# Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

@inproceedings{Alestas2021LatetransitionVS, title={Late-transition vs smooth \$H(z)\$ deformation models for the resolution of the Hubble crisis}, author={George Alestas and David Camarena and Eleonora Di Valentino and Lavrentios Kazantzidis and Valerio Marra and Savvas Nesseris and Leandros Perivolaropoulos}, year={2021} }

George Alestas, ∗ David Camarena, † Eleonora Di Valentino, ‡ Lavrentios Kazantzidis, § Valerio Marra, 5, 6, ¶ Savvas Nesseris, ∗∗ and Leandros Perivolaropoulos †† Department of Physics, University of Ioannina, GR-45110, Ioannina, Greece PPGCosmo, Universidade Federal do Esṕırito Santo, 29075-910, Vitória, ES, Brazil School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom Núcleo de Astrof́ısica e Cosmologia & Departamento de F́ısica…

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