Evidence for extra radiation? Profile likelihood versus Bayesian posterior
arXiv:1110.4271 · doi:10.1088/1475-7516/2012/03/021
Abstract
A number of recent analyses of cosmological data have reported hints for the presence of extra radiation beyond the standard model expectation. In order to test the robustness of these claims under different methods of constructing parameter constraints, we perform a Bayesian posterior-based and a likelihood profile-based analysis of current data. We confirm the presence of a slight discrepancy between posterior- and profile-based constraints, with the marginalised posterior preferring higher values of the effective number of neutrino species N_eff. This can be traced back to a volume effect occurring during the marginalisation process, and we demonstrate that the effect is related to the fact that cosmic microwave background (CMB) data constrain N_eff only indirectly via the redshift of matter-radiation equality. Once present CMB data are combined with external information about, e.g., the Hubble parameter, the difference between the methods becomes small compared to the uncertainty of N_eff. We conclude that the preference of precision cosmological data for excess radiation is "real" and not an artifact of a specific choice of credible/confidence interval construction.
10 pages, 4 figures; v2: discussion section expanded and references added, version accepted for publication by JCAP
References in corpus (8)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Massive neutrinos and cosmology
- Cosmology seeking friendship with sterile neutrinos
- Sterile neutrinos with eV masses in cosmology -- how disfavoured exactly?
- The Case for Dark Radiation
- Maximum Likelihood algorithm for parametric component separation in CMB experiments
- Observational bounds on the cosmic radiation density
- Are priors responsible for cosmology favoring additional neutrino species?
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- The Atacama Cosmology Telescope: Cosmological parameters from three seasons of data
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- Updated constraints on non-standard neutrino interactions from Planck
- Converting non-relativistic dark matter to radiation
- Dark Radiation and Dark Matter in Large Volume Compactifications
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- Asymmetric Dark Matter and Dark Radiation
- Increasing Neff with particles in thermal equilibrium with neutrinos
- Resolving the Hubble tension with Early Dark Energy
- Testing 3+1 and 3+2 neutrino mass models with cosmology and short baseline experiments
- Right-Handed Neutrinos as the Dark Radiation: Status and Forecasts for the LHC
- Vanishing effective mass of the neutrinoless double beta decay including light sterile neutrinos
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- Probing dark radiation with inflationary gravitational waves
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- What is half a neutrino? Reviewing cosmological constraints on neutrinos and dark radiation
- Dark Radiation in extended cosmological scenarios
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- Testing standard and non-standard neutrino physics with cosmological data
- Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
- LHC Phenomenology and Cosmology of String-Inspired Intersecting D-Brane Models
- Profile Likelihoods in Cosmology: When, Why and How illustrated with CDM, Massive Neutrinos and Dark Energy
- Dark energy from dark radiation in strongly coupled cosmologies with no fine tuning
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- Fast and effortless computation of profile likelihoods using CONNECT
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