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Related papers: P-term, D-term and F-term inflation

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We study a $D$-term inflation scenario in a model extended from the minimal supersymmetric standard model (MSSM) by two additional abelian factor groups focussing on its particle physics aspects. Condensates of the fields related to the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Daijiro Suematsu

We revisit the F-term hybrid inflation model in supergravity. In particular, we point out that a constant term in the superpotential has significant effects on the inflaton dynamics. It is shown that the hybrid inflation model suffers from…

High Energy Physics - Phenomenology · Physics 2011-04-15 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We show that inflation which is dominated by the D-term density avoids the `slow-roll' problem of inflation in supergravity. Such an inflationary scenario can naturally emerge in theories with non-anomalous or anomalous U(1) gauge symmetry.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Pierre Binetruy , Gia Dvali

We analyze F-term hybrid inflation (FHI) within various grand unified theories (GUTs) in the presence of a K\"ahler potential for the inflaton field which parameterizes the K\"ahler manifolds $SU(1,1)/U(1)$ or $SU(2)/U(1)$. We take into…

High Energy Physics - Phenomenology · Physics 2026-05-12 Waqas Ahmed , Constantinos Pallis , Mansoor Ur Rehman

A simple model for chaotic inflation in supergravity is proposed. The model is N=1 supersymmetric massive U(1) gauge theory via the Stuckelberg superfield and gives rise to D-term inflation with a quadratic term of inflaton in the…

High Energy Physics - Theory · Physics 2008-12-23 Teruhiko Kawano

Following \cite{Lin:2009yt}, we explore the parameter space of the case when the supersymmetry (SUSY) breaking scale is lower, for example, in gauge mediated SUSY breaking model. During inflation, the form of the potential is $V_0$ plus…

High Energy Physics - Phenomenology · Physics 2014-11-18 Chia-Min Lin , Kingman Cheung

We revisit D-term inflation with the bounds of the cosmic string tension from gravitational wave observations and consider the possible deviation of the spectral index compared with the $\Lambda$CDM model in light of prerecombination…

High Energy Physics - Theory · Physics 2022-11-23 Chia-Min Lin

An inflationary stage dominated by a D-term avoids the slow-roll problem of inflation in supergravity and can naturally emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. In the latter case, however, the scale of…

High Energy Physics - Phenomenology · Physics 2009-10-30 D. H. Lyth , A. Riotto

The minimal supersymmetric (or F-term) hybrid inflation is defined by a unique renormalizable superpotential, fixed by a $U(1)$ R-symmetry, and it employs a canonical K\"{a}hler potential. The inflationary potential takes into account both…

High Energy Physics - Phenomenology · Physics 2013-12-17 Constantinos Pallis , Qaisar Shafi

In the presence of fields without superpotential but with large vevs through D-terms the mass-squared of the inflaton in the context of supergravity hybrid inflation receives positive contributions which could cancel the possibly negative…

High Energy Physics - Phenomenology · Physics 2009-10-31 C. Panagiotakopoulos

We show that an inflationary background might be realized by using any p-form non-minimally coupled to gravity. Standard scalar field inflation corresponds to the 0-form case and vector inflation to the 1-form. Moreover, we show that the 2-…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 Cristiano Germani , Alex Kehagias

We show how the motion through the extra dimensions of a gas of branes and antibranes can, under certain circumstances, produce an era of inflation as seen by observers trapped on a 3-brane, with the inflaton being the inter-brane…

High Energy Physics - Theory · Physics 2010-02-03 C. P. Burgess , M. Majumdar , D. Nolte , F. Quevedo , G. Rajesh , R. -J. Zhang

A sizeable tensor-to-scalar ratio, such as recently claimed by BICEP2, would imply a scale of inflation at the typical scale of supersymmetric grand unification. This could be an accident, or strong support for supersymmetric theories.…

High Energy Physics - Phenomenology · Physics 2015-06-19 Felix Brummer , Valerie Domcke , Veronica Sanz

We shall investigate the inflation for the D-brane model, motivated by the modified gravity $F(\phi,T)$. This gravity has been recently introduced in the literature. The feasibility of the D-brane inflation theory in the $F(\phi,T)$-gravity…

General Relativity and Quantum Cosmology · Physics 2025-08-04 Feyzollah Younesizadeh , Davoud Kamani

We present a D-term hybrid inflation model, embedded in supergravity with moduli stabilisation. Its novel features allow us to overcome the serious challenges of combining D-term inflation and moduli fields within the same string-motivated…

High Energy Physics - Theory · Physics 2010-10-27 Ph. Brax , C. van de Bruck , A. C. Davis , Stephen C. Davis , R. Jeannerot , M. Postma

Inflation is well known to be difficult in the context of supergravity, if the potential is dominated by the $F$ term. Non-renormalizable terms generically give $|V''|\sim V/M^2$, where $V(\phi)$ is the inflaton potential and $M$ is the…

High Energy Physics - Phenomenology · Physics 2009-10-30 David Lyth

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

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…

High Energy Physics - Phenomenology · Physics 2009-10-28 Gia Dvali

We obtain brane inflation in configurations with Dp and D(p-2) branes which are far apart and almost perpendicular to each other. Chaotic brane inflation occurs when the branes can only rotate with the inflaton given by the angle between…

High Energy Physics - Phenomenology · Physics 2007-05-23 Edi Halyo

We consider gravitationally induced corrections to inflaton potentials driven by supersymmetry breaking in a five-dimensional supergravity, compactified on a $ S_1/Z_2 $ orbifold. The supersymmetry breaking takes place on the hidden brane…

High Energy Physics - Theory · Physics 2024-12-10 G. A. Diamandis , K. Kaskavelis , A. B. Lahanas , G. Pavlopoulos