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Related papers: Dilaton Destabilization at High Temperature

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Topological defects can have significant cosmological consequences, so their production must be examined carefully. It is usually assumed that topological defects are produced if the temperature becomes sufficiently high, but in reality…

High Energy Physics - Phenomenology · Physics 2026-01-19 Junseok Lee , Kai Murai , Kazunori Nakayama , Fuminobu Takahashi

For supersymmetric theories with gravitino dark matter, the maximal reheating temperature consistent with big bang nucleosynthesis bounds arises when the physical gaugino masses are degenerate. We consider the cases of a stau or sneutrino…

High Energy Physics - Phenomenology · Physics 2009-12-15 Marek Olechowski , Stefan Pokorski , Krzysztof Turzynski , James D. Wells

If SU(N) gauge fields live in a world with a circular extra dimension, coupling there only to adjointly charged matter, the system possesses a global Z(N) symmetry. If the radius is small enough such that dimensional reduction takes place,…

High Energy Physics - Phenomenology · Physics 2009-11-07 K. Farakos , P. de Forcrand , C. P. Korthals Altes , M. Laine , M. Vettorazzo

Late-time entropy production from scalar decay arises in scenarios like thermal inflation, proposed to dilute long-lived, massive fields like the gravitino and the moduli. The scalar decay may continue into Mev-scale temperatures and affect…

High Energy Physics - Phenomenology · Physics 2007-05-23 Paramita Adhya , D. Rai Chaudhuri

The theory of inflation will be investigated as well as supersymmetry breaking in the context of supergravity, incorporating the target-space duality and the nonperturbative gaugino condensation in the hidden sector. We found an…

High Energy Physics - Phenomenology · Physics 2014-11-17 Mitsuo J. Hayashi , Tomoki Watanabe , Ichiro Aizawa , Koichi Aketo

We investigate preheating in a higher-dimensional generalized Kaluza-Klein theory with a quadratic inflaton potential $V(\phi)=\frac12 m^2\phi^2$ including metric perturbations explicitly. The system we consider is the multi-field model…

High Energy Physics - Phenomenology · Physics 2009-10-31 S. Tsujikawa

It is shown that in quantum gravity at finite temperature, the effective potential evaluated in the tadpole approximation can have a local minimum below a certain critical temperature. However, when the leading higher order thermal loop…

High Energy Physics - Theory · Physics 2008-11-26 F. T. Brandt , J. Frenkel

We study the dilaton stabilization in the D-brane world in which a D-brane constitutes our universe. The dilaton can be stabilized due to the interplay between the D-brane tension and the negative scalar curvature of extra dimensions.…

High Energy Physics - Theory · Physics 2009-11-11 Hang Bae Kim

We analyse the high temperature behaviour of softly broken supersymmetric theories taking into account the role played by effective non-renormalizable terms generated by the decoupling of superheavy degrees of freedom or the Planck scale…

High Energy Physics - Phenomenology · Physics 2009-10-28 Gia Dvali , K. Tamvakis

We formulate new conformal models of inflation and dark energy which generalise the Higgs-Dilaton scenario. We embed these models in unimodular gravity whose effect is to break scale invariance in the late time Universe. In the early…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 P. Brax , A. C. Davis

There are at least two serious moduli problems in string cosmology. The first is the possibility that moduli dominate the energy density at the time of nucleosynthesis. The second is that they may not find their minima all together. After…

High Energy Physics - Theory · Physics 2009-10-31 Michael Dine

Considering gravitino dark matter scenarios, we study constraints on the reheating temperature of inflation. We present the gauge-invariant result for the thermally produced gravitino yield to leading order in the Standard Model gauge…

High Energy Physics - Phenomenology · Physics 2008-11-26 Josef Pradler , Frank Daniel Steffen

We present a modular cosmology scenario where the difficulties encountered in conventional modular cosmology are solved in a self-consistent manner, with definite predictions to be tested by observation. Notably, the difficulty of the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kenji Kadota , Ewan D. Stewart

Using the linear multiplet formulation for the dilaton superfield, we construct an effective lagrangian for hidden-sector gaugino condensation in string effective field theories with arbitrary gauge groups and matter. Nonperturbative string…

High Energy Physics - Theory · Physics 2009-10-30 Pierre Binetruy , Mary K. Gaillard , Yi-Yen Wu

Moduli, modulini and the gravitino have gravitational-strength interactions, and thermal collisions after reheating create all of them with roughly the same abundance. With their mass of order $100\GeV$, corresponding to gravity-mediated…

High Energy Physics - Phenomenology · Physics 2009-10-31 David H. Lyth

We consider the low energy phenomenology of superstrings. In particular we analyse supersymmetry breaking via gaugino condensate and we compare the phenomenology of the two different approaches to stabilize the dilaton field. We study the…

High Energy Physics - Phenomenology · Physics 2016-09-01 Axel de la Macorra

We show the existence of a general mechanism by which heavy scalar fields can be destabilized during inflation, relying on the fact that the curvature of the field space manifold can dominate the stabilizing force from the potential and…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-05 Sébastien Renaux-Petel , Krzysztof Turzyński

We study in a systematic and modular invariant way gaugino condensation in the hidden sector as a potential source of hierarchical supersymmetry breaking and a non--trivial potential for the dilaton $S$ whose real part corresponds to the…

High Energy Physics - Theory · Physics 2009-10-29 B. de Carlos , J. A. Casas , C. Muñoz

The end of inflation is connected to the standard cosmological scenario through reheating. During reheating, the inflaton oscillates around the minimum of the potential and thus decays into the daughter particles that populate the Universe…

General Relativity and Quantum Cosmology · Physics 2016-10-19 R. Kabir , A. Mukherjee , D. Lohiya

We show that the reheating temperature of a matter-domination era in the early universe can be pushed down to the neutrino decoupling temperature at around $2 \ {\rm MeV}$ if the reheating takes place through non-hadronic decays of the…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-11 Gabriela Barenboim , Wan-Il Park