Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
arXiv:2211.11438 · doi:10.1140/epjp/s13360-022-03595-6
Abstract
Following results presented in Spallicci et al. (Eur Phys J Plus 137, 2022) by the same authors, we investigate the observed red shift , working under the hypothesis that it might be composed by the expansion red shift and an additional frequency shift , towards the red or the blue, due to Extended Theories of Electromagnetism (ETE). We have tested this prediction considering the novel Pantheon+ Catalogue, composed by 1701 light curves collected by 1550 SNe Ia, and 16 BAO data, for different cosmological models characterised by the absence of a dark energy component. In particular, we shall derive which values of match the observations, comparing the new results with the ones obtained considering the older Pantheon Catalogue. We find interesting differences in the resulting distributions, highlighted in the text. Later, we also add a discussion regarding Extended Theories of Gravity and how to incorporate them in our methodology.
arXiv comment7 Figures, 8 Tables, 18 Pages. Follow up of arXiv:2202.02731
References in corpus (63)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Observation of Gravitational Waves from a Binary Black Hole Merger
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Extended Theories of Gravity
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- Lorentz-Violating Extension of the Standard Model
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- CPT Violation and the Standard Model
- Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- The Pantheon+ Analysis: Cosmological Constraints
- Beyond the Cosmological Standard Model
- The Cosmic Triangle: Revealing the State of the Universe
- The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
- The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
- Cosmological implications of baryon acoustic oscillation (BAO) measurements
- Cobaya: Code for Bayesian Analysis of hierarchical physical models
- Dynamical systems applied to cosmology: dark energy and modified gravity
- The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey
- On the Hubble constant tension in the SNe Ia Pantheon sample
- Further stable neutron star models from f(R) gravity
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman- forests
- Aspects of the cosmological "coincidence problem"
- Extreme neutron stars from Extended Theories of Gravity
- Towards an automated tool to evaluate the impact of the nuclear modification of the gluon density on quarkonium, D and B meson production in proton-nucleus collisions
- Maximal neutron star mass and the resolution of hyperon puzzle in modified gravity
- Stellar structure models in modified theories of gravity: lessons and challenges
- Modified Gravity and Cosmology: An Update by the CANTATA Network
- Nonperturbative models of quark stars in gravity
- The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
- Photon Mass Limits from Fast Radio Bursts
- Direct Measurements of Neutrino Mass
- Magnetic Neutron Stars in f(R) gravity
- Is exponential gravity a viable description for the whole cosmological history?
- Observational Evidence of the Accelerated Expansion of the Universe
- Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
- Tests and problems of the standard model in Cosmology
- FRB 121102 Casts New Light on the Photon Mass
- Non-Local Gravity Cosmology: an Overview
- Updating constraints on f(T) teleparallel cosmology and the consistency with Big Bang Nucleosynthesis
- Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
- The mass-radius relation for neutron stars in gravity: a comparison between purely metric and torsion formulations
- Addressing the cosmological tension by the Heisenberg uncertainty
- Observational Constraints on Exponential Gravity
- Solar wind test of the de Broglie-Proca's massive photon with Cluster multi-spacecraft data
- Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
- Massive photons from Super and Lorentz symmetry breaking
- Polytropic stars in Palatini gravity
- Observational tests for Λ(t)CDM cosmology
- Photon sector analysis of Super and Lorentz symmetry breaking: effective photon mass, bi-refringence and dissipation
- Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio frequencies
- Cosmology and the massive photon frequency shift in the Standard-Model Extension
- The Heisenberg limit at cosmological scales
- Constraints on the exponential model from latest Hubble parameter measurements
- Investigating dark energy by electromagnetic frequency shifts
- Frequency variation for in vacuo photon propagation in the Standard-Model Extension
- Non minimally coupled condensate cosmologies: matching observational data with phase space
Cited by in corpus (8)
- On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample
- Early Dark Energy with Power-law F(R) Gravity
- Questioning the tension via the look-back time
- A critical discussion on the tension
- Dynamical dark energy can amplify the expansion rate of the Universe
- Testing the Ampère-Maxwell law on the photon mass and Lorentz-Poincaré symmetry violation with MMS multi-spacecraft data
- Photon frequency variation in non-linear electro-magnetism
- A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation