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Related papers: E- & T-Model Hybrid Inflation

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We revisit the no-scale ripple inflation model, where no-scale supergravity is modified by an additional term for the inflaton field in the Kahler potential. This term not only breaks one SU(N,1) symmetry explicitly, but also plays an…

High Energy Physics - Phenomenology · Physics 2015-06-17 Tianjun Li , Zhijin Li , Dimitri V. Nanopoulos

We consider hybrid inflation for small couplings of the inflaton to matter such that the critical value of the inflaton field exceeds the Planck mass. It has recently been shown that inflation then continues at subcritical inflaton field…

High Energy Physics - Phenomenology · Physics 2015-04-16 Wilfried Buchmuller , Koji Ishiwata

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical abelian projection and centerization. The underlying gauge symmetry is…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ralf Hofmann , Mathias Th. Keil

We show how hybrid inflation can be successfully realized in a supersymmetric model with gauge group G_{PS}= SU(4)_c x SU(2)_L x SU(2)_R. By including a non-renormalizable superpotential term, we generate an inflationary valley along which…

High Energy Physics - Phenomenology · Physics 2010-04-06 R. Jeannerot , S. Khalil , G. Lazarides , Q. Shafi

We propose an inflationary model ("natural hybrid model"), which combines the supersymmetric hybrid model and the natural inflation model to achieve the spectral index of 0.96, and the axion decay constant smaller than the Planck scale, f<<…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Ki-Young Choi , Bumseok Kyae

In their minimal form both supersymmetric and smooth hybrid inflation yield a scalar spectral index n_s close to 0.98, to be contrasted with the result n_s=0.951+0.015-0.019 from WMAP3. To realize better agreement, following hep-ph/0604198,…

High Energy Physics - Phenomenology · Physics 2008-11-26 Mansoor ur Rehman , V. N. Senoguz , Qaisar Shafi

In many moduli stabilization schemes in string theory, the scale of inflation appears to be of the same order as the scale of supersymmetry breaking. For low-scale supersymmetry breaking, therefore, the scale of inflation should also be…

High Energy Physics - Theory · Physics 2010-05-12 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

A simple extension of the minimal left-right symmetric supersymmetric grand unified theory model is constructed by adding two pairs of superfields. This naturally violates the partial Yukawa unification predicted by the minimal model. After…

High Energy Physics - Phenomenology · Physics 2014-03-26 R. Armillis , G. Lazarides , C. Pallis

Supersymmetry-based hybrid inflation models (referred to as `spontaneously broken supersymmetry' by the Planck collaboration) are attractive for several reasons, including the appealing feature that inflation is associated with local gauge…

Cosmology and Nongalactic Astrophysics · Physics 2025-04-22 Mansoor Ur Rehman , Qaisar Shafi

We present a mechanism for realizing hybrid inflation using two axion fields with a purely non-perturbatively generated scalar potential. The structure of scalar potential is highly constrained by the discrete shift symmetries of the…

High Energy Physics - Theory · Physics 2021-04-28 Federico Carta , Nicole Righi , Yvette Welling , Alexander Westphal

Inflation and moduli stabilisation mechanisms work well independently, and many string-motivated supergravity models have been proposed for them. However a complete theory will contain both, and there will be (gravitational) interactions…

High Energy Physics - Theory · Physics 2014-11-18 Stephen C. Davis , M. Postma

We consider a supersymmetric hybrid inflation model with two inflaton fields. The superpotential during inflation is dominated by W=(\kappa S+\kappa' S')M^2, where S, S' are inflatons carrying the same U(1)_R charge, \kappa, \kappa' are…

High Energy Physics - Phenomenology · Physics 2015-05-14 Bumseok Kyae

Minimal supersymmetric hybrid inflation based on a minimal Kahler potential predicts a spectral index n_s\gsim 0.98. On the other hand, WMAP three year data prefers a central value n_s \approx 0.95. We propose a class of supersymmetric…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Bastero-Gil , S. F. King , Q. Shafi

Transforming canonical scalars to the Einstein frame can give a multi-field generalization of pole inflation (namely, a scalar with a divergent kinetic term) at vanishing field-dependent Planck mass. However, to obtain an attractor, the…

High Energy Physics - Theory · Physics 2022-09-07 Sotirios Karamitsos , Alessandro Strumia

We investigate an inflation model with the inflaton being identified with a Higgs boson responsible for the breaking of U(1)B-L symmetry. We show that supersymmetry must remain a good symmetry at scales one order of magnitude below the…

High Energy Physics - Phenomenology · Physics 2012-03-13 Kazunori Nakayama , Fuminobu Takahashi

We propose a cosmological inflationary scenario based on the supergravity-embedded Standard Model supplemented by the right-handed neutrinos. We show that with an appropriate Kahler potential the L-H_u direction gives rise to successful…

High Energy Physics - Phenomenology · Physics 2013-05-30 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We discuss the hybrid inflation model where the inflaton field is nonminimally coupled to gravity. In the Jordan frame, the potential contains $\phi^4$ term as well as terms in the original hybrid inflation model. In our model, inflation…

High Energy Physics - Theory · Physics 2011-02-22 Seoktae Koh , Masato Minamitsuji

We propose a new realisation of hybrid inflation in supergravity where the inflaton field does not appear in the superpotential but contributes only through the Kahler potential. The scalar potential derived from an R-invariant…

High Energy Physics - Phenomenology · Physics 2015-06-25 H. Boutaleb-J , A. Chafik , A. L. Marrakchi

We study a supergravity model of inflation essentially depending on one parameter which can be identified with the slope of the potential at the origin. In this type of models the inflaton rolls at high energy from negative values and a…

Astrophysics · Physics 2009-11-10 G. German , A. de la Macorra

We briefly review several Higgs inflation models and discuss their cosmological implications. We first classify the inflation models according to the predicted value of the tensor-to-scalar ratio: (i) $r = {\cal O}(0.01-0.1)$, (ii) $r =…

High Energy Physics - Phenomenology · Physics 2015-06-01 Fuminobu Takahashi