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We solve the worldsheet theory describing the near-horizon dynamics of a D-string in the presence of a very large number N of D5-branes. The model is pre-geometric in the sense that the near-horizon worldsheet Lagrangian does not have…

High Energy Physics - Theory · Physics 2013-09-10 Frank Ferrari , Antonin Rovai

I discuss a specific model of space-time foam, inspired by the modern non-perturbative approach to string theory (D-branes). The model views our world as a three brane, intersecting with D-particles that represent stringy quantum gravity…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Nick E. Mavromatos

We assume a flat brane located at y=0, surrounded by an AdS space, and consider the 5D Einstein equations when the energy flux component of the energy-momentum tensor is related to the Hubble parameter through a constant Q. We calculate the…

General Relativity and Quantum Cosmology · Physics 2009-11-11 Iver Brevik , Jon-Mattis Borven , Sebastian Ng

D-branes are fundamental in all scenarios where there are large extra dimensions and the string scale is much smaller than the four-dimensional Planck mass. We show that this current picture leads to a new approach to string cosmology where…

High Energy Physics - Phenomenology · Physics 2009-10-31 Antonio Riotto

Using standard techniques in string/D-brane scattering amplitude computations, we evaluate the scattering of open strings off D-particles in brane world scenarios. The D-particles are viewed as D3 branes wrapped up around three cycles, and…

High Energy Physics - Theory · Physics 2009-09-28 Tianjun Li , Nick E. Mavromatos , Dimitri V. Nanopoulos , Dan Xie

We propose a new method to describe a recoiling D-brane that is elastically scattered by closed strings in the non-relativistic region. We utilize the low-energy effective field theory on the worldvolume of the D-brane, and the velocity of…

High Energy Physics - Theory · Physics 2010-04-05 Shin Nakamura

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

In the context of a toy model we discuss the phenomenon of colliding five-branes, with two of the extra space dimensions compactified on tori. In one of the branes (hidden world) the torus is magnetised. Assuming opposite-tension branes, we…

High Energy Physics - Theory · Physics 2014-11-18 Elias Gravanis , Nick E. Mavromatos

We identify a time-dependent class of metrics with potential applications to cosmology, which emerge from negative-tension branes. The cosmology is based on a general class of solutions to Einstein-dilaton-Maxwell theory, presented in…

High Energy Physics - Theory · Physics 2009-11-07 C. P. Burgess , F. Quevedo , S. -J. Rey , G. Tasinato , I. Zavala

We consider the thermodynamic and cosmological properties of brane gases in the early universe. Working in the low energy limit of M-theory we assume the universe is a homogeneous but anisotropic 10-torus containing wrapped 2-branes and a…

High Energy Physics - Theory · Physics 2008-11-26 Richard Easther , Brian R. Greene , Mark G. Jackson , Daniel Kabat

In this note we discuss a possible resolution of the flux singularities associated with the insertion of branes in backgrounds supported by fluxes that carry charges opposite to the branes. We present qualitative arguments that such a setup…

High Energy Physics - Theory · Physics 2012-11-22 Johan Blåbäck , Ulf H. Danielsson , Thomas Van Riet

We present holographic descriptions of thermalization in conformal field theories using probe D-branes in AdS X S space-times. We find that the induced metrics on Dp-brane worldvolumes which are rotating in an internal sphere direction have…

High Energy Physics - Theory · Physics 2015-03-17 Sumit R. Das , Tatsuma Nishioka , Tadashi Takayanagi

We consider the evolution of small rotational perturbations, with azimuthal symmetry, of the brane-world cosmological models. The equations describing the temporal, radial, and angular dependence of the perturbations are derived by taking…

High Energy Physics - Theory · Physics 2010-11-19 Chiang-Mei Chen , T. Harko , W. F. Kao , M. K. Mak

We discuss a new mechanism of obtaining a period of cosmological inflation in the context of string theory. This mechanism is based on embedded defects which form dynamically on higher dimensional D-branes. Such defects generate topological…

High Energy Physics - Theory · Physics 2007-05-23 Stephon Alexander , Robert Brandenberger , Moshe Rozali

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

The emergence of the cosmological composition (the reheating era) after the inflationary period is analyzed in the framework of the braneworld models, in which our Universe is a three-brane embedded in a five-dimensional bulk, by assuming…

General Relativity and Quantum Cosmology · Physics 2009-11-18 T. Harko , W. F. Choi , K. C. Wong , K. S. Cheng

A D3-brane probe in the context of AdS/CFT correspondence at finite temperature is considered. The supergravity predictions for the physical effective couplings of the world-volume gauge theory of the probe brane are compared to those…

High Energy Physics - Theory · Physics 2010-02-03 E. Kiritsis

We investigate a possibility of reheating in a scenario of D-brane inflation in a warped deformed conifold background which includes perturbative corrections to throat geometry sourced by chiral operator of dimension 3/2 in the CFT. The…

High Energy Physics - Theory · Physics 2010-05-25 Sudhakar Panda , M. Sami , I. Thongkool

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

In expanding universes, the entanglement entropy must be time-dependent because the background geometry changes with time. For understanding time evolution of quantum correlations, we take into account two distinct holographic models, the…

High Energy Physics - Theory · Physics 2021-07-07 Chanyong Park