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Supersymmetry breaking in string theory is expected to occur when moduli fields acquire non-trivial expectation values. In the early universe these fields start out displaced from their final destinations. I present some recent ideas about…

High Energy Physics - Theory · Physics 2007-05-23 R. Brustein

The interplay between string theory and cosmology is very promising. Since string theory will yield a quantum theory of space-time and unify all forces of nature, it has the potential of addressing many of the conceptual problems of the…

High Energy Physics - Theory · Physics 2007-05-23 Robert H. Brandenberger

We present a full characterization of the phase transition in U(1) scalar field theory and of the associated vortex string thermodynamics in 3D. We show that phase transitions in the string densities exist and measure their critical…

High Energy Physics - Phenomenology · Physics 2016-09-06 Nuno D. Antunes , Luis M. A. Bettencourt , Mark Hindmarsh

Topological defects such as cosmic strings may have been formed at early-universe phase transitions. Direct tests of this idea are impossible, but the mechanism can be elucidated by studying analogous processes in low-temperature…

Soft Condensed Matter · Physics 2009-11-07 T. W. B. Kibble

We present observation of large, expanding string loops forming around a heated wire tip embedded in a nematic liquid crystal sample. Loops expand due to convective stretching. This observation leads to a new insight into phenomena which…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ajit M. Srivastava

We investigate the string configuration that, in the framework of the theoretical scenario introduced in [1], corresponds to the most entropic configuration in the phase space of all the configurations of the universe. This describes a…

General Physics · Physics 2011-03-22 Andrea Gregori

We show that stable local cosmic strings are a generic prediction of supersymmetric models where supersymmetry is broken at scales within a few orders of magnitude of the weak scale and is fed down to the observable sector by gauge…

High Energy Physics - Phenomenology · Physics 2009-10-30 Antonio Riotto

We describe a new mechanism, whose ingredients are realised in string compactifications, for the formation of cosmic (super)string networks. Oscillating string loops grow when their tension $\mu$ decreases with time. If $2H + \dot{\mu}/\mu…

High Energy Physics - Phenomenology · Physics 2024-06-19 Joseph P. Conlon , Edmund J. Copeland , Edward Hardy , Noelia Sánchez González

We argue that in the context of string theory a large number N of connected degenerate vacua that mix will lead to a ground state with much lower energy, essentially because of the standard level repulsion of quantum theory for the…

High Energy Physics - Theory · Physics 2007-05-23 G. L. Kane , M. J. Perry , A. N. Zytkow

We study the primordial magnetic field generated by stochastic currents produced by scalar charged particles created at the beginning of the radiation dominated epoch. We find that for the mass range 10^(-6)GeV \leq m \leq 10^2 GeV, a field…

Astrophysics · Physics 2008-11-26 Esteban A. Calzetta , Alejandra Kandus , Francisco D. Mazzitelli

We discuss how cosmic strings can be created in heterotic M-theory compactifications with stable moduli. We conclude that the only appropriate candidates seem to be fundamental open membranes with a small length. In four dimensions they…

High Energy Physics - Theory · Physics 2009-11-11 Evgeny I. Buchbinder

We investigate the microphysics of cosmic strings in Nonabelian gauge theories with N=1 supersymmetry. We give the vortex solutions in a specific example and demonstrate that fermionic superconductivity arises because of the couplings and…

High Energy Physics - Phenomenology · Physics 2009-10-30 Stephen C. Davis , Anne C. Davis , Mark Trodden

It has been suggested that cosmological dark matter may include a population of vortons (meaning small centrifugally stabilised cosmic string loops) as an outcome of (non-standard) electroweak symmetry breaking. The implications for this…

High Energy Physics - Phenomenology · Physics 2007-05-23 B. Carter

We consider quintessence models within 4D effective descriptions of gravity coupled to two scalar fields. These theories are known to give rise to viable models of late-time cosmic acceleration without any need for flat potentials, and so…

High Energy Physics - Theory · Physics 2022-11-30 Max Brinkmann , Michele Cicoli , Giuseppe Dibitetto , Francisco G. Pedro

We study the generation of primordial magnetic fields, coherent over cosmologically interesting scales, by gravitational creation of charged scalar particles during the reheating period. We show that magnetic fields consistent with those…

High Energy Physics - Phenomenology · Physics 2009-10-07 Alejandra Kandus , Esteban A. Calzetta , Francisco D. Mazzitelli , Carlos E. M. Wagner

We derive a constraint on the cosmic density of string moduli fields in gauge-mediated supersymmetry-breaking theories by requiring that photons emitted from the unstable moduli fields should not exceed the observed X-ray backgrounds. Since…

High Energy Physics - Phenomenology · Physics 2015-06-25 M. Kawasaki , T. Yanagida

An exploratory study of the cosmology of moduli in string theory. Moduli are argued to be natural inflaton fields and lead to a robust inflationary cosmology in which inflation takes place at the top of domain walls. The amplitude of…

High Energy Physics - Theory · Physics 2016-09-06 T. Banks , M. Berkooz , G. Moore , S. H. Shenker , P. J. Steinhardt

In this talk, I review a number of particle-physics models that lead to the creation of magnetic fields in the early universe and address the complex problem of evolving such primordial magnetic fields into the fields observed today.…

Astrophysics · Physics 2016-11-03 Ola Tornkvist

Cosmic superstrings are introduced to non-experts. First D-branes and $(p,q)$ strings are discussed. Then we explain how tachyon condensation in the early universe may have produced F, D and $(p,q)$ strings. Warped geometries which can…

High Energy Physics - Theory · Physics 2007-05-23 Mahbub Majumdar

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