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Investigating dark energy experiments with principal components

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arxiv astro-ph/0510293 v2 pith:UDOYKHDO submitted 2005-10-10 astro-ph gr-qchep-ph

classification astro-phgr-qchep-ph
keywords darkenergyexperimentsprobesprincipalapproacharbitraryarray
verification ladder T0 review T1 audit T2 compute T3 formal
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We use a principal component approach to contrast different kinds of probes of dark energy, and to emphasize how an array of probes can work together to constrain an arbitrary equation of state history w(z). We pay particular attention to the role of the priors in assessing the information content of experiments and propose using an explicit prior on the degree of smoothness of w(z) that is independent of the binning scheme. We also show how a figure of merit based on the mean squared error probes the number of new modes constrained by a data set, and use it to examine how informative various experiments will be in constraining the evolution of dark energy.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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    First integration of tomographic AP tests with MCFs and PCA compression yields 48% and 45% tighter errors on Ω_m and w versus standard two-point functions.

  2. $\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    A variational autoencoder compresses CMB temperature spectra into 5 (LambdaCDM) or 8 (with early dark energy) latent parameters that reconstruct the data within Planck errors and can be constrained with Planck observations.

  3. Probing the independence within the dark sector in the fluid approximation

    astro-ph.CO 2019-08 accept novelty 5.0 of 10

    Current cosmological data show no statistically significant sign of an interaction between cold dark matter and dark energy, with LambdaCDM preferred, and future LSST and DESI data could constrain such a coupling at 2...

  4. Extended Dark Energy analysis using DESI DR2 BAO measurements

    astro-ph.CO 2025-03 conditional novelty 4.0 of 10

    Extended analysis of DESI DR2 data confirms robust evidence for dynamical dark energy with phantom crossing preference, stable under parametric and non-parametric modeling.

  5. Parametrizations for tests of gravity

    astro-ph.CO 2019-08 accept novelty 1.0 of 10

    A review of parametrized frameworks (PPF, EFT, PPN, ppE) for testing gravity across cosmological and astrophysical scales, with an outlook toward unification.

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