{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,12]],"date-time":"2025-10-12T02:43:36Z","timestamp":1760237016883,"version":"build-2065373602"},"reference-count":69,"publisher":"MDPI AG","issue":"2","license":[{"start":{"date-parts":[[2020,2,19]],"date-time":"2020-02-19T00:00:00Z","timestamp":1582070400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Symmetry"],"abstract":"<jats:p>Thermal Leptogenesis and the gravitino problem are reviewed in the framework of non-standard cosmologies. We consider in particular the     f ( T )     cosmology, where    T    is the torsion field. We constrain the parameters space of these cosmological models consistently with thermal Leptogenesis scenario (with degenerate mass spectrum of light neutrinos), and we show that they allow to solve the gravitino problem as well. Owing to the similar characteristics to     f ( T )     cosmology, we shortly discuss also the case of the shear dominated Universe.<\/jats:p>","DOI":"10.3390\/sym12020300","type":"journal-article","created":{"date-parts":[[2020,2,26]],"date-time":"2020-02-26T04:18:29Z","timestamp":1582690709000},"page":"300","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":3,"title":["Consequences of f ( T )     Cosmology in Thermal Leptogenesis and Gravitino Late Abundance"],"prefix":"10.3390","volume":"12","author":[{"given":"Antonio","family":"Capolupo","sequence":"first","affiliation":[{"name":"Dipartimento di Fisica \u201cE.R. Caianiello\u201d Universit\u00e1 di Salerno, and INFN\u2013Gruppo Collegato di Salerno, SA 84084 Fisciano, Italy"}]},{"given":"Salvatore","family":"Giampaolo","sequence":"additional","affiliation":[{"name":"Division of Theoretical Physics, Ruder Bo\u0161kovi\u0107 Institute, Bijen\u010dka cesta 54, 10000 Zagreb, Croatia"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-7574-2330","authenticated-orcid":false,"given":"Gaetano","family":"Lambiase","sequence":"additional","affiliation":[{"name":"Dipartimento di Fisica \u201cE.R. Caianiello\u201d Universit\u00e1 di Salerno, and INFN\u2013Gruppo Collegato di Salerno, SA 84084 Fisciano, Italy"}]},{"given":"Aniello","family":"Quaranta","sequence":"additional","affiliation":[{"name":"Dipartimento di Fisica \u201cE.R. Caianiello\u201d Universit\u00e1 di Salerno, and INFN\u2013Gruppo Collegato di Salerno, SA 84084 Fisciano, Italy"}]}],"member":"1968","published-online":{"date-parts":[[2020,2,19]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"99","DOI":"10.1016\/0370-2693(80)90670-X","article-title":"A New Type of Isotropic Cosmological Models without Singularity","volume":"91","author":"Starobinsky","year":"1980","journal-title":"Phys. Lett. B"},{"key":"ref_2","doi-asserted-by":"crossref","first-page":"1","DOI":"10.1016\/j.physrep.2017.06.001","article-title":"Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution","volume":"692","author":"Nojiri","year":"2017","journal-title":"Phys. Rep."},{"key":"ref_3","doi-asserted-by":"crossref","first-page":"219","DOI":"10.1007\/978-3-540-71013-4_8","article-title":"Models of dark energy","volume":"720","author":"Sami","year":"2007","journal-title":"Lect. 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