Cosmological constant in F(R) supergravity

Sergei V. Ketov, Natsuki Watanabe

Результат исследований: Материалы для журналаСтатья

7 Цитирования (Scopus)

Выдержка

A cosmological constant in the regime of low space-time curvature is calculated in the recently proposed version of F(R) supergravity with a generic cubic function F. The F(R) supergravity is the N= 1 supersymmetric extension of f(R) gravity. The cubic model is known to successfully describe a chaotic (slow-roll) inflation in the regime of high space-time curvature. We find that a simple extension of the same model allows a positive cosmological constant in the regime of low space-time curvature. The inflaton superfield in F(R) supergravity (like inflaton in f(R) gravity) violates the Strong Energy Condition and thus breaks the restriction of the standard supergravity (with usual matter) that can only have either a negative or vanishing cosmological constant.

Язык оригиналаАнглийский
Страницы (с-по)410-413
Число страниц4
ЖурналPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Том705
Номер выпуска4
DOI
СостояниеОпубликовано - 17 ноя 2011
Опубликовано для внешнего пользованияДа

Отпечаток

supergravity
curvature
gravitation
constrictions
energy

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Цитировать

Cosmological constant in F(R) supergravity. / Ketov, Sergei V.; Watanabe, Natsuki.

В: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Том 705, № 4, 17.11.2011, стр. 410-413.

Результат исследований: Материалы для журналаСтатья

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