{"paper":{"title":"Late-Time Mild Inflation --- a possible solution of dilemma: cosmic age and the Hubble parameter ---","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Akika Nakamichi, Masae Miyoshi, Masahiro Morikawa, Mikiko Hatakeyama, Takeshi Fukuyama","submitted_at":"1996-08-15T01:59:47Z","abstract_excerpt":"We explore the cosmological model in which a late-time mild inflation is realized after the star formation epoch. Non-vanishing curvature coupling of a classical boson field yields this mild inflation without a cosmological constant. Accordingly the lifetime of the present Universe is remarkably increased in our model. Thus we show that the present observed high value of the Hubble parameter $H_0 \\approx 70-80{\\rm km/sec/Mpc}$ is compatible with the age of the oldest stars $14{\\rm Gyr}$ without introducing the cosmological constant or the open Universe model. Moreover in our model, the local H"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9608097","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}