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(c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
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Nakayama, Kazunori; Takahashi, Fuminobu; Yanagida, Tsutomu T., E-mail: kazunori@hep-th.phys.s.u-tokyo.ac.jp
arXiv e-print [ PDF ]2013
arXiv e-print [ PDF ]2013
AbstractAbstract
[en] We propose a chaotic inflation model in supergravity based on polynomial interactions of the inflaton. Specifically we study the chaotic inflation model with quadratic, cubic and quartic couplings in the scalar potential and show that the predicted scalar spectral index and tensor-to-scalar ratio can lie within the 1σ region allowed by the Planck results
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S0370-2693(13)00525-X; Available from http://dx.doi.org/10.1016/j.physletb.2013.06.050; Copyright (c) 2013 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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[en] We use the Melnikov method to identify chaotic behavior in geodesic motion perturbed by the minimal length effects around a Schwarzschild black hole. Unlike the integrable unperturbed geodesic motion, our results show that the perturbed homoclinic orbit, which is a geodesic joining the unstable circular orbit to itself, becomes chaotic in the sense that Smale horseshoes chaotic structure is present in phase space.
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Available from: http://dx.doi.org/10.1140/epjc/s10052-020-8335-6; AID: 745
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European Physical Journal. C, Particles and Fields (Online); ISSN 1434-6052;
; CODEN EPCFFB; v. 80(8); p. 1-7

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[en] We reconstruct scalar field theories to realize inflation compatible with the BICEP2 result as well as the Planck. In particular, we examine the chaotic inflation model, natural (or axion) inflation model, and an inflationary model with a hyperbolic inflaton potential. We perform an explicit approach to find out a scalar field model of inflation in which any observations can be explained in principle
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S0370-2693(14)00664-9; Available from http://dx.doi.org/10.1016/j.physletb.2014.09.014; Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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Shaghoulian, Edgar; Wang, Huajia, E-mail: eshaghoulian@gmail.com2016
AbstractAbstract
[en] We study the nature of a family of curvature singularities which are precisely the timelike cousins of the spacelike singularities studied by Belinski, Khalatnikov, and Lifshitz (BKL). We show that the approach to the singularity can be modeled by a billiard ball problem on hyperbolic space, just as in the case of BKL. For pure gravity, generic chaotic behavior is retained in (3 + 1) dimensions, and we provide evidence that it disappears in higher dimensions. We speculate that such singularities, if occurring in AdS/CFT and of the chaotic variety, may be interpreted as (transient) chaotic renormalization group flows which exhibit features reminiscent of chaotic duality cascades. (paper)
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Available from http://dx.doi.org/10.1088/0264-9381/33/12/125020; Country of input: International Atomic Energy Agency (IAEA)
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[en] A new large deviation property for the Lempel-Ziv complexity is numerically studied by using a one-dimesional non-hyperbolic 'modified Bernoulli map', where the transition between stationary and non-stationary chaos is clearly observed. We will show that the Lempel-Ziv complexity and its fluctuations obey the universal scaling laws, and that the Lempel-Ziv complexity has the L1-function property of the infinite ergodic theory. One of the most striking results is that the 1/f spectral process reveals the maximum diversity at the transition point from the stationary chaos to the non-stationary one
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3. 21COE symposium on astrophysics as interdisciplinary science; Tokyo (Japan); 1-3 Sep 2005; Available online at http://stacks.iop.org/1742-6596/31/213/jpconf6_31_059.pdf or at the Web site for the Journal of Physics. Conference Series (Online) (ISSN 1742-6596) http://www.iop.org/; Country of input: International Atomic Energy Agency (IAEA)
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Journal of Physics. Conference Series (Online); ISSN 1742-6596;
; v. 31(1); p. 213-214

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Nakayama, Kazunori; Saikawa, Ken’ichi; Terada, Takahiro; Yamaguchi, Masahide
Funding organisation: SCOAP3, CERN, Geneva (Switzerland)
arXiv e-print [ PDF ]2016
Funding organisation: SCOAP3, CERN, Geneva (Switzerland)
arXiv e-print [ PDF ]2016
AbstractAbstract
[en] Minimal chaotic models of D-term inflation predicts too large primordial tensor perturbations. Although it can be made consistent with observations utilizing higher order terms in the Kähler potential, expansion is not controlled in the absence of symmetries. We comprehensively study the conditions of Kähler potential for D-term plateau-type potentials and discuss its symmetry. They include the α-attractor model with a massive vector supermultiplet and its generalization leading to pole inflation of arbitrary order. We extend the models so that it can describe Coulomb phase, gauge anomaly is cancelled, and fields other than inflaton are stabilized during inflation. We also point out a generic issue for large-field D-term inflation that the masses of the non-inflaton fields tend to exceed the Planck scale.
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Available from http://dx.doi.org/10.1007/JHEP05(2016)067; Available from http://repo.scoap3.org/record/15578; PUBLISHER-ID: JHEP05(2016)067; ARXIV:1603.02557; OAI: oai:repo.scoap3.org:15578; Copyright (c) OPEN ACCESS, © The Authors; This article is distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/) (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.; Country of input: International Atomic Energy Agency (IAEA)
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Journal of High Energy Physics (Online); ISSN 1029-8479;
; v. 2016(05); p. 67

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[en] We show how backreaction of the inflaton potential energy on heavy scalar fields can flatten the inflationary potential, as the heavy fields adjust to their most energetically favorable configuration. This mechanism operates in previous UV-complete examples of axion monodromy inflation--flattening a would-be quadratic potential to one linear in the inflaton field--but occurs more generally, and we illustrate the effect with several examples. Special choices of compactification minimizing backreaction may realize chaotic inflation with a quadratic potential, but we argue that a flatter potential such as power-law inflation V(φ)∝φp with p<2 is a more generic option at sufficiently large values of φ.
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(c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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[en] Chaotic strings are a class of non-hyperbolic coupled map lattices, exhibiting a rich structure of complex dynamical phenomena with a surprising correspondence to physical contents. In this paper we introduce different types and models for chaotic strings, where 2B-strings with finite length are considered in detail. We demonstrate possibilities to extract renormalized quantities, which are expected to describe essential properties of the string.
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QQQ Conference 2012: 6. ECM satellite QQQQ Conference 3Quantum: Algebra Geometry Information; Talinn (Estonia); 10-13 Jul 2012; Available from http://dx.doi.org/10.1088/1742-6596/532/1/012008; Country of input: International Atomic Energy Agency (IAEA)
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Journal of Physics. Conference Series (Online); ISSN 1742-6596;
; v. 532(1); [9 p.]

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[en] We consider the effects of the curvaton, late-decaying scalar condensation, to observational constraints on inflation models. From current observations of cosmic density fluctuations, severe constraints on some classes of inflation models are obtained, in particular, on the chaotic inflation with higher-power monomials, the natural inflation, and the new inflation. We study how the curvaton scenario changes (and relaxes) the constraints on these models
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(c) 2005 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
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