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Supersymmetry is generally broken by the non-vanishing vacuum energy density present during inflation. In supergravity models, such a source of supersymmetry breaking typically makes a contribution to scalar masses of order ${\tilde m}^2…

高能物理 - 唯象学 · 物理学 2009-09-15 Mary K. Gaillard , Hitoshi Murayama , Keith A. Olive

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…

高能物理 - 唯象学 · 物理学 2016-04-06 Taku Hayakawa , Masahiro Kawasaki , Masaki Yamada

Baryogenesis from the coherent production of a scalar condensate along a flat direction of the supersymmetric extension of the standard model (Affleck-Dine mechanism) is investigated. Two important effects are emphasized. First,…

高能物理 - 唯象学 · 物理学 2009-09-15 Michael Dine , Lisa Randall , Scott Thomas

Supersymmetry breaking in the early universe induces scalar soft potentials with curvature of order the Hubble constant. This has a dramatic effect on the coherent production of scalar fields along flat directions. For the moduli problem it…

高能物理 - 唯象学 · 物理学 2016-09-01 Michael Dine , Lisa Randall , Scott Thomas

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…

高能物理 - 唯象学 · 物理学 2009-09-29 Greg. W. Anderson , Andrei Linde , Antonio Riotto

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…

高能物理 - 唯象学 · 物理学 2015-06-16 Marcos A. G. Garcia , Keith A. Olive

We show that a baryon asymmetry can be generated by dissipative effects during warm inflation via a supersymmetric two-stage mechanism, where the inflaton is coupled to heavy mediator fields that then decay into light species through B- and…

高能物理 - 唯象学 · 物理学 2015-05-30 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa

A variation of Affleck-Dine mechanism was proposed to generate the observed baryon asymmetry in [1], in which the inflaton was assumed to be a complex scalar field with a weakly broken $U(1)$ symmetry, and the baryon asymmetry generation…

宇宙学与河外天体物理 · 物理学 2015-06-22 Nan Li , Ding-fang Zeng

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…

高能物理 - 唯象学 · 物理学 2009-11-07 T. Asaka

We consider a possibility that one of the flat directions in the minimal supersymmetric standard model plays the role of the inflaton field and realizes large-field inflation. This is achieved by introducing a generalized shift symmetry on…

高能物理 - 唯象学 · 物理学 2015-06-19 Shinta Kasuya , Fuminobu Takahashi

We study the cosmology of supersymmetric models in which the supersymmetry breaking effects are mediated by gauge interactions at about the 10^5 GeV scale. We first point out that the gravitino is likely to overclose the Universe in this…

高能物理 - 唯象学 · 物理学 2009-09-29 Andre de Gouvea , Takeo Moroi , Hitoshi Murayama

We argue that an extension of the Minimal Supersymmetric Standard Model that gives rise to viable thermal inflation, and so does not suffer from a Polonyi/moduli problem, should contain right-handed neutrinos which acquire their masses due…

高能物理 - 唯象学 · 物理学 2009-10-28 E. D. Stewart , M. Kawasaki , T. Yanagida

We propose a new scenario of Affleck-Dine baryogenesis where a flat direction in the MSSM generates B-L asymmetry just after the end of inflation. The resulting amount of baryon asymmetry is independent of low-energy supersymmetric models…

高能物理 - 唯象学 · 物理学 2016-04-27 Masaki Yamada

It is shown that, in the context of split supersymmetry, a simple model with a single complex scalar field can produce chaotic inflation and generate the observed amount of baryon asymmetry via the Affleck-Dine mechanism. While the inflaton…

高能物理 - 唯象学 · 物理学 2009-11-06 Yeo-Yie Charng , Da-Shin Lee , Chung Ngoc Leung , Kin-Wang Ng

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,…

高能物理 - 唯象学 · 物理学 2024-10-17 Naoyuki Haba , Yasuhiro Shimizu , Yoshihiro Tanabe , Toshifumi Yamada

The generation of the baryon asymmetry of the Universe (BAU) from the hypermagnetic helicity, the physical interpretation of which is given in terms of hypermagnetic knots, is studied in inflationary cosmology, taking into account the…

高能物理 - 唯象学 · 物理学 2008-11-26 Kazuharu Bamba

We propose a mechanism by which the inflaton can generate baryogenesis, by taking the inflaton to be a complex scalar field with a weakly broken global symmetry and present a new version of the Affleck-Dine mechanism. The smallness of the…

高能物理 - 唯象学 · 物理学 2014-04-02 Mark P. Hertzberg , Johanna Karouby

We present a minimal approach to the generation of the baryon ($B$) asymmetry of the Universe, in which the asymmetry is generated in a complex inflaton condensate via $B$-violating quadratic inflaton potential terms using the Affleck-Dine…

高能物理 - 唯象学 · 物理学 2021-06-16 Amy Lloyd-Stubbs , John McDonald

Supersymmetric theories often include the non-compact directions in the field space along which the tree level potential grows only up to a certain limited value (determined by the mass scale of the theory) and then stays constant for the…

高能物理 - 唯象学 · 物理学 2009-10-28 Gia Dvali

We discuss two independent issues about the baryon asymmetry of the universe. First, assuming that it is generated by an unspecified source at high temperatures, we study the effects of non-perturbative $SU(2)_W$ dynamics above the…

高能物理 - 唯象学 · 物理学 2009-10-22 Luis E. Ibanez , Fernando Quevedo
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