PDC mobile packet data communication network

Hirata, Shoichi; Nakajima, A.; Uesaka, H.

doi:10.1109/icupc.1995.497088

Cited by 10 publications

(1 citation statement)

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“…This Z-statistic [127] has been used to estimate the impact of improvements to cosmic recombination history computations on CMB parameter estimation [97,99,101]. If Z 1, we can safely conclude that the systematic errors in C A induced by use of the EFA make a negligible impact on the estimation of both Ω ax and standard cosmological parameters.…”

Section: Z-statistic and Biasmentioning

confidence: 99%

How sound are our ultralight axion approximations?

2020

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Ultra-light axions (ULAs) are a promising dark-matter candidate. ULAs may have implications for small-scale challenges to the ΛCDM model, and arise in string scenarios. ULAs are already constrained by cosmic microwave background (CMB) experiments and large-scale structure surveys, and will be probed with much greater sensitivity by future efforts. It is challenging to compute observables in ULA scenarios with sufficient speed and accuracy for cosmological data analysis because the ULA field oscillates rapidly. In past work, an effective fluid approximation has been used to make these computations feasible. Here this approximation is tested against an exact solution of the ULA equations, comparing the induced error of CMB observables with the sensitivity of current and future experiments. In the most constrained mass range for a ULA dark matter component (10 −27 eV ≤ max ≤ 10 −25 eV), the induced bias on the allowed ULA fraction of dark matter from Planck data is less than 1σ. In the cosmic-variance limit (including temperature and polarization data), the bias is 2σ for primary CMB anisotropies, with more severe biases (as high as ∼ 4σ) resulting for less reliable versions of the effective fluid approximation. If all of the standard cosmological parameters are fixed by other measurements, the expected bias rises to 4 − 20σ (well beyond the validity of the Fisher approximation), though the required level of degeneracy breaking will not be achieved by any planned surveys.PACS numbers: 14.80. Mz,90.70.Vc,95.35.+d,98.80.Cq

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