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We investigate the viability of Affleck-Dine baryogenesis in D=4, N=1 supergravity descending from string theory. The process relies on an initial condition where visible sector supersymmetric flat directions obtain tachyonic masses during…

High Energy Physics - Theory · Physics 2010-11-11 Bhaskar Dutta , Kuver Sinha

Flat manifold leptogenesis a la Affleck-Dine is investigated with the slepton and Higgs fields, L, H_u, H_d, in the supersymmetric standard model. The multi-dimensional motion of these scalar fields is realized in the case that the L H_u…

High Energy Physics - Phenomenology · Physics 2009-11-07 Masato Senami , Katsuji Yamamoto

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…

High Energy Physics - Phenomenology · Physics 2014-04-02 Mark P. Hertzberg , Johanna Karouby

We propose to introduce non-minimal couplings of Affleck-Dine (AD) field to gravity by adding the coupling of AD field to the Ricci scalar curvature. As the Jordan frame supergravity always predict $|\Phi|^2 {\cal R}/6$ type coupling for…

General Relativity and Quantum Cosmology · Physics 2022-04-13 Fei Wang , Rui Wang

We investigate how gravity affects "Q-balls" with the Affleck-Dine potential $V_{AD}(\phi):=\frac{m^2}{2}\phi^2[ 1+K\ln (\frac{\phi}{M})^2]$. Contrary to the flat case, in which equilibrium solutions exist only if $K<0$, we find three types…

General Relativity and Quantum Cosmology · Physics 2015-05-28 Takashi Tamaki , Nobuyuki Sakai

In the MSSM, cosmological scalar field condensates formed along flat directions of the scalar potential (Affleck-Dine condensates) are typically unstable with respect to formation of Q-balls, a type of non-topological soliton. I discuss the…

High Energy Physics - Phenomenology · Physics 2016-11-03 Kari Enqvist

The Affleck-Dine mechanism is a leading baryogenesis scenario in which scalar condensates form coherently during inflation along supersymmetric flat directions that are lifted by supersymmetry-breaking effects. We update the viable…

High Energy Physics - Phenomenology · Physics 2026-02-10 Yi-Peng Wu , Xingang Chen , Nino Ephremidze , Lingfeng Li

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

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…

High Energy Physics - Phenomenology · Physics 2009-11-07 Masaaki Fujii , K. Hamaguchi , T. Yanagida

Affleck-Dine baryogenesis is preconditioned on a certain structure of non-renormalizable operators in the Kahler potential. In this paper, we geometrically characterize the resulting constraint on the field space Kahler geometry and survey…

High Energy Physics - Theory · Physics 2015-05-30 David Marsh

It has been known for some time that asymptotic parity invariance of weak interactions can provide a solution to the strong CP problem without the need for the axion. Left-right symmetric theories which employ a minimal Higgs sector…

High Energy Physics - Phenomenology · Physics 2023-07-28 K. S. Babu , Rabindra N. Mohapatra , Nobuchika Okada

In this letter we show that the inflaton can generate the cosmological baryon asymmetry. We take the inflaton to be a complex scalar field with a weakly broken global symmetry and develop a new variant on the Affleck-Dine mechanism. The…

High Energy Physics - Phenomenology · Physics 2014-08-26 Mark P. Hertzberg , Johanna Karouby

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

We study the conditions for successful Affleck-Dine baryogenesis and the origin of gravitino dark matter in GMSB models. AD baryogenesis in GMSB models is ruled out by neutron star stability unless Q-balls are unstable and decay before…

High Energy Physics - Phenomenology · Physics 2011-06-09 Francesca Doddato , John McDonald

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 baryon asymmetry in the supersymmetry Dine-Fischler-Srednicki-Zhitnitsky axion model without R-parity. It turns out that the R-parity violating terms economically explain the atmospheric mass-squared difference of…

High Energy Physics - Phenomenology · Physics 2019-04-03 Kensuke Akita , Hajime Otsuka

We consider the Affleck-Dine mechanism for leptogenesis in the minimal MSSM with Dirac or Pseudo-Dirac neutrinos. The rolling of scalars along D-flat directions generates a left-right asymmetry in the sneutrino sector, only the left part of…

High Energy Physics - Phenomenology · Physics 2009-11-11 Steven Abel , Veronique Page

The presently observed cosmological baryon asymmetry has been finally determined at the time of the electroweak phase transition, when baryon and lepton number violating interactions fell out of thermal equilibrium. We discuss the…

High Energy Physics - Phenomenology · Physics 2007-05-23 W. Buchmuller

We consider the cosmological moduli problem in the context of high-scale supersymmetry breaking suggested by the recent discovery of the standard-model like Higgs boson. In order to solve the notorious moduli-induced gravitino problem, we…

High Energy Physics - Phenomenology · Physics 2015-06-05 Tetsutaro Higaki , Kohei Kamada , Fuminobu Takahashi

Perturbation theory at finite temperature suffers from well-known infrared problems. In the standard model, as a result, one cannot calculate the effective potential for arbitrarily small values of $\phi$, the Higgs expectation value.…

High Energy Physics - Phenomenology · Physics 2011-07-19 John Bagnasco , Michael Dine
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