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From the 1 of 10 linked papers with an AI index.

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10 papers

astro-ph.CO2026

Model-Independent Indication for a Localized Anomaly in the Late-Time Expansion History

Shibendu Gupta Choudhury, Purba Mukherjee, Eleonora Di Valentino +1

Using a model‑independent spline reconstruction of distances from DESI BAO data and DES supernovae, the authors find a localized ~3.5σ deviation from the Planck ΛCDM expansion hist…

astro-ph.CO2026

Quintessential Implications of the presence of AdS in the Dark Energy sector

Purba Mukherjee, Dharmendra Kumar, Anjan A Sen

We explore the implications for an Anti-de Sitter (AdS) vacuum, equivalently a negative cosmological constant (nCC), in the dark energy (DE) sector using current cosmological obser…

astro-ph.CO2026

Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?

Anirban Chakraborty, Tirthankar Roy Choudhury, Anjan Ananda Sen +1

The unexpectedly large abundance of UV-bright galaxies at discovered by the James Webb Space Telescope poses a significant challenge to the standard CDM cosmology. This…

astro-ph.CO2025

Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations

Drishti Sharma, Purba Mukherjee, Anjan A Sen +1

We investigate the impact of instrumental and astrophysical systematics on dark energy constraints derived from Type~Ia supernova (SN-Ia) observations. Using simulated datasets con…

astro-ph.CO2025

Anchoring the Universe with Characteristic Redshifts using Raychaudhuri Equation Informed Reconstruction Algorithm (REIRA)

Shibendu Gupta Choudhury, Purba Mukherjee, Anjan Ananda Sen

We study the robustness and physical implications of a set of characteristic redshifts that capture key features of the late-time Universe. Using both model-independent reconstruct…

astro-ph.CO2025

New Expansion Rate Anomalies at Characteristic Redshifts Geometrically Determined using DESI-DR2 BAO and DES-SN5YR Observations

Purba Mukherjee, Anjan A Sen

We perform a model-independent reconstruction of the cosmic distances using the Multi-Task Gaussian Process (MTGP) framework as well as knot-based spline techniques with DESI-DR2 B…