,5 ]
Sehrish, S. [2 ]
Zuntz, J. [1 ]
机构
[1] Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England
[2] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[3] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[4] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[5] Univ Chicago, Ctr Res Comp, Chicago, IL 60637 USA
[6] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
基金
美国国家科学基金会;
关键词
D O I
10.1088/1742-6596/664/7/072036
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
CosmoSIS is a modular system for cosmological parameter estimation, based on Markov Chain Monte Carlo and related techniques. It provides a series of samplers, which drive the exploration of the parameter space, and a series of modules, which calculate the likelihood of the observed data for a given physical model, determined by the location of a sample in the parameter space. While CosmoSIS ships with a set of modules that calculate quantities of interest to cosmologists, there is nothing about the framework itself, nor in the Markov Chain Monte Carlo technique, that is specific to cosmology. Thus CosmoSIS could be used for parameter estimation problems in other fields, including HEP. This paper describes the features of CosmoSIS and show an example of its use outside of cosmology. It also discusses how collaborative development strategies differ between two different communities: that of HEP physicists, accustomed to working in large collaborations, and that of cosmologists, who have traditionally not worked in large groups.
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页数:8
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