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Related papers: A Minimal Approach to Baryogenesis via Affleck-Din…

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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

We investigate the Affleck-Dine baryogenesis after D-term inflation with a positive Hubble-induced mass term for a B-L flat direction. It stays at a large field value during D-term inflation, and just after inflation ends it starts to…

High Energy Physics - Phenomenology · Physics 2015-04-16 Masahiro Kawasaki , Masaki Yamada

We propose a novel and minimal setup where the observed baryon asymmetry of the Universe and neutrino oscillation data can be satisfied with only one right-handed neutrino (RHN) and a second Higgs doublet with the latter being also…

High Energy Physics - Phenomenology · Physics 2026-04-22 Disha Bandyopadhyay , Debasish Borah , Suruj Jyoti Das , Nobuchika Okada

Thermal inflation is an attractive idea to dilute cosmic density of unwanted particles such as moduli fields which cause cosmological difficulties. However, it also dilutes preexisting baryon asymmetry and some viable baryogenesis is…

High Energy Physics - Phenomenology · Physics 2016-04-06 Taku Hayakawa , Masahiro Kawasaki , Masaki Yamada

Constructing models of inflation and/or baryogenesis in the context of N=1 supergravity is known to be difficult as the finite energy density during inflation typically generates large (order the Hubble scale) mass terms. This is the…

High Energy Physics - Phenomenology · Physics 2015-06-16 Marcos A. G. Garcia , Keith A. Olive

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

The Affleck-Dine mechanism creates the baryon asymmetry of the universe from an angular motion of a complex scalar field. The mechanism is efficient and allows for a low reheating temperature of the universe if the scalar field has a flat…

High Energy Physics - Phenomenology · Physics 2019-09-04 Keisuke Harigaya

We consider the possibility of a successful Affleck-Dine mechanism along the u^c d^c d^c direction in R-parity symmetric extensions of the minimal supersymmetric Standard Model (MSSM) which contain a gauge singlet superfield phi. Such gauge…

High Energy Physics - Phenomenology · Physics 2009-10-28 J. McDonald

In this letter we explore the possibility of creating the baryon asymmetry of the universe during inflation and reheating due to the decay of a field associated with the inflaton. CP violation is attained by assuming that this field is…

High Energy Physics - Phenomenology · Physics 2014-11-17 D. V. Nanopoulos , Raghavan Rangarajan

String theory generically predicts the coupling between the Affleck-Dine field and axion field through higher-dimensional operators. We thus explore the Affleck-Dine baryogenesis on an axion background. It turns out that the axion…

High Energy Physics - Phenomenology · Physics 2017-04-28 Kensuke Akita , Tatsuo Kobayashi , Hajime Otsuka

The phenomenology of supersymmetric models of inflation, where the inflationary vacuum energy is dominated by D-terms of a U(1), is investigated. Particular attention is paid to the questions of how to arrange for sufficient e-folds of…

High Energy Physics - Phenomenology · Physics 2009-10-31 Christopher Kolda , John March-Russell

We study Affleck-Dine leptogenesis via the L H_u flat direction in supersymmetric theories. We find that the baryon asymmetry is enhanced when the energy scale of the inflation is sufficiently low. Especially, we consider models of low…

High Energy Physics - Phenomenology · Physics 2009-11-07 T. Asaka

We evaluate the constraints that the COBE observations put on baryogenesis in inflationary cosmologies.We consider the supersymmetric version of the proposal of Fukugita and Yanagida, that the baryon asymmetry of the universe is created by…

High Energy Physics - Phenomenology · Physics 2009-09-15 B. A. Campbell , S. Davidson , K. A. Olive

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 the baryon asymmetry of the universe is explained in the framework of the supersymmetric extension of the Standard Model with R-parity violating interactions. It is shown that the Affleck-Dine mechanism naturally…

High Energy Physics - Phenomenology · Physics 2014-08-05 Tetsutaro Higaki , Kazunori Nakayama , Ken'ichi Saikawa , Tomo Takahashi , Masahide Yamaguchi

The dynamics at the end of inflation can generate an asymmetry between particles and anti-particles of the inflaton field. This asymmetry can be transferred to baryons via decays, generating a baryon asymmetry in our Universe. We explore…

High Energy Physics - Phenomenology · Physics 2014-12-05 Kaloian D. Lozanov , Mustafa A. Amin

We study an inflection point inflation scenario where a flat direction of the minimal supersymmetric standard model (MSSM) is identified with the inflaton. We focus on the case where the flat direction (inflaton) has non-zero baryon number,…

High Energy Physics - Phenomenology · Physics 2024-10-17 Naoyuki Haba , Yasuhiro Shimizu , Yoshihiro Tanabe , Toshifumi Yamada

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

We study the dynamics of the Affleck-Dine field after inflation in more detail. After inflation, the Affleck-Dine field inevitably oscillates around the potential minimum. This oscillation is hard to decay and can cause accidental…

High Energy Physics - Phenomenology · Physics 2017-09-27 Fuminori Hasegawa , Masahiro Kawasaki

We describe a simple and predictive scenario for baryogenesis in theories with large extra dimensions which resembles Affleck-Dine baryogenesis. The Affleck-Dine field is a complex scalar field carrying a $U(1)_{\chi}$ charge which is…

High Energy Physics - Phenomenology · Physics 2009-11-07 Rouzbeh Allahverdi , Kari Enqvist , Anupam Mazumdar , Abdel Pérez-Lorenzana