Implications of an extended dark energy model with massive neutrinos

Recently there has been reports of finding a lower bound on the neutrino mass parameter (\(\Sigma m_\nu\)) when using ACT and SPTpol data however these bounds on the \(\Sigma m_\nu\) are still weaker for most case around at 1 \(\sigma\) level. In this context, here in this work, we study the consequ...

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Veröffentlicht in:	arXiv.org 2022-06
Hauptverfasser:	Sharma, Ravi Kumar, Kanhaiya Lal Pandey, Das, Subinoy
Format:	Artikel
Sprache:	eng
Schlagworte:	Dark energy Equations of state Evolution Mathematical models Neutrinos Parameterization Parameters Physics - Cosmology and Nongalactic Astrophysics Sharpness Supernovae
Online-Zugang:	Volltext
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