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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

Models of inflation are instructive playgrounds for supersymmetry breaking in Supergravity and String Theory. In particular, combinations of branes and orientifolds that are not mutually BPS can lead to \emph{brane supersymmetry breaking},…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-08 A. Sagnotti

Brane inflation in superstring theory ends when branes collide, initiating the hot big bang. Cosmic superstrings are produced during the brane collision. The cosmic superstrings produced in a D3-brane-antibrane inflationary scenario have a…

Astrophysics · Physics 2014-10-13 S. -H. Henry Tye , Ira Wasserman , Mark Wyman

Cosmic strings are predicted by many field-theory models, and may have been formed at a symmetry-breaking transition early in the history of the universe, such as that associated with grand unification. They could have important…

High Energy Physics - Theory · Physics 2010-05-07 Edmund J. Copeland , T. W. B. Kibble

The Standard Model is the low-energy limit of a microscopic theory which includes extra dimensions and new symmetries. A part of my thesis consisted in constructing a new class of models with two extra dimensions. We showed that these…

High Energy Physics - Theory · Physics 2007-08-27 Chloe Papineau

We show how chiral type I models whose tadpole conditions have no supersymmetric solution can be consistently defined introducing antibranes with non-supersymmetric world volumes. At tree level, the resulting stable non-BPS configurations…

High Energy Physics - Theory · Physics 2014-11-18 C. Angelantonj , I. Antoniadis , G. D'Appollonio , E. Dudas , A. Sagnotti

D-branes are fundamental in all scenarios where there are large extra dimensions and the string scale is much smaller than the four-dimensional Planck mass. We show that this current picture leads to a new approach to string cosmology where…

High Energy Physics - Phenomenology · Physics 2009-10-31 Antonio Riotto

We consider the 3+1 visible sector to live on a Hanany-Witten D-brane construction in type IIA string theory. The messenger sector consists of stretched strings from the visible brane to a hidden D6-brane in the extra spatial dimensions. In…

High Energy Physics - Theory · Physics 2007-05-23 John H. Brodie

We study a class of type I string models with supersymmetry broken on the world-volume of some D-branes and vanishing tree-level potential. Despite the non-supersymmetric spectrum, supersymmetry is non-linearly realized on these D-branes,…

High Energy Physics - Theory · Physics 2015-06-26 I. Antoniadis , K. Benakli , A. Laugier

The first part of this review tries to provide a self-contained view of supersymmetry breaking from the bottom-up perspective. We thus describe N=1 supersymmetry in four dimensions, the Standard Model and the MSSM, with emphasis on the…

High Energy Physics - Theory · Physics 2026-02-25 E. Dudas , J. Mourad , A. Sagnotti

In the present thesis I studied the phenomenology arising from a class of string models called sequestered compactifications, which were born with the aim of getting low-energy SUSY from strings. This is not an easy task if combined with…

High Energy Physics - Theory · Physics 2016-03-21 Francesco Muia

We consider dynamics of a scalar field in compactification scenario of Einstein-Gauss-Bonnet cosmology. It is shown that if the field is non-minimally coupled to curvature, its asymptotic value under certain conditions may be shifted from…

General Relativity and Quantum Cosmology · Physics 2024-09-27 Dmitry Chirkov , Alex Giacomini , Alexey Toporensky , Petr Tretyakov

In brane world models of nature, supersymmetry breaking is often isolated on a distant brane in a higher dimensional space. The form of the Kahler potential in generic string and M-theory brane world backgrounds is shown to give rise to…

High Energy Physics - Theory · Physics 2008-11-26 Alexey Anisimov , Michael Dine , Michael Graesser , Scott Thomas

String theory has no parameter except the string scale $M_S$, so the Planck scale $M_\text{Pl}$, the supersymmetry-breaking scale, the EW scale $m_\text{EW}$ as well as the vacuum energy density (cosmological constant) $\Lambda$ are to be…

High Energy Physics - Theory · Physics 2021-01-25 Yu-Cheng Qiu , S. -H. Henry Tye

We study supersymmetry breaking by Scherk-Schwarz compactifications in type I string theory. While in the gravitational sector all mass splittings are proportional to a (large) compactification radius, supersymmetry remains unbroken for the…

High Energy Physics - Theory · Physics 2009-10-31 I. Antoniadis , E. Dudas , A. Sagnotti

We study whether the universal runaway behaviour of stringy scalar potentials towards infinite field distance limits can produce an accelerated expanding cosmology \`{a} la quintessence. We identify a loophole to some proposed bounds that…

High Energy Physics - Theory · Physics 2024-01-11 José Calderón-Infante , Ignacio Ruiz , Irene Valenzuela

We explore the cosmological dynamics of a minimalistic yet generic string-inspired model for multifield dark energy. Adopting a supergravity four-dimensional viewpoint, we motivate the model's structure arising from superstring…

High Energy Physics - Theory · Physics 2024-02-16 Diego Gallego , J. Bayron Orjuela-Quintana , César A. Valenzuela-Toledo

In this work, we investigate the properties of string effective theories with scalar field(s) and a scalar potential. We first claim that in most examples known, such theories are multifield, with at least 2 non-compact field directions;…

High Energy Physics - Theory · Physics 2025-04-29 David Andriot , Muthusamy Rajaguru , George Tringas

We demonstrate that string consistency in four spacetime dimensions leads to a spectrum of string states which satisfies the supertrace constraints Str(M^0)=0 and Str(M^2)=\Lambda at tree level, where \Lambda is the one-loop string…

High Energy Physics - Theory · Physics 2009-10-28 Keith R. Dienes , Moshe Moshe , Robert C. Myers

We investigate the scalar potential of string compactifications in the parametric regime where string loops and higher derivative corrections to 10d supergravity can be ignored and where the fields are rolling down exponential slopes…

High Energy Physics - Theory · Physics 2024-01-09 Thomas Van Riet