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We explore the possibility that quantum cosmology considerations could provide a selection principle in the landscape of string vacua. We propose that the universe emerged from the string era in a thermally excited state and determine,…

High Energy Physics - Theory · Physics 2009-11-11 R. Brustein , S. P. de Alwis

We investigate cosmological evolution in models where the effective potential V(\phi) may become negative for some values of the field \phi. Phase portraits of such theories in space of variables (\phi,\dot\phi,H) have several qualitatively…

High Energy Physics - Theory · Physics 2009-09-29 Gary Felder , Andrei Frolov , Lev Kofman , Andrei Linde

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

Most parameterizations of the dark energy equation of state do not reflect realistic underlying physical models. Here, we develop a relatively simple description of dark energy based on the dynamics of a scalar field which is exact in the…

Astrophysics · Physics 2008-11-26 Robert Crittenden , Elisabetta Majerotto , Federico Piazza

We introduce moduli spaces of quasi-admissible hyperelliptic covers with at worst A and D singularities. The stability conditions for these moduli spaces depend on two parameters describing allowable singularities. By varying these…

Algebraic Geometry · Mathematics 2010-12-03 Maksym Fedorchuk

We consider the cosmological evolution induced by the free energy F of a gas of maximally supersymmetric heterotic strings at finite temperature and weak coupling in dimension D>=4. We show that F, which plays the role of an effective…

High Energy Physics - Theory · Physics 2011-06-20 John Estes , Lihui Liu , Herve Partouche

A dual component made of non-relativistic particles and a scalar field, exchanging energy, naturally falls onto an attractor solution, making them a (sub)dominant part of the cosmic energy during the radiation dominated era, provided that…

Cosmology and Nongalactic Astrophysics · Physics 2012-08-15 Silvio A. Bonometto , Giandomenico Sassi , Giuseppe La Vacca

We examine the modular properties of nonrenormalizable superpotential terms in string theory and show that the requirement of modular invariance necessitates the nonvanishing of certain Nth order nonrenormalizable terms. In a class of…

High Energy Physics - Theory · Physics 2009-10-22 S. Kalara , J. Lopez , D. Nanopoulos

In theories beyond the Standard Model, in particular in theories with extra spatial dimensions such as superstring theory, there are a large number of scalar fields which appear in the low energy effective action. These moduli fields must…

High Energy Physics - Theory · Physics 2021-09-29 Mesbah Alsarraj , Robert Brandenberger

We study how two moduli can be stabilized in a Minkowski/de Sitter vacuum for a wide class of string-inspired Supergravity models with an effective Fayet-like Supersymmetry breaking. It is shown under which conditions this mechanism can be…

High Energy Physics - Theory · Physics 2008-12-04 Diego Gallego , Marco Serone

We review the structure of the moduli space of particular N = (2,2) superconformal field theories. We restrict attention to those of particular use in superstring compactification, namely those with central charge c = 3d for some integer d…

High Energy Physics - Theory · Physics 2007-05-23 Paul Aspinwall

We find the N-soliton solution at infinite theta, as well as the metric on the moduli space corresponding to spatial displacements of the solitons. We use a perturbative expansion to incorporate the leading 1/theta corrections, and find an…

High Energy Physics - Theory · Physics 2010-02-03 L. Hadasz , U. Lindstrom , M. Rocek , R. von Unge

Cosmological constraints on moduli, whose coupling to matter is stronger than Planck mass suppressed coupling, are derived. In particular, moduli are considered to be produced by oscillating loops of cosmic strings and constraints are…

High Energy Physics - Phenomenology · Physics 2010-11-08 Eray Sabancilar

Recently, an interesting class of the direct gauge mediation supersymmetry (SUSY) breaking models are proposed, in which the minimum of the potential of the SUSY breaking field is determined by the inverted hierarchy mechanism. We consider…

High Energy Physics - Phenomenology · Physics 2014-11-17 Takeo Moroi

We calculate the scalar potential of supersymmetric QCD (in the regime N_f < N_c) coupled to N=1 supergravity with moduli-dependent gauge kinetic function and masses. The gauge dynamics are described by the Taylor-Veneziano-Yankielowicz…

High Energy Physics - Theory · Physics 2009-10-31 Thomas Dent

Oscillating moduli fields can support a cosmological scaling solution in the presence of a perfect fluid when the scalar field potential satisfies appropriate conditions. We examine when such conditions arise in higher-dimensional,…

High Energy Physics - Theory · Physics 2008-11-26 James E. Lidsey , Karim A. Malik

The symmetric spaces that appear as moduli spaces in string theory and supergravity can be decomposed with explicit metrics using parabolic subgroups. The resulting isometry between the original moduli space and this decomposition can be…

High Energy Physics - Theory · Physics 2024-07-31 Paul S. Aspinwall

We present a moduli dependent target space effective field theory action for (truncated) heterotic string toroidal compactifications. When moving continuously along moduli space, the stringy gauge symmetry enhancement-breaking effects,…

High Energy Physics - Theory · Physics 2019-03-27 G. Aldazabal , E. Andrés , M. Mayo , V. Penas

To understand in detail the contribution of a world-sheet instanton to the superpotential in a heterotic string compactification, one has to understand the moduli dependence (bundle and complex structure moduli) of the one-loop determinants…

High Energy Physics - Theory · Physics 2009-10-02 Gottfried Curio

Observation indicates that the expansion of the Universe is accelerating and favours a dynamical cosmological constant, \Lambda(t). We consider the possibility that this is due to a scalar field which has undergone a very recent phase…

High Energy Physics - Phenomenology · Physics 2014-11-17 John McDonald
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