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Related papers: Induced superstring cosmologies and moduli stabili…

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We conduct a systematic search for a viable string/M-theory cosmology, focusing on cosmologies that include an era of slow-roll inflation, after which the moduli are stabilized and the Universe is in a state with an acceptably small…

High Energy Physics - Theory · Physics 2009-11-07 R. Brustein , S. P. de Alwis , E. G. Novak

We discuss formation of cosmic strings associated with a spontaneously broken approximate $U(1)$ symmetry by performing classical field-theoretical simulations. An original $U(1)$ symmetry is explicitly broken down to its subgroup $Z_N$…

High Energy Physics - Phenomenology · Physics 2024-10-11 Kohei Fujikura , Mairi Sakellariadou , Michiru Uwabo-Niibo , Masahide Yamaguchi

It is tempting to inflate along one of the many flat directions that arise in supersymmetric theories. The required flatness of the potential to obtain sufficient inflation and to not overproduce density fluctuations occurs naturally.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Katherine Freese , Tony Gherghetta , Hideyuki Umeda

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 study cosmic strings in the complex symmetron model, a scalar-tensor theory with a spontaneously broken local $U(1)$ symmetry in low matter density regions. Using numerical simulations, we show that these strings preferentially attach to…

High Energy Physics - Phenomenology · Physics 2025-08-19 Ali Nezhadsafavi , Levon Pogosian

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

Cosmic strings are one-dimensional topological defects which could have been formed in the early stages of our Universe. They triggered a lot of interest, mainly for their cosmological implications: they could offer an alternative to…

High Energy Physics - Theory · Physics 2009-11-11 Mairi Sakellariadou

We build a number of integrable one--scalar spatially flat cosmologies, which play a natural role in inflationary scenarios, examine their behavior in several cases and draw from them some general lessons on this type of systems, whose…

High Energy Physics - Theory · Physics 2015-06-16 P. Fré , A. Sagnotti , A. S. Sorin

Supersymmetry breaking of a supersymmetric harmonic oscillator with polynomial interaction is analyzed. Some thermal effects are studied in the context of Thermo Field Dynamics (TFD). The restored supersymmetry results in non vanishing…

Quantum Physics · Physics 2018-05-29 C. Marques , GS Dias , FC Khanna , H. S. Chavez

We study the effect of thermal corrections on the evolution of moduli in effective Supergravity models. This is motivated by previous results in the literature suggesting that these corrections could alter and, even, erase the presence of a…

High Energy Physics - Phenomenology · Physics 2009-02-20 T. Barreiro , B. de Carlos , E. J. Copeland , N. J. Nunes

We examine the evolution of cosmological perturbations in a non-thermal post-inflationary history with a late-time matter domination period prior to BBN. Such a cosmology could arise naturally in the well-motivated moduli scenario in the…

High Energy Physics - Phenomenology · Physics 2014-09-05 JiJi Fan , Ogan Ozsoy , Scott Watson

The thermal duality of E(8) x E(8) and SO(32) heterotic string theories may underpin a mechanism that would convert the kinetic energy of infalling matter during gravitational collapse to form a region of a hot string phase that would expel…

High Energy Physics - Theory · Physics 2015-07-07 Michael Hewitt

We present a novel source of dark energy, which is motivated by the prevalence of hidden sectors in string theory models and is consistent with all of the proposed swampland conjectures. Thermal effects hold a light hidden sector scalar at…

High Energy Physics - Theory · Physics 2020-01-08 Edward Hardy , Susha Parameswaran

The dynamics of a symmetry breaking phase transition is studied in a radiation and matter dominated spatially flat FRW cosmology in the large N limit of a scalar field theory.The quantum density matrix is evolved from an initial state of…

High Energy Physics - Phenomenology · Physics 2009-10-31 D. Boyanovsky , H. J. de Vega

The high temperature behaviour of the open bosonic string free energy in the space $S^1 \otimes H^N$ with vanishingly small curvature is investigated. The leading term of the high temperature expansion of the one-loop free energy, near the…

High Energy Physics - Theory · Physics 2009-09-17 A. A. Btysenko , S. D. Odintsov , S. Zerbini

We discuss various issues related to stabilized embedded strings in a thermal background. In particular, we demonstrate that such strings will generically become superconducting at moderately low temperatures, thus enhancing their…

High Energy Physics - Phenomenology · Physics 2009-11-07 Brandon Carter , Robert H. Brandenberger , Anne-Christine Davis

In a recent companion paper, we observed that the rules of ordinary thermodynamics generally fail to respect thermal duality, a symmetry of string theory under which the physics at temperature T is related to the physics at the inverse…

High Energy Physics - Theory · Physics 2009-11-10 Keith R. Dienes , Michael Lennek

We discuss semi-classical string configurations at finite temperature. We find that those soliton solution in the background describing type IIA strings disappear or become divergent when we approach the Hagedorn temperature in the strong…

High Energy Physics - Theory · Physics 2009-05-25 J. D. Madrigal , P. Talavera

We study string theory on $\mathbb{R}^d\times \mathbb{S}^1$. For applications to thermodynamics, the circumference of the $\mathbb{S}^1$ is the inverse temperature, $\beta$. We show that for $d=6$, the low energy effective field theory at…

High Energy Physics - Theory · Physics 2022-04-20 Bruno Balthazar , Jinwei Chu , David Kutasov

In this paper, we investigate thermal equilibrium in string gas cosmology which is dominated by closed string.We consider two interesting regimes, Hagedorn and radiation regimes.We find that for short strings in small radius of Hagedorn…

High Energy Physics - Theory · Physics 2011-07-08 J. Sadeghi , H. Farahani , B. Pourhassan