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In this paper we will illustrate how to constrain unavoidable K\"ahler corrections for ${\cal N}=1$ supergravity (SUGRA) inflation from the recent Planck data. We will show that the non-renormalizable K\"ahler operators will induce in…

High Energy Physics - Theory · Physics 2014-04-15 Sayantan Choudhury , Anupam Mazumdar , Ernestas Pukartas

A class of well-motivated models of inflation end by producing cosmic strings. The current status of efforts to calculate and observe the signals from such models are outlined, with a particular emphasis on cosmic strings, and on the Cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Mark Hindmarsh

In string theory compactifications it is common to find an effective Lagrangian for the scalar fields with a non-canonical kinetic term. We study the effective action of the scalar position moduli of Type II D$p$-branes. In many instances…

High Energy Physics - Theory · Physics 2016-06-07 Sjoerd Bielleman , Luis E. Ibanez , Francisco G. Pedro , Irene Valenzuela , Clemens Wieck

We examine a non-Abelian SUSY $SU(2) \times U(1)$ gauge theory and a SUSY U(1) theory originally used to investigate the microphysics of cosmic strings in supersymmetric theories. We show that both theories automatically include hybrid…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. C. Davis , M. Majumdar

We investigate whether cosmological inflation is possible in a class of flux compactifications of type IIA strings on rigid Calabi-Yau manifolds, when all perturbative string corrections are taken into account. We confine ourselves to the…

High Energy Physics - Theory · Physics 2017-08-28 Yuki Wakimoto , Sergei V. Ketov

In this talk I discuss recent developments in moduli stabilisation, SUSY breaking and chiral D-brane models together with several interesting features of cosmological models built in the framework of type IIB string compactifications. I…

High Energy Physics - Theory · Physics 2016-04-05 Michele Cicoli

We use a new mechanism for generating a Fayet-Iliopoulos term in supergravity, which is not associated to an R symmetry, to construct a semi-realistic theory of slow-roll inflation for a theory with the same K\"ahler potential and…

High Energy Physics - Theory · Physics 2021-05-14 Hun Jang , Massimo Porrati

We show that the parameter space for F-term inflation which predict the formation of cosmic strings is larger than previously estimated. Firstly, because realistic embeddings in GUT theories alter the standard scenerio, making the…

High Energy Physics - Theory · Physics 2009-11-11 Rachel Jeannerot , Marieke Postma

We perform a general algebraic analysis on the possibility of realising slow-roll inflation in the moduli sector of string models. This problem turns out to be very closely related to the characterisation of models admitting metastable…

High Energy Physics - Theory · Physics 2014-11-18 Laura Covi , Marta Gomez-Reino , Christian Gross , Jan Louis , Gonzalo A. Palma , Claudio A. Scrucca

In this work, we present two classes of inflationary models in the framework of type IIB string theory. The inflatons correspond to blow-up K\"ahler modulus arising from compactifying type IIB string theory on a Calabi-Yau. Using…

High Energy Physics - Theory · Physics 2025-07-08 Mishaal Hai , Ahmed Rakin Kamal , Noshin Ferdous Shamma , Md Shaikot Jahan Shuvo

Fibre inflationary models are constructed in type-IIB string flux compactification. These models have been shown to be in agreement with the cosmological observations under appropriate choices of parameters, which originate from their…

High Energy Physics - Theory · Physics 2025-09-04 Dibya Chakraborty , Rudnei O. Ramos

We consider a cosmological scenario within the KKLT framework for moduli stabilization in string theory. The universal open string tachyon of decaying non-BPS D-brane configurations is proposed to drive eternal topological inflation.…

High Energy Physics - Theory · Physics 2009-11-11 Daniel Cremades , Fernando Quevedo , Aninda Sinha

High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large…

High Energy Physics - Theory · Physics 2016-01-20 Michele Cicoli , Francesco Muia , Francisco Gil Pedro

We study the possibility of canceling the cosmological constant in supergravity string models. We show that with a suitable choice of superpotential the vacuum energy may vanish with the dilaton field at its minimum and supersymmetry broken…

High Energy Physics - Phenomenology · Physics 2016-09-01 Axel de la Macorra

We study the cosmology of a recent model of supersymmetry breaking, in the presence of a tuneable positive cosmological constant, based on a gauged shift symmetry of a string modulus that can be identified with the string dilaton. The…

High Energy Physics - Phenomenology · Physics 2016-12-20 I. Antoniadis , A. Chatrabhuti , H. Isono , R. Knoops

Tribrid inflation is a class of supersymmetric inflation models where the scalar component of a matter superfield, or a $D$-flat direction of matter fields, drives inflation. Similar to Hybrid inflation, the end of inflation is reached when…

High Energy Physics - Phenomenology · Physics 2024-11-06 Stefan Antusch , Katarina Trailović

Inflationary potentials are investigated for specific models in type IIB string theory via flux compactification. As concrete models, we investigate several cases where the internal spaces are weighted projective spaces. The models we…

High Energy Physics - Theory · Physics 2011-03-15 Sunggeun Lee , Soonkeon Nam

We obtain cosmological constraints on models of inflation which exhibit rapid roll solutions. Rapid roll attractors exist for potentials with large mass terms and are thus of interest for inflationary model building within string theory. We…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-15 Takeshi Kobayashi , Shinji Mukohyama , Brian A. Powell

Minimal chaotic models of D-term inflation predicts too large primordial tensor perturbations. Although it can be made consistent with observations utilizing higher order terms in the K\"ahler potential, expansion is not controlled in the…

High Energy Physics - Theory · Physics 2016-05-13 Kazunori Nakayama , Ken'ichi Saikawa , Takahiro Terada , Masahide Yamaguchi

The potential during inflation must be very flat in, at least, the direction of the inflaton. In renormalizable global supersymmetry, flat directions are ubiquitous, but they are not preserved in a generic supergravity theory. It is known…

High Energy Physics - Theory · Physics 2009-09-29 Mary K. Gaillard , David H. Lyth , Hitoshi Murayama