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We consider the formation of topological defects after inflation. In order to take into account the effects of the rescattering of fluctuations, we integrate the classical equation that describes the evolution of a complex scalar field on…

High Energy Physics - Phenomenology · Physics 2009-10-31 S. Kasuya , M. Kawasaki

Topological defects can be formed during inflation by phase transitions as well as by quantum nucleation. We study the effect of the expansion of the Universe on the internal structure of the defects. We look for stationary solutions to the…

General Relativity and Quantum Cosmology · Physics 2010-11-01 R. Basu , A. Vilenkin

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

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

We investigate the possibility of preheating in hybrid inflation. This scenario involves at least two scalar fields, the inflaton field $\phi$, and the symmetry breaking field $\sigma$. We found that the behavior of these fields after…

High Energy Physics - Phenomenology · Physics 2009-09-29 Juan Garcia-Bellido , Andrei Linde

We describe a novel phenomenon in which vortices are produced due to resonant oscillations of a scalar field which is driven by a periodically varying temperature T, with T remaining much below the critical temperature $T_c$. Also, in a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Sanatan Digal , Rajarshi Ray , Supratim Sengupta , Ajit M. Srivastava

Currently favoured extensions of the Standard Model typically contain `flaton fields' defined as fields with large vacuum expectation values (vevs) and almost flat potentials. If a flaton field is trapped at the origin in the early…

High Energy Physics - Phenomenology · Physics 2009-10-28 Tiago Barreiro , E. J. Copeland , David H. Lyth , Tomislav Prokopec

At the first stage of reheating after inflation, parametric resonance may rapidly transfer most of the energy of an inflaton field $\phi$ to the energy of other bosons. We show that quantum fluctuations of scalar and vector fields produced…

High Energy Physics - Theory · Physics 2009-09-29 Lev Kofman , Andrei Linde , Alexei A. Starobinsky

We numerically investigate the decay, via parametric resonance, of the inflaton with an m^2 phi^2 potential into a scalar matter field with a symmetry breaking potential. We consider the case where symmetry breaking takes place during…

High Energy Physics - Phenomenology · Physics 2016-08-25 M. F. Parry , A. T. Sornborger

We consider the generation of super-horizon metric fluctuations during an epoch of preheating in the presence of a scalar field \chi quadratically coupled to the inflaton. We find that the requirement of efficient broad resonance is…

High Energy Physics - Phenomenology · Physics 2009-10-31 Karsten Jedamzik , Guenter Sigl

Preheating after inflation may lead to nonthermal phase transitions with symmetry restoration. These phase transitions may occur even if the total energy density of fluctuations produced during reheating is relatively small as compared with…

High Energy Physics - Phenomenology · Physics 2009-10-31 Gary Felder , Lev Kofman , Andrei Linde , Igor Tkachev

Inflation can occur in the cores of topological defects, where the scalar field is forced to stay near the maximum of its potential. This topological inflation does not require fine-tuning of the initial conditions.

High Energy Physics - Theory · Physics 2010-11-01 Alexander Vilenkin

We consider the generation of the scalar mode of the metric perturbations during preheating stage in a two field model with the potential $V(\phi, \chi)= {m^{2}\phi^{2}\over 2}+{g^{2}\phi^{2}\chi^{2}\over 2}$. We discuss two possible…

Astrophysics · Physics 2016-08-25 Pavel Ivanov

In higher-curvature inflation models ($R+\alpha_n R^n$), we study a parametric preheating of a scalar field $\chi$ coupled non-minimally to a spacetime curvature $R$ ($\xi R \chi^2$). In the case of $R^2$-inflation model, efficient…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Tsujikawa , K. Maeda , T. Torii

We show that the primordial curvature perturbations may originate not from the quantum fluctuations of inflaton during inflation but from isocurvature perturbations which are amplified during preheating after inflation. We consider a simple…

Astrophysics · Physics 2008-11-26 Teruaki Suyama , Shuichiro Yokoyama

In the context of supersymmetric models, we analyze the production of topological defects at the end of inflation driven by a conjugate pair of inflaton fields which are non-singlets under the continuous symmetry group of the theory. We…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides , Q. Shafi

Fluctuations of scalar fields produced at the stage of preheating after inflation are so large that they can break supersymmetry much stronger than inflation itself. These fluctuations may lead to symmetry restoration along flat directions…

High Energy Physics - Phenomenology · Physics 2009-09-29 Greg. W. Anderson , Andrei Linde , Antonio Riotto

We study the dynamics of topological defects in the context of ``topological inflation" proposed by Vilenkin and Linde independently. Analysing the time evolution of planar domain walls and of global monopoles, we find that the defects…

General Relativity and Quantum Cosmology · Physics 2014-11-17 Nobuyuki Sakai , Hisa-aki Shinkai , Takashi Tachizawa , Kei-ichi Maeda

We study chaotic dynamics in preheating after inflation in which an inflaton $\phi$ is coupled to another scalar field $\chi$ through an interaction $(1/2)g^2\phi^2\chi^2$. We first estimate the size of the quasi-homogeneous field $\chi$ at…

High Energy Physics - Phenomenology · Physics 2009-11-10 Yoshida Jin , Shinji Tsujikawa

During the last ten years a detailed investigation of preheating was performed for chaotic inflation and for hybrid inflation. However, nonperturbative effects during reheating in the new inflation scenario remained practically unexplored.…

High Energy Physics - Theory · Physics 2009-09-29 Mariel Desroche , Gary N. Felder , Jan M. Kratochvil , Andrei Linde
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