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We consider cosmological consequences of string theory tachyon condensation. We show that it is very difficult to obtain inflation in the simplest versions of this theory. Typically, inflation in these theories could occur only at…

High Energy Physics - Theory · Physics 2009-11-07 Lev Kofman , Andrei Linde

The coupling between a pseudo-scalar inflaton and a gauge field leads to an amount of additional density perturbations and gravitational waves (GWs) that is strongly sensitive to the inflaton speed. This naturally results in enhanced GWs at…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-24 Juan Garcia-Bellido , Alexandros Papageorgiou , Marco Peloso , Lorenzo Sorbo

We present inflationary models of the early universe in the braneworld scenario considering both scalar field and tachyon field separately. The technique of Chervon and Zhuravlev to obtain inflationary cosmological models without…

High Energy Physics - Theory · Physics 2007-08-08 B. C. Paul , Dilip Paul

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

We propose a field theory for describing the tachyon on a brane-antibrane system near the minimum of the potential. This field theory realizes two known properties of the tachyon effective action: 1) absence of plane-wave solutions around…

High Energy Physics - Theory · Physics 2009-09-15 Ashoke Sen

An unstable $D3$-brane universe governed by the DBI action of the tachyon field minimally coupled to a U(1) gauge boson is examined. The cosmological evolution of this coupled system, is further analyzed, in terms of the expansion rate of…

High Energy Physics - Theory · Physics 2009-11-11 Anastasios Psinas

We study inflation and reheating in models for the brane universe, considering hybrid brane inflation without tachyon condensation. We expect that some fields that are localized on different branes interact with O(1) coupling when branes…

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

We study brane-world preheating in massive chaotic inflationary scenario where scalar fields are confined on the 3-brane. Assuming that quadratic contribution in energy densities dominates the Hubble expansion rate during preheating, the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Shinji Tsujikawa , Kei-ichi Maeda , Shuntaro Mizuno

Previous studies demonstrate that the inflaton, when coupled to the hypercharge Chern-Simons density, can source an explosive production of helical hypermagnetic fields. Then, in the absence of fermion production, those fields have the…

High Energy Physics - Phenomenology · Physics 2023-06-21 Yann Cado , Mariano Quirós

We study the explosive production of gauge fields during axion inflation in a novel gradient expansion formalism that describes the time evolution of a set of bilinear electromagnetic functions in position space. Based on this formalism, we…

High Energy Physics - Phenomenology · Physics 2021-12-06 E. V. Gorbar , K. Schmitz , O. O. Sobol , S. I. Vilchinskii

We present an analytic solution for tachyon condensation on a non-BPS D-brane in Berkovits' open superstring field theory. The solution is presented as a product of $2\times 2$ matrices in two distinct $GL_2$ subgroups of the open string…

High Energy Physics - Theory · Physics 2015-06-16 Theodore Erler

Using boundary string field theory we study the decay of unstable D-branes to lower dimensional D-branes via the tachyon condensation at one loop level. We analyze one loop divergences and use the Fischler-Susskind mechanism to cancel…

High Energy Physics - Theory · Physics 2007-05-23 D. Nemeschansky , V. Yasnov

It has been shown recently that by turning on a large noncommutativity parameter, the description of tachyon condensation in string theory can be drastically simplified. We reconsider these issues from the standpoint of string field theory,…

High Energy Physics - Theory · Physics 2007-05-23 E. Witten

We study inflation arising from the motion of a BPS D3-brane in the background of a stack of k parallel D5-branes. There are two scalar fields in this set up-- (i) the radion field R, a real scalar field, and (ii) a complex tachyonic scalar…

High Energy Physics - Theory · Physics 2008-11-26 Sudhakar Panda , M. Sami , Shinji Tsujikawa , John Ward

In this talk, I review briefly a scenario for the evolution of a string-inspired cosmological model, in which condensates of primordial gravitational waves (GW), formed at the very early eras after the Big Bang, are considered responsible…

General Relativity and Quantum Cosmology · Physics 2020-03-26 Nikolaos E. Mavromatos

Using the construction of D-branes with nonzero $B$ field in the matrix model we give a physical interpretation of the known background independence in gauge theories on a noncommutative space. The background independent variables are…

High Energy Physics - Theory · Physics 2009-10-31 Nathan Seiberg

We compute the one-loop partition function for quadratic tachyon background in open string theory. Both closed and open string representations are developed. Using these representations we study the one-loop divergences in the partition…

High Energy Physics - Theory · Physics 2007-05-23 K. Bardakci , A. Konechny

We analyze the fate of excitations in regions of closed string tachyon condensate, a question crucial for understanding unitarity in a class of black holes in string theory. First we introduce a simple new example of {\it quasilocal}…

High Energy Physics - Theory · Physics 2008-11-26 Gary T. Horowitz , Eva Silverstein

String theory generically predicts the coupling between the Affleck-Dine field and axion field through higher-dimensional operators. We thus explore the Affleck-Dine baryogenesis on an axion background. It turns out that the axion…

High Energy Physics - Phenomenology · Physics 2017-04-28 Kensuke Akita , Tatsuo Kobayashi , Hajime Otsuka

We demonstrate that string motivated inflation ending via tachyonic instability leaves a detectable imprint on the cosmic microwave background (CMB) radiation by virtue of the excitation of non-Gaussian gravitational fluctuations. The…

High Energy Physics - Theory · Physics 2007-05-23 Kari Enqvist , Asko Jokinen , Anupam Mazumdar , Tuomas Multamaki , Antti Vaihkonen