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Related papers: Compactification Effects in D-brane Inflation

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We use F-theory to derive a general expression for the flux potential of type II compactifications with D7/D3 branes, including open string moduli and 2-form fluxes on the branes. Our main example is F-theory on K3 $\times$ K3 and its…

High Energy Physics - Theory · Physics 2008-11-26 D. Lust , P. Mayr , S. Reffert , S. Stieberger

We analyze properties of non-supersymmetric isometry-preserving perturbations to the infrared region of the warped deformed conifold, i.e. the Klebanov Strassler solution. We discuss both perturbations that "squash" the geometry, so that…

High Energy Physics - Theory · Physics 2014-11-20 Paul McGuirk , Gary Shiu , Yoske Sumitomo

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

Fluxbrane inflation is a stringy version of D-term inflation in which two fluxed D7-branes move towards each other until their (relative) gauge flux annihilates. Compared to brane-antibrane inflation, the leading-order inflationary…

High Energy Physics - Theory · Physics 2013-01-25 Arthur Hebecker , Sebastian C. Kraus , Moritz Kuntzler , Dieter Lust , Timo Weigand

We analyze observational constraints on the parameter space of tachyonic inflation with a Gaussian potential and discuss some predictions of this scenario. As was shown by Kofman and Linde, it is extremely problematic to achieve the…

High Energy Physics - Theory · Physics 2008-11-26 Joris Raeymaekers

We derive a formula for D3-brane charge on a compact spacetime, which includes torsion corrections to the tadpole cancellation condition. We use this to classify D-branes and RR fluxes in type II string theory on RP^3xRP^{2k+1}xS^{6-2k}…

High Energy Physics - Theory · Physics 2007-05-23 P. Bouwknegt , J. Evslin , B. Jurco , V. Mathai , H. Sati

We study the assisted inflation scenario from the rolling of $N$ BPS D3-brane into the NS5-branes, on a transverse geometry of $R^3 \times S^1$, coupled to four dimensional gravity. We assume that the branes are distributed along $S^1$ and…

High Energy Physics - Theory · Physics 2009-11-19 Kamal L. Panigrahi , Harvendra Singh

Non-perturbative features of the derivative expansion of the effective action of a single D3-brane are obtained by considering scattering amplitudes of open and closed strings. This motivates expressions for the coupling constant dependence…

High Energy Physics - Theory · Physics 2014-11-18 Michael B. Green , Michael Gutperle

We analyze the trajectories for multifield DBI inflation, which can arise in brane inflation models, and show that the trajectories are the same as in typical slow roll inflation. We calculate the power spectrum and find that the higher…

High Energy Physics - Theory · Physics 2008-11-26 Min-xin Huang , Gary Shiu , Bret Underwood

In a recent paper we showed how Starobinsky-like inflation could emerge from dilaton dynamics in brane cosmology scenarios based on string theory, in which our universe is represented as a three-brane and the effective potential acquires a…

High Energy Physics - Theory · Physics 2015-06-19 John Ellis , Nick E. Mavromatos , Dimitri V. Nanopoulos

We illustrate a framework for constructing models of chaotic inflation where the inflaton is the position of a D3 brane along the universal cover of a string compactification. In our scenario, a brane rolls many times around a non-trivial…

High Energy Physics - Theory · Physics 2014-03-19 Benjamin Shlaer

We discuss various realizations of the four dimensional braneworld inflation in warped geometries of string theory. In all models the inflaton field is represented by a Dp probe brane scalar specifying its position in the warped throat of…

High Energy Physics - Theory · Physics 2009-11-10 Alex Buchel , Ahmad Ghodsi

We study the effect of rolling of N D3-branes in the vicinity of NS5-branes. We find out that this system coupled with the four dimensional gravity gives the slow roll assisted inflation of the scalar field theory. Once again this…

High Energy Physics - Theory · Physics 2009-06-11 Kamal L. Panigrahi , Harvendra Singh

The derivation of the complete anti-D3-brane low energy effective action in KKLT is reviewed. All worldvolume fields are included, together with the background moduli. The result is recast into a manifest supersymmetric form in terms of the…

High Energy Physics - Theory · Physics 2020-03-31 Niccolò Cribiori

We study the combined effect of world-volume and background fluxes on Euclidean D3-brane instantons in F-theory compactifications. We derive an appropriate form of the fermionic effective action, in which the fermions are topologically…

High Energy Physics - Theory · Physics 2015-06-12 Massimo Bianchi , Gianluca Inverso , Luca Martucci

Anti-D3 branes at the bottom of warped throats, commonly used to uplift the cosmological constant in String-Theory de Sitter proposals, source a plaethora of supersymmetry-breaking fluxes, that can interact nontrivially with other…

High Energy Physics - Theory · Physics 2022-11-29 Iosif Bena , Emilian Dudas , Mariana Graña , Gabriele Lo Monaco , Dimitrios Toulikas

We derive a microscopic bound on the maximal field variation of the inflaton during warped D-brane inflation. By a result of Lyth, this implies an upper limit on the amount of gravitational waves produced during inflation. We show that a…

High Energy Physics - Theory · Physics 2008-11-26 Daniel Baumann , Liam McAllister

We propose new large field inflation scenarios built on the framework of F-term axion monodromy. Our setup is based on string compactifications where D-branes create potentials for closed string axions via F-terms. Because the source of the…

High Energy Physics - Theory · Physics 2016-04-13 Dagoberto Escobar , Aitor Landete , Fernando Marchesano , Diego Regalado

We update predictions for observables in the "delicate" D3/anti-D3 inflationary model on the conifold. We use a full CMB likelihood calculation to assess goodness-of-fit, which is necessary because in this model the zeta power spectrum…

Cosmology and Nongalactic Astrophysics · Physics 2022-02-11 Kareem Marzouk , Alessandro Maraio , David Seery

I calculate the semiclassical phase shift ($\delta$), as function of impact parameter ($b$) and velocity ($v$), when one D-brane moves past another. From its low-velocity expansion I show that, for torroidal compactifications, the moduli…

High Energy Physics - Theory · Physics 2010-11-19 C. Bachas
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