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Related papers: Affleck-Dine baryogenesis with modulated reheating

200 papers

We examine the viability of the Affleck-Dine mechanism for baryogenesis under radiatively induced running of soft breaking $({\rm mass})^2$ of the flat directions stemming from non-zero energy density of the inflaton during inflation. A…

High Energy Physics - Phenomenology · Physics 2009-11-07 Rouzbeh Allahverdi , Manuel Drees , Anupam Mazumdar

In this paper, we investigate the parameter space in the framework of hilltop supernatural inflation in which the inflaton field can play the role of Affleck-Dine field to produce successful baryogenesis. The suitable value of reheating…

High Energy Physics - Phenomenology · Physics 2020-08-19 Chia-Min Lin , Kazunori Kohri

We investigate whether a recently proposed modulation of the power spectrum of primordial density fluctuations generated through transplankian (maybe stringy) effects during inflation can be observed. We briefly review the mechanism leading…

High Energy Physics - Theory · Physics 2014-11-18 L. Bergstrom , U. H. Danielsson

The classical picture of GUT baryogenesis has been strongly modified by theoretical progress concerning two nonperturbative features of the standard model: the phase diagram of the electroweak theory, and baryon and lepton number changing…

High Energy Physics - Phenomenology · Physics 2011-11-10 Wilfried Buchmüller

A generic feature of the known string inflationary models is that the same physics that makes the inflaton lighter than the Hubble scale during inflation often also makes other scalars this light. These scalars can acquire isocurvature…

High Energy Physics - Theory · Physics 2015-06-04 M. Cicoli , G. Tasinato , I. Zavala , C. P. Burgess , F. Quevedo

We investigate the non-Gaussianity of primordial curvature perturbation in the modulated reheating scenario where the primordial perturbation is generated due to the spacial fluctuation of the inflaton decay rate to radiation. We use the…

Astrophysics · Physics 2008-11-26 Teruaki Suyama , Masahide Yamaguchi

In the modulated reheating scenario, the field that drives inflation has a spatially varying decay rate, and the resulting inhomogeneous reheating process generates adiabatic perturbations. We examine the statistical properties of the…

Cosmology and Nongalactic Astrophysics · Physics 2014-01-28 Naoya Kobayashi , Takeshi Kobayashi , Adrienne L. Erickcek

We study a scenario that large non-Gaussianity arises from the baryon asymmetry of the Universe. There are baryogenesis scenarios containing a light scalar field, which may result in baryonic isocurvature perturbations with some amount of…

High Energy Physics - Phenomenology · Physics 2009-01-14 Masahiro Kawasaki , Kazunori Nakayama , Fuminobu Takahashi

The scalar mode density perturbations in a the warm inflationary scenario are analysed with a view to predicting the amount of non-gaussianity produced by this scenario. The analysis assumes that the inflaton evolution is strongly damped by…

Astrophysics · Physics 2010-10-27 Ian G Moss , Chun Xiong

Previously, we proposed a model of low energy Affleck-Dine leptogenesis in the context of thermal inflation. The lepton asymmetry is generated at the end of thermal inflation, which occurs at a relatively low energy scale with the Hubble…

High Energy Physics - Phenomenology · Physics 2010-10-27 Gary N. Felder , Hyunbyuk Kim , Wan-Il Park , Ewan D. Stewart

We introduce a class of non-supersymmetric models explaining baryogenesis a la Affleck-Dine, which use a decay of two superheavy scalar fields with close masses. These scalars acquire non-zero expectation values during inflation through…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-08 Eugeny Babichev , Dmitry Gorbunov , Sabir Ramazanov

In D-term inflation models, the fluctuations of squark fields in the flat directions give rise to isocurvature density fluctuations stored in the Affleck-Dine condensate. After the condensate breaks up in B-balls, these can be perturbations…

High Energy Physics - Phenomenology · Physics 2007-05-23 Kari Enqvist

There are many flat directions in SUSY models, which may dissipate their energy and source the radiation background during inflation. However, the only possibility that has been studied in this direction is warm inflation, which uses "warm"…

High Energy Physics - Phenomenology · Physics 2010-01-26 Tomohiro Matsuda

We present a novel Affleck-Dine scenario for the generation of the observed baryon asymmetry of the Universe based on the non-trivial interplay between quintessential inflationary models containing a kinetic dominated post-inflationary era…

Cosmology and Nongalactic Astrophysics · Physics 2018-07-30 Dario Bettoni , Javier Rubio

Within the framework of RG improved inflationary cosmology motivated by asymptotically safe gravity, we study the dynamics of a scalar field which can be interpreted as the Higgs field. The background trajectories of this model can provide…

High Energy Physics - Theory · Physics 2013-10-16 Yi-Fu Cai , Yu-Chiao Chang , Pisin Chen , Damien A. Easson , Taotao Qiu

For Affleck-Dine baryogenesis to proceed, there must have been two types of phase transitions. One is the destabilized-stabilized phase transition of the flat direction, which is in general induced by the Hubble parameter. The other is the…

High Energy Physics - Phenomenology · Physics 2016-09-06 Tomohiro Matsuda

Reheating is the the epoch which connects inflation to the subsequent hot Big-Bang phase. Conceptually very important, this era is however observationally poorly known. We show that the current Planck satellite measurements of the Cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2015-10-08 Jerome Martin , Christophe Ringeval , Vincent Vennin

Recent observations from the Atacama Cosmology Telescope (ACT) indicate a moderate upward shift in the scalar spectral index $n_s$ compared to Planck $2018$, thereby placing tighter constraints on inflationary scenarios. Motivated by these…

Cosmology and Nongalactic Astrophysics · Physics 2025-08-25 Li-Yang Chen , Rongrong Zha , Feng-Yi Zhang

We consider the Affleck-Dine baryogenesis comprehensively in the minimal supersymmetric standard model with gauge-mediated supersymmetry breaking. Considering the high temperature effects, we see that the Affleck-Dine field is naturally…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. Kasuya

Thermal inflation can solve serious cosmological problems such as overproduction of gravitinos and moduli. However, it also dilutes the preexisting baryon asymmetry. We investigate a possibility that Affleck-Dine mechanism works after…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masahiro Kawasaki , Kazunori Nakayama