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Inflación
13
Inflación (Finanzas)
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5
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Enciclopedias
1
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181“…Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. …”
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182
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183por García-Bellido, J“…The idea that the universe might be open is an old one, and the possibility of having an open universe arise form inflation is not new either. However, a concrete realization of a consistent single-bubble open inflation model is known only recently. …”
Publicado 1998
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184“…An inflationary stage dominated by a $D$-term avoids the slow-roll problem of inflation in supergravity and may emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. …”
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185“…This enables dilaton stabilisation during inflation with the $D$-term still dominating the vacuum energy at the stable minimum.…”
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186“…This happens in models of hybrid inflation based on orbifold constructions, in which a modulus $T$ field is responsible for the large value of the potential during inflation, and a second field illustrate the mechanism with a model in which the inflaton potential is provided by gaugino condensation, leading to succesful inflation.…”
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187“…We compute the leading-order back-reaction to dilaton-driven inflation, due to graviton, dilaton and gauge-boson production. …”
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188
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192
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193por Giovannini, Massimo“…Depending upon various parameters (scalar mass, curvature scale at the end of inflation and at the onset of the radiation epoch), the two-point function of the magnetic inhomogeneities grows during the de Sitter stage of expansion and, consequently, large scale magnetic fields are generated. …”
Publicado 2002
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194“…We give a pedagogical review of a mechanism through which long wave length photons can become massive during inflation. Our account begins with a discussion of the period of exponentially rapid expansion known as inflation. …”
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195“…We find faster-than-exponential growth in the fermion wave function, consistent with the production of fermions through a process in which a scalar and a fermion-anti-fermion pair are ripped out of the vacuum by inflation.…”
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196
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197“…We present a model of inflation based on a racetrack model without flux stabilization. …”
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198
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199“…We show how to enlarge the $\nu$MSM (the minimal extension of the standard model by three right-handed neutrinos) to incorporate inflation and provide a common source for electroweak symmetry breaking and for right-handed neutrino masses. …”
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