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Related papers: D-term inflation in D-brane cosmology

200 papers

We study reheating after the end of inflation in models where the inflaton is the superpartner of goldstino and is charged under a gauged $U(1)$ R-symmetry. We consider two classes of models -- one is small field characterized by an almost…

High Energy Physics - Theory · Physics 2021-12-10 Yermek Aldabergenov , Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono

We revisit phenomenological as well as string-theoretical aspects of D-brane inflation cosmological models. Phenomenologically these models stand out on par with $\alpha$-attractors, as models with Planck-compatible values of $n_s$, moving…

High Energy Physics - Theory · Physics 2019-01-30 Renata Kallosh , Andrei Linde , Yusuke Yamada

In axion monodromy inflation, traversing $N$ axion periods corresponds to discharging $N$ units of a quantized charge. In certain models with moving D7-branes, such as Higgs-otic inflation, this monodromy charge is D3-brane charge induced…

High Energy Physics - Theory · Physics 2018-12-11 Manki Kim , Liam McAllister

In this paper, we show that if we extend D-term hybrid inflation by adding a light scalar field which couples to a waterfall field, large non-Gaussianity can be generated at the end of inflation. Contribution of cosmic strings generated…

High Energy Physics - Phenomenology · Physics 2009-08-31 Chia-Min Lin

We present a general set-up for inflation in string theory where the inflaton field corresponds to Wilson lines in compact space in the presence of magnetic fluxes. T-dualities and limits on the value of the magnetic fluxes relate this…

High Energy Physics - Theory · Physics 2008-11-26 A. Avgoustidis , D. Cremades , F. Quevedo

The warm inflation paradigm considers the continuous production of radiation during inflation due to dissipative effects. In its strong dissipation limit, warm inflation gives way to a radiation dominated Universe. High scale inflation then…

High Energy Physics - Phenomenology · Physics 2011-03-18 Juan C. Bueno Sanchez , Mar Bastero-Gil , Arjun Berera , Konstantinos Dimopoulos , Kazunori Kohri

We argue that the mass of the inflaton can be much smaller than the Hubble constant in supergravity models in which inflation is driven by D--terms and not F--terms. We investigate a supergravity toy model which leads to hybrid inflation…

High Energy Physics - Phenomenology · Physics 2009-10-28 Edi Halyo

We study the possibility of realising cosmic inflation, dark matter (DM), baryon asymmetry of the universe (BAU) and light neutrino masses in non-supersymmetric minimal gauged $B-L$ extension of the standard model with three right handed…

High Energy Physics - Phenomenology · Physics 2021-03-17 Debasish Borah , Suruj Jyoti Das , Abhijit Kumar Saha

We propose that under certain conditions the universal open string tachyon can drive topological inflation in moduli stabilised frameworks. Namely, the presence of electric field in the world volume of the D-brane can slow down its decay…

High Energy Physics - Theory · Physics 2009-11-11 Daniel Cremades

We study the dynamics of two concrete inflationary models, namely Spontaneous Symmetry Breaking Inflation as well as Loop Inflation. We constrain the parameters for which a viable inflationary Universe emerges using the latest PLANCK…

General Relativity and Quantum Cosmology · Physics 2020-01-17 Matias Lopez , Nelson Videla , Grigoris Panotopoulos

Tribrid inflation is a class of supersymmetric inflation models where the scalar component of a matter superfield, or a $D$-flat direction of matter fields, drives inflation. Similar to Hybrid inflation, the end of inflation is reached when…

High Energy Physics - Phenomenology · Physics 2024-11-06 Stefan Antusch , Katarina Trailović

A small tensor-to-scalar ratio $r$ may lead to distinctive phenomenology of high-scale supersymmetry. Assuming the same origin of SUSY breaking between the inflation and visible sector, we show model independent features. The simplest…

High Energy Physics - Phenomenology · Physics 2015-08-26 Sibo Zheng

No-scale supergravity provides a successful framework for Starobinsky-like inflation models. Two classes of models can be distinguished depending on the identification of the inflaton with the volume modulus, $T$ (C-models), or a…

High Energy Physics - Phenomenology · Physics 2020-01-15 Kunio Kaneta , Yann Mambrini , Keith A. Olive , Sarunas Verner

F-term hybrid inflation models in the context of supergravity generically have corrections to the inflaton mass squared of the order of H^{2} (the \eta-problem). In addition they have a problem with large deviations of the spectrum of…

High Energy Physics - Phenomenology · Physics 2009-11-07 John McDonald

Scalar and tensor perturbations arising in an inflationary braneworld scenario driven by a single scalar field are considered, where the bulk on either side of the brane corresponds to Anti-de Sitter spaces with different cosmological…

Astrophysics · Physics 2009-11-07 Greg Huey , James E. Lidsey

We investigate models in which inflation is driven by a single geometrical tachyon. We assume that the D-brane as a probe brane in the background of NS5-branes has non-zero angular momentum which is shown to play similar role as the number…

High Energy Physics - Theory · Physics 2015-05-28 Pyung Seong Kwon , Gyeong Yun Jun , Kamal L. Panigrahi , M. Sami

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

We study an effective four-dimensional theory with an action with two scalar fields minimally coupled to gravity, and with a matter action which couples to the two scalar fields via an overall field-dependent coefficient in the action. Such…

High Energy Physics - Theory · Physics 2009-11-11 Tirthabir Biswas , Robert Brandenberger , Damien A. Easson , Anupam Mazumdar

We study cosmological inflation on a warped DGP braneworld where inflaton field is non-minimally coupled to induced gravity on the brane. We present a detailed calculation of the perturbations and inflation parameters both in Jordan and…

General Relativity and Quantum Cosmology · Physics 2015-06-05 Kourosh Nozari , Narges Rashidi

Combining previous results, the D3-anti-D3-brane pair potential U(T,{\phi}) is presented here, where the inflaton {\phi} measures the separation between the D3-brane and the anti-D3-brane, and the complex scalar mode T becomes tachyonic…

High Energy Physics - Theory · Physics 2024-01-01 Henry S. -H. Tye
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