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The spacetime physics of bulk closed string tachyon condensation is studied at the level of a two-derivative effective action. We derive the unique perturbative tachyon potential consistent with a full class of linearized tachyonic…

High Energy Physics - Theory · Physics 2008-11-26 Ian Swanson

The electric Weak Gravity Conjecture demands that axions with large decay constant $f$ couple to light instantons. The resulting large instantonic corrections pose problems for natural inflation. We explore an alternative argument based on…

High Energy Physics - Theory · Physics 2017-04-26 Arthur Hebecker , Philipp Henkenjohann , Lukas T. Witkowski

We propose a model for large field inflation in heterotic string theory. The construction applies the near alignment mechanism of Kim, Nilles, and Peloso. By including gaugino condensates and world-sheet instanton non-perturbative effects,…

High Energy Physics - Theory · Physics 2015-04-16 Tibra Ali , S. Shajidul Haque , Vishnu Jejjala

We study Abelian strings in a fixed de Sitter background. We find that the gauge and Higgs fields extend smoothly across the cosmological horizon and that the string solutions have oscillating scalar fields outside the cosmological horizon…

High Energy Physics - Theory · Physics 2008-11-26 Yves Brihaye , Betti Hartmann

Some of the phenomenological implications of string cosmological models are reviewed, with particular attention to the spectra of the tensor, scalar and vector modes of the geometry. A class of self-dual string cosmological models is…

High Energy Physics - Theory · Physics 2007-05-23 Massimo Giovannini

We find solutions of Einstein's field equation for topologically stable strings associated with the breaking of a U(1) symmetry. Strings form in many GUTs and are expected whenever the homotopy group $\Pi_1(M_0)$ is non-trivial. The…

Astrophysics · Physics 2009-10-22 Charles C. Dyer , Francine R. Marleau

In this note we show that models of natural inflation based on closed string axions are incompatible with the weak gravity conjecture (WGC). Specifically, we use T-duality in order to map the bounds on the charge-to-mass ratio of particles…

High Energy Physics - Theory · Physics 2015-04-20 Jon Brown , William Cottrell , Gary Shiu , Pablo Soler

We provide a compact review on recent developments on axion $F(R)$ gravity. The axion field is a string theory originating theoretical particle that is a perfect candidate for low-mass particle dark matter. In this review we present how a…

General Relativity and Quantum Cosmology · Physics 2020-04-22 S. D. Odintsov , V. K. Oikonomou

Axion fields provide the most elegant solution to the strong CP problem. In string compactifications it is difficult to obtain an axion whose decay constant is consistent with current cosmological bounds. We examine this question in…

High Energy Physics - Theory · Physics 2014-11-18 Kang-Sin Choi , Hans Peter Nilles , Saul Ramos-Sanchez , Patrick K. S. Vaudrevange

We have studied numerically the evolution and decay of axion strings. These global defects decay mainly by axion emission and thus contribute to the cosmological axion density. The relative importance of this source relative to misalignment…

High Energy Physics - Phenomenology · Physics 2009-10-31 C. Hagmann , S. Chang , P. Sikivie

The static stationary axially symmetric background ("infinite cosmic string") of the $D=4$ string theory provided with an axion charge is studied in the effective theory approach. The most general exact solution is constructed. It is found…

High Energy Physics - Theory · Physics 2009-10-22 Nemanja Kaloper

In the context of string theory, axions appear to provide the most plausible solution of the strong CP problem. However, as has been known for a long time, in many string-based models, the axion coupling parameter F_a is several orders of…

High Energy Physics - Theory · Physics 2010-04-07 Peter Svrcek , Edward Witten

An exploratory study of the cosmology of moduli in string theory. Moduli are argued to be natural inflaton fields and lead to a robust inflationary cosmology in which inflation takes place at the top of domain walls. The amplitude of…

High Energy Physics - Theory · Physics 2016-09-06 T. Banks , M. Berkooz , G. Moore , S. H. Shenker , P. J. Steinhardt

This paper is about the use of a novel, exact functional quantization method as applied to two commonly studied actions in theoretical physics. The functional method in question has its roots in the exact renormalisation group flow…

High Energy Physics - Theory · Physics 2012-12-20 Dylan Tanner

We investigate the validity of effective field theory methods and the decoupling of heavy fields during inflation. Considering models of inflation in which the inflaton is coupled to a heavy (super-Hubble) degree of freedom initially in its…

These lectures present a brief review of inflationary cosmology, provide an overview of the theory of cosmological perturbations, and then focus on the conceptual problems of the current paradigm of early universe cosmology, thus motivating…

High Energy Physics - Theory · Physics 2009-01-30 Robert Brandenberger

In supersymmetric theories, the Peccei-Quinn symmetry has a complex extension as a symmetry of the superpotential, so that the scalar potential always has an almost flat direction, the dilaton. We discuss how coherent oscillation of the…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Hashimoto , K. -I. Izawa , M. Yamaguchi , T. Yanagida

We study an effective four-dimensional theory with an action with two scalar fields minimally coupled to gravity, and with a matter action which couples to the two scalar fields via an overall field-dependent coefficient in the action. Such…

High Energy Physics - Theory · Physics 2009-11-11 Tirthabir Biswas , Robert Brandenberger , Damien A. Easson , Anupam Mazumdar

In this paper we study regular cosmic string solutions of the non-Abelian Higgs model coupled with the Einstein gravity. In order to do that, we constructed a set of coupled differential ordinary equation. Because there is no closed…

High Energy Physics - Theory · Physics 2015-07-08 Antônio de Pádua Santos , Eugênio R. Bezerra de Mello

Understanding axion cosmology has important experimental consequences since it constrains the range of allowed values for the axion mass. In the standard thermal scenario, which assumes Peccei-Quinn symmetry restoration after inflation, an…

Astrophysics · Physics 2007-05-23 R. A. Battye , E. P. S. Shellard