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Related papers: An Inflationary Model in String Theory

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"Brane supersymmetry breaking" occurs in String Theory when the only available combinations of D-branes and orientifolds are not mutually BPS and yet do not introduce tree-level tachyon instabilities. It is characterized by the emergence of…

High Energy Physics - Theory · Physics 2015-06-18 N. Kitazawa , A. Sagnotti

We discuss the effect of the dynamics of D-branes on moduli stabilization in type IIB string theory compactifications, with reference to a concrete toy model of T6/Z3 orientifold compactification with fractional D3-branes and anti-D3-branes…

High Energy Physics - Theory · Physics 2017-10-11 Noriaki Kitazawa

Non-supersymmetric brane world scenarios in string theory display perturbative instabilities that usually involve run-away potentials for scalar moduli fields. We investigate in the framework of intersecting brane worlds whether the leading…

High Energy Physics - Theory · Physics 2009-10-07 Ralph Blumenhagen , Boris Kors , Dieter Lust , Tassilo Ott

We explore the mechanics of inflation in simplified extra-dimensional models involving an inflaton interacting with the Einstein-Maxwell system in two extra dimensions. The models are Goldilocks-like in that they are just complicated enough…

General Relativity and Quantum Cosmology · Physics 2016-08-31 C. P. Burgess , Jared J. H. Enns , Peter Hayman , Subodh P. Patil

We present a new version of our racetrack inflation scenario which, unlike our original proposal, is based on an explicit compactification of type IIB string theory: the Calabi-Yau manifold P^4_[1,1,1,6,9]. The axion-dilaton and all complex…

High Energy Physics - Theory · Physics 2015-06-26 J. J. Blanco-Pillado , C. P. Burgess , J. M. Cline , C. Escoda , M. Gomez-Reino , R. Kallosh , A. Linde , F. Quevedo

String theory abounds with light scalar fields (the dilaton and various moduli) which create a host of observational problems, and notably some serious cosmological difficulties similar to the ones associated with the Polonyi field in the…

High Energy Physics - Theory · Physics 2009-10-28 Thibault Damour , Alexander Vilenkin

We show that the use of higher dimensional wrapped branes can significantly extend the inflaton field range compared to brane inflation models which use D3-branes. We construct a simple inflationary model in terms of 5-branes wrapping a…

High Energy Physics - Theory · Physics 2008-11-26 Melanie Becker , Louis Leblond , Sarah Shandera

We consider gravitational wave production during inflation in type IIB string theory, and the possibility of observable gravitational waves in small field inflation. We show that the gauge field excitations on a set of coincident D7 branes,…

High Energy Physics - Theory · Physics 2018-11-21 Evan McDonough , Stephon Alexander

The continuous shift symmetry of axions is at the heart of several realizations of inflationary models. In particular, axion monodromy inflation aims at achieving super-Planckian field ranges for the inflaton in the context of string…

High Energy Physics - Theory · Physics 2014-11-05 Fernando Marchesano , Gary Shiu , Angel M. Uranga

The inflationary paradigm provides a robust description of the peculiar initial conditions which are required for the success of the Hot Big Bang model of cosmology, as well as of the recent precision measurements of temperature…

High Energy Physics - Theory · Physics 2008-11-26 C. P. Burgess

We construct a multi-field inflationary model consisting of multiple K\"ahler moduli derived from type IIB string compactification in the large volume limit. The model consists of both heavy and light fields, with the former being frozen…

High Energy Physics - Theory · Physics 2009-12-09 Per Berglund , Guoqin Ren

We demonstrate an inflationary solution to the cosmological horizon problem during the Hagedorn regime in the early universe. Here the observable universe is confined to three spatial dimensions (a three-brane) embedded in higher…

High Energy Physics - Theory · Physics 2007-05-23 Steven Abel , Katherine Freese , Ian Kogan

We demonstrate an inflationary solution to the cosmological horizon problem during the Hagedorn regime in the early universe. Here the observable universe is confined to three spatial dimensions (a three-brane) embedded in higher…

High Energy Physics - Theory · Physics 2014-11-18 Steven Abel , Katherine Freese , Ian Kogan

The previously proposed class of phenomenological inflationary models in which the assumption of inflaton slow-roll is replaced by the more general, constant-roll condition is compared with the most recent cosmological observational data,…

Cosmology and Nongalactic Astrophysics · Physics 2017-04-28 Hayato Motohashi , Alexei A. Starobinsky

A supersymmetric inflationary stage dominated by an $F$-term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter $\eta$ gets contributions of order unity. We show that…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. A. Casas , G. B. Gelmini , A. Riotto

We provide a systematic treatment of possible corrections to the inflaton potential for D-brane inflation in the warped deformed conifold. We consider the D3-brane potential in the presence of the most general possible corrections to the…

High Energy Physics - Theory · Physics 2009-04-22 Daniel Baumann , Anatoly Dymarsky , Shamit Kachru , Igor R. Klebanov , Liam McAllister

We initiate a comprehensive survey of axion inflation in compactifications of type IIB string theory on Calabi-Yau hypersurfaces in toric varieties. For every threefold with $h^{1,1} \le 4$ in the Kreuzer-Skarke database, we compute the…

High Energy Physics - Theory · Physics 2017-03-08 Cody Long , Liam McAllister , John Stout

We present concrete embeddings of fibre inflation models in globally consistent type IIB Calabi-Yau orientifolds with closed string moduli stabilisation. After performing a systematic search through the existing list of toric Calabi-Yau…

High Energy Physics - Theory · Physics 2017-11-17 Michele Cicoli , Francesco Muia , Pramod Shukla

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

We construct a model of inflation based on a low-energy effective theory of spontaneously broken global scale invariance. This provides a shift symmetry that protects the inflaton potential from quantum corrections. Since the underlying…

High Energy Physics - Theory · Physics 2014-10-22 Csaba Csaki , Nemanja Kaloper , Javi Serra , John Terning
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