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相关论文: Affleck-Dine Baryogenesis in Type IIB String Model…

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We consider the construction of inverted hybrid inflation models in which the vacuum energy during inflation is at the TeV scale, and the inflaton couples to the Higgs field. Such models are of interest in the context of some recently…

高能物理 - 唯象学 · 物理学 2009-11-07 Edmund J. Copeland , David Lyth , Arttu Rajantie , Mark Trodden

Affleck-Dine baryogenesis in models where the gravitino is both the lightest supersymmetric particle and the dark matter candidate is investigated. For a high enough reheating temperature to produce sufficient gravitinos by thermal…

高能物理 - 唯象学 · 物理学 2009-11-11 Osamu Seto

We show that in a large volume scenario of type IIB string or F-theory compactifications, single thermal inflation provides only a partial solution to the cosmological problem of the light volume modulus. We then clarify the conditions for…

高能物理 - 唯象学 · 物理学 2015-06-12 Kiwoon Choi , Wan-Il Park , Chang Sub Shin

We present a type IIB 4D string model with stabilised moduli which is able to describe the history of the universe from inflation to quintessence. The underlying Calabi-Yau volume is controlled by two moduli which are stabilised by…

高能物理 - 理论 · 物理学 2024-07-08 Michele Cicoli , Francesc Cunillera , Antonio Padilla , Francisco G. Pedro

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…

高能物理 - 理论 · 物理学 2015-06-04 M. Cicoli , G. Tasinato , I. Zavala , C. P. Burgess , F. Quevedo

Affleck-Dine leptogenesis after thermal inflation along the $LH_u$ direction requires $m_L^2+m_{H_u}^2 < 0$ up to the AD scale ($|L|\simeq |H_u|\sim 10^9$ GeV). We renormalised this condition from the AD scale to the soft supersymmetry…

高能物理 - 唯象学 · 物理学 2020-09-30 Seolhwa Kim , Ewan D. Stewart

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…

高能物理 - 唯象学 · 物理学 2016-09-06 Tomohiro Matsuda

We present an explicit embedding of axionic N-flation in type IIB string compactifications where most of the Kahler moduli are stabilised by perturbative effects, and so are hierarchically heavier than the corresponding N >> 1 axions whose…

高能物理 - 理论 · 物理学 2015-07-24 Michele Cicoli , Koushik Dutta , Anshuman Maharana

We investigate whether the Affleck-Dine (AD) mechanism works when the contribution of the two-loop thermal correction to the potential is negative in the gauge-mediated supersymmetry breaking models. The AD field is trapped far away from…

高能物理 - 唯象学 · 物理学 2009-11-10 S. Kasuya , M. Kawasaki , Fuminobu Takahashi

We perform a detailed analysis on Affleck-Dine leptogenesis taking into account the thermal effects on the dynamics of the flat direction field $\phi$. We find that an extremely small mass for the lightest neutrino $\nu_1$, ${m_\nu}_1\lsim…

高能物理 - 唯象学 · 物理学 2009-10-31 T. Asaka , Masaaki Fujii , K. Hamaguchi , T. Yanagida

We propose a mechanism for cogenesis of baryon and dark matter (DM) in the universe via the Affleck-Dine (AD) route. An AD field which breaks the lepton number symmetry, leads to the generation of lepton asymmetry by virtue of its cosmic…

高能物理 - 唯象学 · 物理学 2023-05-24 Debasish Borah , Suruj Jyoti Das , Nobuchika Okada

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

One interpretation of proton stability is the existence of extra-flat directions of the MSSM, in particular $u^{c}u^{c}d^{c}e^{c}$ and $QQQL$, where the operators lifting the potential are suppressed by a mass scale $\Lambda$ which is much…

高能物理 - 唯象学 · 物理学 2008-11-26 John McDonald , Osamu Seto

The ultra-slow-roll (USR) inflation represents a class of single-field models with sharp deceleration of the rolling dynamics on small scales, leading to a significantly enhanced power spectrum of the curvature perturbations and primordial…

高能物理 - 唯象学 · 物理学 2023-03-27 Yi-Peng Wu , Elena Pinetti , Kalliopi Petraki , Joseph Silk

In this talk I discuss recent developments in moduli stabilisation, SUSY breaking and chiral D-brane models together with several interesting features of cosmological models built in the framework of type IIB string compactifications. I…

高能物理 - 理论 · 物理学 2016-04-05 Michele Cicoli

In D-term inflation models, Affleck-Dine baryogenesis produces isocurvature density fluctuations. These can be perturbations in the baryon number, or, in the case where the present neutralino density comes directly from B-ball decay,…

高能物理 - 唯象学 · 物理学 2009-10-31 Kari Enqvist , John McDonald

In this paper we point out that the cosmological baryon asymmetry in our universe is generated almost independently of the reheating temperature $T_R$ in Affleck-Dine leptogenesis and it is determined mainly by the mass of the lightest…

高能物理 - 唯象学 · 物理学 2009-11-07 Masaaki Fujii , K. Hamaguchi , T. Yanagida

The early universe could feature multiple reheating events, leading to jumps in the visible sector entropy density that dilute both particle asymmetries and the number density of frozen-out states. In fact, late time entropy jumps are…

高能物理 - 唯象学 · 物理学 2017-03-08 Joseph Bramante , James Unwin

Motivated by the recently proposed Trans-Planckian Censorship Conjecture (TCC), we propose a gauged $B-L$ model of inflection-point inflation with axion dark matter. The Hubble scale during inflation ($H_{\rm inf}$) satisfies the TCC bound…

高能物理 - 唯象学 · 物理学 2020-12-09 Nobuchika Okada , Digesh Raut , Qaisar Shafi

Radiative neutrino mass models have interesting features, which make it possible to relate neutrino masses to the existence of dark matter. However, the explanation of the baryon number asymmetry in the universe seems to be generally…

高能物理 - 唯象学 · 物理学 2015-03-17 H. Higashi , T. Ishima , D. Suematsu