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Inflación
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1
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84“…In both cases the models have one real scalar, the inflaton, naturally suited for single-field inflation. Vectors and tensors required by supersymmetry to complement a single real scalar do not acquire vev's during inflation, so there is no need to stabilize the extra scalars which are always present in the theories with chiral matter multiplets. …”
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85
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86“…We present a setup that provides a partial UV-completion of the ghost inflation model up to a scale which can be almost as high as the Planck mass. …”
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87“…Higgs inflation can occur if the Standard Model (SM) is a self-consistent effective field theory up to inflationary scale. …”
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88“…Both of these can describe the data well and give slow-roll inflation for large fields without the need for a precise balancing of terms in the potential. …”
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89“…The slow roll regime of inflation models is understood in this context as the slow evolution close to a fixed point, described by the methods of renormalisation group. …”
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Enlace del recurso
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90
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91
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94por Espinosa, Jose Ramon“…--HTML-->After reviewing the nice properties of Higgs inflation and some of its problems, I will discuss a simple unitarization of the scenario that is genuinely weakly coupled up to Planckian energies. …”
Publicado 2015
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95
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96“…Sneutrino inflation employs the fermionic partners of the inflaton and stabilizer field as right-handed neutrinos to realize the seesaw mechanism for light neutrino masses. …”
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Enlace del recurso
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97“…We prove that all inflationary models, including those with dark energy after the end of inflation, can be embedded in minimal supergravity with a single chiral superfield. …”
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Enlace del recurso
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98
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