Extended dark energy analysis using DESI DR2 BAO measurements

dc.contributor.authorK. Lodha
dc.contributor.authorR. Calderón
dc.contributor.authorWilliam L. Matthewson
dc.contributor.authorArman Shafieloo
dc.contributor.authorM Ishak
dc.contributor.authorJian Pan
dc.contributor.authorC. García-Quintero
dc.contributor.authorD Huterer
dc.contributor.authorGeorgios Valogiannis
dc.contributor.authorLuís Alfonso Ureña López
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T13:55:10Z
dc.date.available2026-03-22T13:55:10Z
dc.date.issued2025
dc.descriptionCitaciones: 82
dc.description.abstractWe conduct an extended analysis of dark energy constraints, in support of the findings of the Dark Energy Spectroscopic Instrument (DESI) second data release cosmology key paper, including DESI data, Planck cosmic microwave background observations, and three different supernova compilations. Using a broad range of parametric and nonparametric methods, we explore the dark energy phenomenology and find consistent trends across all approaches, in good agreement with the <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>w</a:mi><a:mn>0</a:mn></a:msub><a:msub><a:mi>w</a:mi><a:mi>a</a:mi></a:msub><a:mi>CDM</a:mi></a:math> (cold dark matter) key paper results. Even with the additional flexibility introduced by nonparametric approaches, such as binning and Gaussian processes, we find that extending <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi mathvariant="normal">Λ</c:mi><c:mi>CDM</c:mi></c:math> to include a two-parameter <f:math xmlns:f="http://www.w3.org/1998/Math/MathML" display="inline"><f:mi>w</f:mi><f:mo stretchy="false">(</f:mo><f:mi>z</f:mi><f:mo stretchy="false">)</f:mo></f:math> is sufficient to capture the trends present in the data. Finally, we examine three dark energy classes with distinct dynamics, including quintessence scenarios satisfying <j:math xmlns:j="http://www.w3.org/1998/Math/MathML" display="inline"><j:mi>w</j:mi><j:mo>≥</j:mo><j:mo>−</j:mo><j:mn>1</j:mn></j:math>, to explore what underlying physics can explain such deviations. The current data indicate a clear preference for models that feature a phantom crossing; although alternatives lacking this feature are disfavored, they cannot yet be ruled out. Our analysis confirms that the evidence for dynamical dark energy, particularly at low redshift (<l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"><l:mi>z</l:mi><l:mo>≲</l:mo><l:mn>0.3</l:mn></l:math>), is robust and stable under different modeling choices.
dc.identifier.doi10.1103/w4c6-1r5j
dc.identifier.urihttps://doi.org/10.1103/w4c6-1r5j
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/43485
dc.language.isoen
dc.publisherAmerican Physical Society
dc.relation.ispartofPhysical review. D/Physical review. D.
dc.sourceKorea Astronomy and Space Science Institute
dc.subjectDark energy
dc.subjectPhysics
dc.subjectQuintessence
dc.subjectCosmic microwave background
dc.subjectPlanck
dc.subjectCosmology
dc.subjectAstrophysics
dc.subjectRedshift
dc.subjectNonparametric statistics
dc.subjectBaryon acoustic oscillations
dc.titleExtended dark energy analysis using DESI DR2 BAO measurements
dc.typearticle

Files