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Recently, various observational data predict a possibility that inflation may naturally occur in a warm region. In this scenario, radiation is produced during the inflation epoch and reheating is avoided. The main question arises that what…

General Relativity and Quantum Cosmology · Physics 2015-06-19 M. R. Setare , A. Sepehri , V. Kamali

We derive the general form of the cosmological scalar field potential which is compatible both with the existence of black holes and p-branes related to string/M theory and with multidimensional inflationary cosmology. It is shown that the…

High Energy Physics - Theory · Physics 2009-11-11 Konstantin G. Zloshchastiev

We present a minimal model for the Universe evolution fully extracted from effective String Theory. This model is by its construction close to the standard cosmological evolution, and it is driven selfconsistently by the evolution of the…

High Energy Physics - Theory · Physics 2007-05-23 N. Sanchez

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

We consider, in the context of a braneworld cosmology, the motion of the universe coupled to a four-form gauge field, with constant field strength, defined in higher dimensions. It is found, under rather general initial conditions, that in…

High Energy Physics - Theory · Physics 2017-01-18 Jeff Greensite

We examine the possibility that an epoch of inflationary expansion induces high-frequency oscillations of Newton's constant, $G$. The effect occurs because inflation can shift the expectation value of a non-minimally coupled,…

Astrophysics · Physics 2009-09-25 Clifford M. Will , Paul J. Steinhardt

We consider the interactions between Dp-branes intersecting at an arbitrary number of angles in the context of type II string theory. For cosmology purposes we concentrate in the theory on R^{3,1} x T^6. Interpreting the distance between…

High Energy Physics - Theory · Physics 2009-11-07 M. Gomez-Reino , I. Zavala

A quantum-mechanical technique is used within the framework of U(2) super-Yang-Mills theory to investigate what happens in the process after recombination of two D-p-branes at one angle. Two types of initial conditions are considered, one…

High Energy Physics - Theory · Physics 2010-04-05 Takeshi Sato

We reconsider a string theoretic inflationary model, where inflation is driven by $n$ multiple coincident $D3$-branes in the finite $n$ limit. We show that the finite $n$ action can be continued to the limit of large $n$, where it converges…

High Energy Physics - Theory · Physics 2010-01-22 Aaron Berndsen , James. E. Lidsey , John Ward

In this paper we consider inflation as a probe of new physics near the string or Planck scale. We discuss how new physics can be captured by the choice of vacuum, and how this leads to modifications of the primordial spectrum as well as the…

High Energy Physics - Theory · Physics 2009-11-11 Ulf H. Danielsson

String Gas Cosmology is a model of the evolution of the very early universe based on fundamental principles and key new degrees of freedom of string theory which are different from those of point particle field theories. In String Gas…

High Energy Physics - Theory · Physics 2015-05-28 Robert H. Brandenberger

Within the framework of a novel functional method on the world-sheet of the string, we discuss simple but re-summed (in the Regge slope) inflationary scenarios in the context of closed Bosonic strings, living in four target-space…

High Energy Physics - Theory · Physics 2009-03-27 Jean Alexandre , Anna Kostouki , Nick E. Mavromatos

In the context of (4+d)-dimensional general relativity, we propose an inflationary scenario wherein 3 spatial dimensions grow large, while d extra dimensions remain small. Our model requires that a self-interacting d-form acquire a vacuum…

High Energy Physics - Theory · Physics 2009-11-10 C. Armendariz-Picon , Vikram Duvvuri

We study the Friedmann equation for the warped codimension-two braneworld background which most closely resembles the Randall-Sundrum model. Extra matter on the (Planck) 4-brane, with equation of state p_\theta=(\alpha-1)\rho for the…

High Energy Physics - Theory · Physics 2008-11-26 Fang Chen , James M. Cline , Sugumi Kanno

We consider a 4+N dimensional Einstein gravity coupled to a non-linear sigma model. This theory admits a solution in which the N extra dimensions contract exponentially while the ordinary space expand exponentially. Physically, the…

High Energy Physics - Phenomenology · Physics 2015-05-18 Chiu Man Ho , Thomas W. Kephart

We have investigated the finite temperature systems of non-BPS D-branes and D-brane-anti-D-brane pairs in the previous papers. It has been shown that non-BPS D9-branes and D9-anti-D9 pairs become stable near the Hagedorn temperature on the…

High Energy Physics - Theory · Physics 2009-11-11 Kenji Hotta

We consider gravitational wave production during inflation in type IIB string theory, and the possibility of observable gravitational waves in small field inflation. We show that the gauge field excitations on a set of coincident D7 branes,…

High Energy Physics - Theory · Physics 2018-11-21 Evan McDonough , Stephon Alexander

It is widely believed that string theory easily allows for a QCD axion in the cosmologically favoured mass range. The required small decay constant, $f_a\ll M_P$, can be implemented by using a large compactification volume. This points to…

High Energy Physics - Theory · Physics 2022-10-19 Michele Cicoli , Arthur Hebecker , Joerg Jaeckel , Manuel Wittner

The four-form field recently considered by Hawking and Turok couples naturally to a charged membrane, across which the effective cosmological constant has a discontinuity. We present instantons for the creation of an open inflationary…

High Energy Physics - Theory · Physics 2009-10-31 Raphael Bousso , Andrew Chamblin

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…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. R. Espinosa , A. Riotto , G. G. Ross
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