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Related papers: Affleck-Dine Baryogenesis, Split Supersymmetry, an…

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We propose a new scenario of Affleck-dine baryogenesis in the context of theories with large extra dimensions. In this paper we consider baryogenesis after thermal brane inflation and show how our mechanism works. We specifically consider…

High Energy Physics - Phenomenology · Physics 2009-11-07 Tomohiro Matsuda

The onset of inflation in hybrid models require fine tuning in the initial conditions. The inflaton field should have an initial value close to the Planck scale $M_{P}$, whereas the auxiliary "orthogonal" field must be close to zero with an…

High Energy Physics - Phenomenology · Physics 2009-11-07 Zurab Berezhiani , Anupam Mazumdar , Abdel Pérez-Lorenzana

Many models of supersymmetry breaking involve particles with weak scale mass and Planck mass suppressed couplings. Coherent production of such particles in the early universe destroys the successful predictions of nucleosynthesis. We show…

High Energy Physics - Phenomenology · Physics 2009-09-15 Lisa Randall , Scott Thomas

The observed baryon asymmetry, as well as potentially an asymmetry in the dark matter sector, can be produced through dissipative particle production during inflation. A distinctive feature of this mechanism is the generation of matter…

Cosmology and Nongalactic Astrophysics · Physics 2014-10-29 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa

Inflation universally produces classical almost scale free Gaussian inhomogeneities of any light scalars. Assuming the coupling constants at the time of inflation depend on some light moduli fields, we encounter the generation of modulated…

Astrophysics · Physics 2009-11-10 Francis Bernardeau , Lev Kofman , Jean-Philippe Uzan

Supersymmetry breaking close to the scale of grand unification can explain cosmic inflation. As we demonstrate in this paper, this can be achieved in strongly coupled supersymmetric gauge theories, such that the energy scales of inflation…

High Energy Physics - Phenomenology · Physics 2018-06-26 Valerie Domcke , Kai Schmitz

In this work, we present a unified theoretical framework that simultaneously addresses some of the most intriguing puzzles in particle physics and cosmology, namely the origins of neutrino mass, baryon asymmetry, and cosmic inflation. In…

High Energy Physics - Phenomenology · Physics 2024-09-05 Ajay Kaladharan , Shaikh Saad

We re-examine Affleck-Dine baryo/leptogenesis from the oscillation of condensates along flat directions of the supersymmetric standard model, which attained large vevs at the end of inflationary epoque. The key observation is that…

High Energy Physics - Phenomenology · Physics 2009-09-11 Rouzbeh Allahverdi , Bruce. A. Campbell , John Ellis

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…

High Energy Physics - Phenomenology · Physics 2014-07-31 Wilfried Buchmuller , Valerie Domcke , Kohei Kamada , Kai Schmitz

The MSSM has flat directions in its scalar potential, along which it is natural for Bose condensates of squarks to form in the early Universe. A baryon asymmetry can be induced in these condensates via Affleck-Dine baryogenesis. The…

High Energy Physics - Phenomenology · Physics 2007-05-23 John McDonald

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

A decade ago, the first leptogenesis model based on inflation was proposed, where the complex phase of the inflaton field carries lepton number. If the inflaton field is an axion, it can couple to gravitational waves and gauge fields via.…

High Energy Physics - Theory · Physics 2016-11-23 Stephon H. S. Alexander

In this letter, we quantify the challenge of explaining the baryon asymmetry using initial conditions in a universe that undergoes inflation. Contrary to lore, we find that such an explanation is possible if net $B-L$ number is stored in a…

High Energy Physics - Phenomenology · Physics 2017-09-06 Gordan Krnjaic

Erickcek, Kamionkowski and Carroll proposed in 2008 that the dipole modulation of the CMB could be due to a very large scale perturbation of the field $\phi$ causing the primordial curvature perturbation. We repeat their calculation using…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 David H. Lyth

If the inflaton decays into several components during reheating, and if the corresponding decay rates are functions of spacetime-dependent quantities, it is possible to generate entropy perturbations after a stage of single-field inflation.…

Astrophysics · Physics 2007-05-23 C. Armendariz-Picon

We propose a unified framework that describes both the curvaton mechanism for generating primordial density fluctuations and the Affleck-Dine (AD) mechanism for baryogenesis. By introducing a complex scalar field (AD field) carrying a…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-16 Anish Ghoshal , Abhishek Naskar , Nobuchika Okada

The smallness of the baryon asymmetry in our universe is one of the greatest mysteries and may originate from some profound physics beyond the standard model. We investigate the Affleck-Dine baryogenesis in split supersymmetry, and find…

High Energy Physics - Phenomenology · Physics 2009-11-11 Shinta Kasuya , Fuminobu Takahashi

We discuss a mechanism for producing baryon density perturbations during inflationary stage and study the evolution of the baryon charge density distribution in the framework of the low temperature baryogenesis scenario. This mechanism may…

Astrophysics · Physics 2009-10-31 D. P. Kirilova , M. V. Chizhov

We consider the complex inflaton field with a CP asymmetric term for its potential. This CP asymmetric term produces the global charge of the inflaton after inflation. With the assignment of the baryon number to the inflaton, the baryon…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Naoyuki Takeda

We study stochastic inflation in the presence of a dynamical gravitational constant. We describe the Arnowitt--Deser--Misner formalism for Jordan--Brans--Dicke theory of gravity with an inflaton field. The inflaton and dilaton scalar fields…

Astrophysics · Physics 2009-10-22 Juan Garcia-Bellido
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