Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition?
Giovanni Montani, Iolanda Navone, Maria Giovanna Dainotti, Shigehiro Nagataki
astro-ph.CO
Submitted: 2026-07-01
Comments: 26 pages, 6 figures
DOI: 10.1103/xthk-9854
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A New Master Supernovae Ia sample and the investigation of the $H_0$ tension
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- The Hubble constant tension: current status and future perspectives through new cosmological probes
- Quasar standardization: Overcoming Selection Biases and Redshift Evolution
- A new binning method to choose a standard set of Quasars
- Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities
- The Scavenger Hunt for Quasar Samples to Be Used as Cosmological Tools
- The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
- Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
- High-redshift Cosmology by Gamma-Ray Bursts: an overview
- Revisiting the Concordance $\Lambda$CDM model using Gamma-Ray Bursts together with Supernovae Ia and Planck data
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Revealing Limitation in the Standard Cosmological Model: A Redshift-Dependent Hubble Constant from Fast Radio Bursts
- Hubble Constant and Mass Determination of Centaurus A & M83 from TRGB Distances
- A model-independent measurement of the Hubble constant from gravitational-wave standard sirens and electromagnetic observations
- Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models
- Evolving Dark Energy or Supernovae Systematics?
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