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We examine variations in the equation of state of the cosmic string portion of the cosmological fluid which lead to perturbations of the background matter density. These fluctuations in the equation of state are due to variations in the…

Astrophysics · Physics 2010-01-06 Pedro Avelino , Robert Caldwell

We explicitly compute the Compton amplitude for the scattering of a photon and a (massless) ``electron/positron'' at tree level and one loop, in a four-dimensional fermionic heterotic string model. We comment on the relationship between the…

High Energy Physics - Theory · Physics 2009-10-30 A. Pasquinucci , M. Petrini

An infinite number of distinct $d=1$ matrix models reproduce the perturbation theory of $d=2$ string theory. Due to constraints of causality, however, we argue that none of the existing constructions gives a consistent nonperturbative…

High Energy Physics - Theory · Physics 2009-10-09 Joseph Polchinski

This essay presents a critical evaluation of the concepts of string theory and its impact on particle physics. The point of departure is a historical review of four decades of ST within the broader context of six decades of failed attempts…

High Energy Physics - Theory · Physics 2010-12-06 Bert Schroer

It has long been thought that a highly excited string can be regarded as a black hole: the correspondence principle between strings and a black hole, while recent studies found that black holes are characterized by chaos. This suggests that…

High Energy Physics - Theory · Physics 2022-12-14 Koji Hashimoto , Yoshinori Matsuo , Takuya Yoda

In the background of several holographic confining backgrounds, we present the connections between the behaviors of string scattering amplitudes and mutual information. We lay down the analogies between the logarithmic branch cut behavior…

High Energy Physics - Theory · Physics 2025-08-18 Mahdis Ghodrati

It is shown that the multiplicity distribution associated to self-shadowing events satisfies an universal equation in terms of the minimum bias distribution. The number of elementary collisions, basic in the structure of any multiple…

High Energy Physics - Phenomenology · Physics 2007-05-23 C. Pajares , C. A. Salgado , E. G. Ferreiro

We present a class of solvable models that resemble string theories in many respects but have a strikingly different non-perturbative sector. In particular, there are no exponentially small contributions to perturbation theory in the string…

High Energy Physics - Theory · Physics 2007-05-23 Clifford V. Johnson

We propose a novel string theory propagating in a non-commutative deformation of the four dimensional space T* T^2 whose scattering states correspond to superconformal theories in 5 dimensions and the scattering amplitudes compute…

High Energy Physics - Theory · Physics 2012-09-13 Cumrun Vafa

We summarize recent work, in which we consider scattering amplitudes of non-critical strings in the limit where the energy of all external states is large compared to the string tension. We show that the high energy limit is dominated by a…

High Energy Physics - Theory · Physics 2014-11-18 Kenichiro Aoki , Eric D'Hoker

The interaction energy and force between widely separated strings is analyzed in a field theory having applications to superconducting cosmic strings, the SO(5) model of high-temperature superconductivity, and solitons in nonlinear optics.…

High Energy Physics - Theory · Physics 2009-11-10 R. MacKenzie , M. -A. Vachon , U. F. Wichoski

Perturbative scattering amplitudes in Yang-Mills theory have many unexpected properties, such as holomorphy of the maximally helicity violating amplitudes. To interpret these results, we Fourier transform the scattering amplitudes from…

High Energy Physics - Theory · Physics 2010-04-07 Edward Witten

Lorentz invariance, unitarity, and causality enforce powerful constraints on the theory space of physical scattering amplitudes. However, virtually all efforts in this direction have centered on the very simplest case of four-point…

High Energy Physics - Theory · Physics 2025-07-17 Clifford Cheung , Grant N. Remmen

Within two specific string cosmology scenarios --differing in the way the pre- and post-big bang phases are joined-- we compute the size and spectral slope of various types of cosmologically amplified quantum fluctuations that arise in…

High Energy Physics - Theory · Physics 2009-10-30 A. Buonanno , K. Meissner , C. Ungarelli , G. Veneziano

String theory, if it describes nature, is probably strongly coupled. As a result, one might despair of making any statements about the theory. In the framework of a set of clearly spelled out assumptions, we show that this is not…

High Energy Physics - Theory · Physics 2013-11-13 T. Banks , M. Dine

It has been known for about thirty years that a scattering amplitude involving D0-branes and closed strings suffers from infrared divergences beyond tree level. These divergences arise because the conventional world-sheet approach cannot…

High Energy Physics - Theory · Physics 2025-12-09 Ashoke Sen , Bogdan Stefański

Ultrahigh-energy string scattering is investigated to clarify the relative role of string and gravitational effects, and their possible contributions to nonlocal behavior. Different regimes can be characterized by varying the impact…

High Energy Physics - Theory · Physics 2008-11-26 Steven B. Giddings , David J. Gross , Anshuman Maharana

We make some remarks on possible definition of open string path integral in the presence of additional boundary couplings corresponding to the presence of masses at the ends of the string. These couplings are not conformally invariant…

High Energy Physics - Theory · Physics 2020-11-12 A. A. Tseytlin

We discuss the breakdown of perturbative unitarity of noncommutative quantum field theories in electric-type background in the light of string theory. We consider the analytic structure of string loop two-point functions using a suitable…

High Energy Physics - Theory · Physics 2009-11-07 Alessandro Torrielli

We study the impact of fragmentation on the cosmic string loop number density, using an approach inspired by the three-scale model and a Boltzmann equation. We build a new formulation designed to be more amenable to numerical resolution and…

Cosmology and Nongalactic Astrophysics · Physics 2025-12-12 Pierre Auclair
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