The Mad Era: A Possible New Resolution to the Horizon, Flatness, and Monopole Problems

dc.creatorFreese, Katherine
dc.creatorLevin, Janna J
dc.date1992-11-10
dc.date.accessioned2026-07-07T02:18:43Z
dc.date.available2026-07-07T02:18:43Z
dc.descriptionA cosmology with a dynamical Planck mass $m_{pl}$ is shown to solve the horizon and monopole problems (and possibly flatness) if there is an early MAD (modified aging) era where the universe becomes older than in the standard model as a result of a large $m_{pl}$: the causality condition is $m_{pl}(T_c)/ m_{pl}(T_o) \gta T_c/T_o$ ($T_c$ is some high temperature while $T_o = 2.74K$.) Unlike inflation, there is no period of vacuum domination nor any entropy violation. We study: a) bare scalar theories of gravity, b) self-interacting models, and c) bare theories with a phase transition in the matter sector.
dc.description12 pages,Tex, XXX
dc.identifierhttps://arxiv.org/abs/astro-ph/9211008
dc.identifierhttp://arxiv.org/abs/astro-ph/9211008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9595
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe Mad Era: A Possible New Resolution to the Horizon, Flatness, and Monopole Problems
dc.typetext

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