Guardado en:
Detalles Bibliográficos
Autor principal: Di Valentino, Eleonora
Formato: Preprint
Publicado: 2026
Materias:
Acceso en línea:https://arxiv.org/abs/2601.01525
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866918271582732288
author Di Valentino, Eleonora
author_facet Di Valentino, Eleonora
contents Cosmology has entered an era of unprecedented precision, yet increasing accuracy has revealed cracks in the standard $Λ$CDM paradigm. Although the model remains highly successful when confronted with individual datasets, joint analyses expose a network of tensions involving the Hubble constant, CMB lensing, curvature, neutrino masses, and the nature of dark energy. In this contribution to the 3rd General Meeting of the COST Action COSMIC WISPers (CA21106), within the context of Working Group~2, we critically assess these discrepancies, emphasizing the role of model assumptions, parameter degeneracies, and dataset consistency. We review proposed early- and late-time solutions, discuss how recent DESI BAO results alter the viability of late-time extensions, and explore interacting dark-sector scenarios. Our analysis highlights the need for caution in interpreting cosmological measurements and underscores the importance of internal consistency among cosmological probes before claiming percent-level accuracy or invoking new physics.
format Preprint
id arxiv_https___arxiv_org_abs_2601_01525
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Cracks in the Standard Cosmological Model: Anomalies, Tensions, and Hints of New Physics
Di Valentino, Eleonora
Cosmology and Nongalactic Astrophysics
Cosmology has entered an era of unprecedented precision, yet increasing accuracy has revealed cracks in the standard $Λ$CDM paradigm. Although the model remains highly successful when confronted with individual datasets, joint analyses expose a network of tensions involving the Hubble constant, CMB lensing, curvature, neutrino masses, and the nature of dark energy. In this contribution to the 3rd General Meeting of the COST Action COSMIC WISPers (CA21106), within the context of Working Group~2, we critically assess these discrepancies, emphasizing the role of model assumptions, parameter degeneracies, and dataset consistency. We review proposed early- and late-time solutions, discuss how recent DESI BAO results alter the viability of late-time extensions, and explore interacting dark-sector scenarios. Our analysis highlights the need for caution in interpreting cosmological measurements and underscores the importance of internal consistency among cosmological probes before claiming percent-level accuracy or invoking new physics.
title Cracks in the Standard Cosmological Model: Anomalies, Tensions, and Hints of New Physics
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2601.01525