Generalized dilaton–axion models of inflation, de Sitter vacua and spontaneous SUSY breaking in supergravity; European Physical Journal C; Vol. 79, iss. 8

Generalized dilaton–axion models of inflation, de Sitter vacua and spontaneous SUSY breaking in supergravity; European Physical Journal C; Vol. 79, iss. 8

Dades bibliogràfiques
Parent link:European Physical Journal C
Vol. 79, iss. 8.— 2019.— [713, 12 p.]
Autor principal: Aldabergenov Ye. Yermek
Autor corporatiu: Национальный исследовательский Томский политехнический университет Исследовательская школа физики высокоэнергетических процессов
Altres autors: Chatrabhuti A. Auttakit, Ketov S. V. Sergey Vladimirovich
Sumari:Title screen
We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in N=1N=1 supergravity with the dilaton-axion chiral superfield T in the presence of an N=1N=1 vector multiplet with the alternative Fayet-Iliopoulos term. By using the Kähler potential as K=−αlog(T+T¯¯¯¯)K=−αlog⁡(T+T¯) and the superpotential as a sum of a constant and a linear term, we find that viable inflation is possible for 3≤α≤αmax3≤α≤αmax where αmax≈7.235αmax≈7.235. Observations of the amplitude of primordial scalar perturbations fix the SUSY breaking scale in our models as high as 1013 GeV1013 GeV. In the case of α>3α>3 the axion gets the tree-level (non-tachyonic) mass comparable to the inflaton mass.
Idioma:anglès
Publicat: 2019
Matèries:
электронный ресурс
труды учёных ТПУ
Accés en línia:https://doi.org/10.1140/epjc/s10052-019-7225-2
Format: Electrònic Capítol de llibre
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=663705

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