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Within the context of supersymmetric hybrid inflation, we study a multiple-stage inflationary scenario that can generate a primordial spectrum of adiabatic density perturbations with a break at $k_b \simeq 0.05 h Mpc^{-1}$. The presence of…

高能物理 - 唯象学 · 物理学 2007-05-23 Mairi Sakellariadou , Nikos Tetradis

Adams et al. (1997b) have noted that according to our current understanding of the unification of fundamental interactions, there should have been phase transitions associated with spontaneous symmetry breaking {\em during} the inflationary…

天体物理学 · 物理学 2008-11-26 Jose Barriga , Enrique Gaztanaga , Mario Santos , Subir Sarkar

Two extensions of ideas lying in the basis of the inflationary scenario of the early Universe and their effect on the large scale structure of the present-day Universe are discussed. The first of them is the possibility of fast phase…

天体物理学 · 物理学 2007-05-23 A. A. Starobinsky

A scenario with two subsequent periods of inflationary expansion in the very early universe is examined. The model is based on a potential motivated by symmetries being found in field theory at high energy. For various parameter sets of the…

宇宙学与河外天体物理 · 物理学 2016-01-13 Simon Schettler , Jurgen Schaffner-Bielich

Observations of anisotropies in the cosmic microwave background by the Wilkinson Microwave Anisotropy Probe suggest the possibility of oscillations in the primordial density perturbation. Such deviations from the usually assumed scale-free…

天体物理学 · 物理学 2011-02-16 Paul Hunt , Subir Sarkar

We explore the possibility that a multiple-stage inflationary scenario based on supersymmetric GUT models, can account for the break at $k_b \simeq 0.05 h/Mpc$ in the power spectrum of galaxy clustering, while it reproduces the angular…

高能物理 - 唯象学 · 物理学 2009-10-31 Mairi Sakellariadou

Forthcoming missions probing the absolute intensity of the CMB are expected to be able to measure spectral distortions, which are deviations from its blackbody distribution. As cosmic inflation can induce spectral distortions, these…

宇宙学与河外天体物理 · 物理学 2024-04-22 Alexander Baur , Marcos A. G. Garcia , Raul Henriquez-Ortiz , Mauricio Hernandez-Neri , Saul Ramos-Sanchez

If the conformal invariance of electromagnetism is broken during inflation, then primordial magnetic fields may be produced. If this symmetry breaking is generated by the coupling between electromagnetism and a scalar field---e.g. the…

宇宙学与河外天体物理 · 物理学 2013-05-29 Robert R. Caldwell , Leonardo Motta , Marc Kamionkowski

Supersymmetric hybrid inflation is an exquisite framework to connect inflationary cosmology to particle physics at the scale of grand unification. Ending in a phase transition associated with spontaneous symmetry breaking, it can naturally…

高能物理 - 唯象学 · 物理学 2014-07-31 Wilfried Buchmuller , Valerie Domcke , Kohei Kamada , Kai Schmitz

It is conjectured that inflation, taking account of quantum gravity, leads to a discrete spectrum of cosmological perturbations, instead of the continuous Gaussian spectrum predicted by standard field theory in an unquantized background.…

天体物理学 · 物理学 2009-11-10 Craig J. Hogan

In effective supergravity theories following from the superstring, a modulus field can quite naturally set the neccessary initial conditions for successful cosmological inflation to be driven by a hidden sector scalar field. The leading…

高能物理 - 唯象学 · 物理学 2007-05-23 Subir Sarkar

Recently, there has been some interest for building supersymmetric models of double inflation. These models, realistic from a particle physics point of view, predict a broken-scale-invariant power spectrum of primordial cosmological…

高能物理 - 唯象学 · 物理学 2014-11-17 Julien Lesgourgues

We study thermally induced density perturbations during inflation. This scenario is characterized by two thermodynamical conditions: (1) The primordial perturbations originate in the epoch when the inflationary universe contains a…

天体物理学 · 物理学 2009-10-30 Wolung Lee , Li-Zhi Fang

We study the generation of the primordial curvature perturbation in multi-field inflation. Considering both the evolution of the perturbation during inflation and the effects generated at the end of inflation, we present a general formula…

宇宙学与河外天体物理 · 物理学 2015-06-04 Ki-Young Choi , Soo A Kim , Bumseok Kyae

Inflation arises in supersymmetric grand unified theories (susy GUTs) without fine tuning and cosmic strings usually form at the end of inflation. Hence both strings and inflation contribute to the density perturbations in the very early…

高能物理 - 唯象学 · 物理学 2016-10-26 R. Jeannerot

We present a model with a complex and a real scalar fields and a potential whose symmetry is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe…

天体物理学 · 物理学 2007-05-23 Gabriel Zsembinszki

We study a model of inflation with multiple pseudo-scalar fields coupled to a $U(1)$ gauge field through Chern-Simons interactions. Because of parity violating interactions, one polarization of the gauge field is amplified yielding to…

宇宙学与河外天体物理 · 物理学 2023-05-12 Alireza Talebian , Seyed Ali Hosseini Mansoori , Hassan Firouzjahi

I elaborate on a link between the string--scale breaking of supersymmetry that occurs in a class of superstring models and the onset of inflation. The link rests on spatially flat cosmologies supported by a scalar field driven by an…

高能物理 - 理论 · 物理学 2013-07-10 A. Sagnotti

Theories with elementary scalar degrees of freedom seem nowadays required for simple descriptions of the Standard Model and of the Early Universe. It is then natural to embed theories of inflation in supergravity, also in view of their…

高能物理 - 理论 · 物理学 2015-09-30 S. Ferrara , A. Sagnotti

Models of cosmic inflation suggest that our universe underwent an early phase of accelerated expansion, driven by the dynamics of one or more scalar fields. Inflationary models make specific, quantitative predictions for several observable…

宇宙学与河外天体物理 · 物理学 2016-05-10 David I. Kaiser
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