Abstract
Following results presented in Spallicci et al. (Eur Phys J Plus 137, 2022) by the same authors, we investigate the observed red shift z, working under the hypothesis that it might be composed by the expansion red shift \(z_{\mathrm{C}}\) and an additional frequency shift \(z_{\mathrm{S}}\), 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 \(z_{\mathrm{S}}\) match the observations, comparing the new results with the ones obtained considering the older Pantheon Catalogue. We find interesting differences in the resulting \(z_{\mathrm{S}}\) distributions, highlighted in the text. Later, we also add a discussion regarding Extended Theories of Gravity and how to incorporate them in our methodology.
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Acknowledgements
Acknowledgements are due to J.A. Helayël-Neto (Rio de Janeiro) for our common work on the Extended Theories of Electromagnetism, to S. Savastano (Potsdam) for the work on the Cobaya routine, and to M. Lòpez Corredoira (La Laguna) for general comments and inputs. GS is grateful to the LPC2E laboratory for its hospitality during the work period on this manuscript. GS and SC acknowledge the support of Istituto Nazionale di Fisica Nucleare, Sez. di Napoli, Iniziative Specifiche MOONLIGHT-2 and QGSKY.
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Sarracino, G., Spallicci, A.D.A.M. & Capozziello, S. Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample. Eur. Phys. J. Plus 137, 1386 (2022). https://doi.org/10.1140/epjp/s13360-022-03595-6
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DOI: https://doi.org/10.1140/epjp/s13360-022-03595-6