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相关论文: Comments on D-term inflation

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An inflationary stage dominated by a $D$-term avoids the slow-roll problem of inflation in supergravity and may emerge in theories with a non-anomalous or anomalous U(1) gauge symmetry. The most intriguing and commonly invoked possibility…

高能物理 - 唯象学 · 物理学 2009-10-31 J. R. Espinosa , A. Riotto , G. G. Ross

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.…

高能物理 - 唯象学 · 物理学 2009-10-28 Pierre Binetruy , Gia Dvali

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 this talk different aspects of D-term…

高能物理 - 唯象学 · 物理学 2016-10-26 Antonio Riotto

We examine the consequences of recent developments on Fayet-Iliopoulos (FI) terms for D-term inflationary models. There is currently no known way to couple constant FI terms to supergravity consistently; only field-dependent FI terms are…

高能物理 - 理论 · 物理学 2011-03-22 Rhiannon Gwyn , Mairi Sakellariadou , Spyros Sypsas

Hybrid inflation, driven by a Fayet-Iliopoulos (FI) D term, is an intriguing inflationary model. In its usual formulation, it however suffers from several shortcomings. These pertain to the origin of the FI mass scale, the stability of…

高能物理 - 唯象学 · 物理学 2018-06-29 Valerie Domcke , Kai Schmitz

We propose a new model of the D-term hybrid inflation in the framework of supergravity. Although our model introduces, analogously to the conventional D-term inflation, the inflaton and a pair of scalar fields charged under a $U(1)$ gauge…

高能物理 - 唯象学 · 物理学 2017-12-06 Kenji Kadota , Tatsuo Kobayashi , Keigo Sumita

D-term inflation realized in heterotic string theory has two problems: the scale of the anomalous D-term is too large for accounting for COBE data and the coupling constant of the anomalous U(1) is too large for supergravity to be valid. We…

高能物理 - 唯象学 · 物理学 2009-10-31 Edi Halyo

Standard D-term inflation is studied in the framework of supergravity. D-term inflation produces cosmic strings, however it can still be compatible with CMB measurements without invoking any new physics. The cosmic strings contribution to…

高能物理 - 唯象学 · 物理学 2009-11-10 Jonathan Rocher , Mairi Sakellariadou

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…

高能物理 - 理论 · 物理学 2010-10-27 Ph. Brax , C. van de Bruck , A. C. Davis , Stephen C. Davis , R. Jeannerot , M. Postma

We propose a new model of single-field D-term inflation in supergravity, where the inflation is driven by a single modulus field which transforms non-linearly under the U(1) gauge symmetry. One of the notable features of our modulus D-term…

高能物理 - 唯象学 · 物理学 2018-05-09 Kenji Kadota , Tatsuo Kobayashi , Ikumi Saga , Keigo Sumita

Two of the most attractive realizations of inflation in supergravity are based upon the presence of a constant Fayet-Iliopoulos (FI) term. In D-term hybrid inflation it is the FI term itself which sets the energy scale of inflation.…

高能物理 - 理论 · 物理学 2014-11-11 Clemens Wieck , Martin Wolfgang Winkler

The influence of higher-order terms in the K\"{a}hler potential of the supergravity D-term inflation model on the density perturbation is studied. We show that these terms can make the inflaton potential flatter, which lowers the energy…

高能物理 - 唯象学 · 物理学 2009-11-11 Osamu Seto , Jun'ichi Yokoyama

We present a new model of D-term dominated chaotic inflation in supergravity. The F-flat direction present in this model is lifted by the dominant D-term, which leads to chaotic inflation and subsequent reheating. No cosmic string is formed…

高能物理 - 唯象学 · 物理学 2008-11-26 Kenji Kadota , Teruhiko Kawano , Masahide Yamaguchi

We analyse the consequences of a new gauge invariant Fayet-Iliopoulos (FI) term proposed recently to a class of inflation models driven by supersymmetry breaking with the inflaton being the superpartner of the goldstino. We first show that…

高能物理 - 理论 · 物理学 2018-06-19 Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono , Rob Knoops

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…

高能物理 - 理论 · 物理学 2008-12-23 Teruhiko Kawano

Models of supersymmetric D-term inflation require a new mass scale near 10^{15-16} GeV in order to match the density perturbation spectrum observed by COBE. Attempts to obtain such a scale from the anomalous U(1) of string theories fail in…

高能物理 - 唯象学 · 物理学 2007-05-23 Christopher Kolda , David H. Lyth

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…

高能物理 - 唯象学 · 物理学 2014-11-17 Daijiro Suematsu

We present a superstring-inspired version of D-term inflation which does not lead to cosmic string formation and appears to satisfy the current CMB constraints. It differs from minimal D-term inflation by a second pair of charged…

高能物理 - 理论 · 物理学 2009-11-10 J. Urrestilla , A. Achucarro , A. C. Davis

D-term inflation is one of the most interesting and versatile models of inflation. It is possible to implement naturally D-term inflation within high energy physics, as for example SUSY GUTs, SUGRA, or string theories. D-term inflation…

高能物理 - 理论 · 物理学 2009-11-11 Jonathan Rocher , Mairi Sakellariadou

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…

高能物理 - 唯象学 · 物理学 2018-06-26 Valerie Domcke , Kai Schmitz
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