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In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the vacuum fluctuations of the inflaton field corresponding to the position of the brane. We show that a significant, and possibly dominant,…

Astrophysics · Physics 2009-11-11 D. H. Lyth , A. Riotto

In this paper we study the tachyonic inflation in brane world cosmology with Gauss-Bonnet term in the bulk. We obtain the exact solution of slow roll equations in case of exponential potential. We attempt to implement the proposal of Lidsey…

High Energy Physics - Theory · Physics 2009-11-10 B. C. Paul , M. Sami

Using only general properties of the tachyon potential we show that inflation may be generic when many branes and anti-branes become coincident. Inflation may occur because of: (1) the assistance of the many diagonal tachyon fields; (2)…

High Energy Physics - Theory · Physics 2009-11-10 Mahbub Majumdar , Anne-Christine Davis

Topological defects are generically expected to form in models of brane inflation. Brane-anti-brane annihilation provides a way to gracefully end inflation, and the dynamics of the tachyon field results in defect formation. The formation of…

High Energy Physics - Theory · Physics 2008-11-26 Horace Stoica

The solution representing a brane-anti-brane system in matrix models breaks the usual matrix spacetime symmetry. We show that the spacetime symmetry on the branes is not breaking, rather appears as a combination of the matrix spacetime…

High Energy Physics - Theory · Physics 2010-11-19 Miao Li

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

Closed string tachyon condensation in spacetime generates potentials on the worldsheet that model two-dimensional inflationary cosmology. These models illustrate and elucidate a variety of aspects of inflation, in particular the generation…

High Energy Physics - Theory · Physics 2009-11-10 Bruno Carneiro da Cunha , Emil J. Martinec

In this paper we propose a new mechanism of inflating the Universe with non-BPS $D4$ branes which decay into stable $D3$ branes via tachyon condensation. In a single brane scenario the tachyon potential is very steep and unable to support…

High Energy Physics - Phenomenology · Physics 2009-11-07 Anupam Mazumdar , Sudhakar Panda , Abdel Pérez-Lorenzana

We perform canonical quantization of the open string on a unstable D-brane in the background of the tachyon condensation. Evaluating the Polyakov path-integral on a stripe, we obtain the field theoretical propagator in the open string…

High Energy Physics - Theory · Physics 2009-11-07 Taejin Lee

It has been conjectured that at a stationary point of the tachyon potential for the D-brane of bosonic string theory, the negative energy density exactly cancels the D-brane tension. We evaluate this tachyon potential by off-shell…

High Energy Physics - Theory · Physics 2009-10-31 Ashoke Sen , Barton Zwiebach

We present the study of the dynamics of the geometrical tachyon field on an unstable D3-brane in the background of a bulk tachyon field of a D3-brane solution of Type-0 string theory. We find that the geometrical tachyon potential is…

High Energy Physics - Theory · Physics 2007-05-23 Vassilios Zamarias

It is shown that classical decay of unstable D-branes in bosonic and superstring theories produces pressureless gas with non-zero energy density. The energy density is stored in the open string fields, even though around the minimum of the…

High Energy Physics - Theory · Physics 2009-11-07 Ashoke Sen

It has recently been realized that brane-antibrane annihilation (a possible explanation for ending inflation) may result in defect formation, due to the dynamics of the tachyon field. Studies of this possibility have generally ignored the…

High Energy Physics - Theory · Physics 2008-11-26 Guy D. Moore , Horace Stoica

We demonstrate the attractor behavior of inflation driven by a scalar field or a tachyon field in the context of recently proposed four-dimensional effective gravity induced on the world-volume of a three-brane in five-dimensional Einstein…

High Energy Physics - Phenomenology · Physics 2009-11-10 Zong-Kuan Guo , Hong-Sheng Zhang , Yuan-Zhong Zhang

We consider non-tachyonic hybrid inflation in the context of the braneworld cosmology. When one considers models for brane inflation, hybrid inflation is a natural consequence of the tachyon condensation if it appears at the end of…

High Energy Physics - Phenomenology · Physics 2009-11-10 Tomohiro Matsuda

We point out some intriguing analogies between field theoretic solitons (topological defects) and D-branes. Annihilating soliton-antisoliton pairs can produce stable solitons of lower dimensionality. Solitons that localize massless gauge…

High Energy Physics - Theory · Physics 2009-11-07 Gia Dvali , Alexander Vilenkin

We show that the naive application of the Kibble mechanism seriously underestimates the initial density of cosmic superstrings that can be formed during the annihilation of D-branes in the early universe, as in models of brane-antibrane…

High Energy Physics - Theory · Physics 2009-11-10 Neil Barnaby , Aaron Berndsen , James M. Cline , Horace Stoica

The level truncation approach to string field theory is used to study the zero-momentum action for vector excitations on a bosonic D-brane which has been annihilated by tachyon condensation. It is shown that in the true vacuum the…

High Energy Physics - Theory · Physics 2009-10-31 Washington Taylor

We consider the motion of the brane universe moving in a background bulk space of tachyonic and non-tachyonic type 0B string theory. The effective densities are calculated for both cases and they show different power law behavior. Brane…

High Energy Physics - Theory · Physics 2009-10-31 Jin Young Kim

We show that in hybrid inflation it is possible to generate large second-order perturbations in the cosmic microwave background due to the instability of the tachyonic field during preheating. We carefully calculate this effect from the…

Astrophysics · Physics 2009-11-11 Neil Barnaby , James M. Cline