Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM

In this work, we consider an Om diagnostic using a non-parametric reconstruction by employing the Loess–Simex factory. This procedure allows us to perform a model-independent comparison for w(z) with the astrophysical data. The concordance model can be tested with the advantage that our approach rep...

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Bibliographic Details
Main Authors: Celia Escamilla-Rivera, Júlio C. Fabris
Format: Article
Language:English
Published: MDPI AG 2016-12-01
Series:Galaxies
Subjects:
Online Access:http://www.mdpi.com/2075-4434/4/4/76
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spelling doaj-677b0f8de8b34300bc0dd45f577cc7392020-11-24T23:22:54ZengMDPI AGGalaxies2075-44342016-12-01447610.3390/galaxies4040076galaxies4040076Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDMCelia Escamilla-Rivera0Júlio C. Fabris1Mesoamerican Centre for Theoretical Physics, Universidad Autónoma de Chiapas, Carretera Zapata Km. 4, Real del Bosque (Terán), 29040 Tuxtla Gutiérrez, MexicoDepartamento de Física, Universidade Federal do Espírito Santo, Av. Fernando Ferrari 514, Vitória 29075-910, BrazilIn this work, we consider an Om diagnostic using a non-parametric reconstruction by employing the Loess–Simex factory. This procedure allows us to perform a model-independent comparison for w(z) with the astrophysical data. The concordance model can be tested with the advantage that our approach represents an alternative and efficient way to relax the use of priors and find a possible w that reliably describes the data with no previous knowledge of a cosmological model.http://www.mdpi.com/2075-4434/4/4/76cosmic accelerationdark energynon-parametric diagnostics
collection DOAJ
language English
format Article
sources DOAJ
author Celia Escamilla-Rivera
Júlio C. Fabris
spellingShingle Celia Escamilla-Rivera
Júlio C. Fabris
Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM
Galaxies
cosmic acceleration
dark energy
non-parametric diagnostics
author_facet Celia Escamilla-Rivera
Júlio C. Fabris
author_sort Celia Escamilla-Rivera
title Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM
title_short Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM
title_full Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM
title_fullStr Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM
title_full_unstemmed Nonparametric Reconstruction of the Om Diagnostic to Test ΛCDM
title_sort nonparametric reconstruction of the om diagnostic to test λcdm
publisher MDPI AG
series Galaxies
issn 2075-4434
publishDate 2016-12-01
description In this work, we consider an Om diagnostic using a non-parametric reconstruction by employing the Loess–Simex factory. This procedure allows us to perform a model-independent comparison for w(z) with the astrophysical data. The concordance model can be tested with the advantage that our approach represents an alternative and efficient way to relax the use of priors and find a possible w that reliably describes the data with no previous knowledge of a cosmological model.
topic cosmic acceleration
dark energy
non-parametric diagnostics
url http://www.mdpi.com/2075-4434/4/4/76
work_keys_str_mv AT celiaescamillarivera nonparametricreconstructionoftheomdiagnostictotestlcdm
AT juliocfabris nonparametricreconstructionoftheomdiagnostictotestlcdm
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