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Related papers: Axions as Quintessence in String Theory

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The weakly-coupled heterotic string is known to have problems of dilaton/moduli stabilization, supersymmetry breaking (by hidden-sector gaugino condensation), gauge coupling unification (or the Newton's constant), QCD axion, as well as…

High Energy Physics - Theory · Physics 2007-05-23 Yi-Yen Wu

At present we know nothing about the nature of the dark energy accounting for about 70% of the energy density of the Universe. One possibility is that the dark energy is provided by an extremely light field, the quintessence, rolling down…

High Energy Physics - Phenomenology · Physics 2009-11-07 D. J. H. Chung , L. L. Everett , A. Riotto

We argue that, for generic string compactifications, dark energy is likely to signal the beginning of the end of our universe, perhaps even through decompactification, with possible implications for the cosmological coincidence problem.…

High Energy Physics - Theory · Physics 2021-10-27 Francesc Cunillera , Antonio Padilla

Using tachyon or quintessence fields along with a barotropic fluid on the brane we examine the different cosmological stages in a Friedmann-Robertson-Walker(FRW) universe, from the first radiation scenario to the later era dominated by…

General Relativity and Quantum Cosmology · Physics 2011-08-11 Luis P. Chimento , Monica Forte , Gilberto M. Kremer , Martin G. Richarte

A generic prediction of string theory is the existence of many axion fields. It has recently been argued that many of these fields should be light and, like the well known QCD axion, lead to observable cosmological consequences. In this…

Cosmology and Nongalactic Astrophysics · Physics 2013-02-19 David J. E. Marsh , Edward Macaulay , Maxime Trebitsch , Pedro G. Ferreira

We present updated constraints on an interacting dark energy - dark matter model with pure momentum transfer, where dark energy is in the form of a quintessence scalar field with an exponential potential. We run a suite of MCMC analyses…

Cosmology and Nongalactic Astrophysics · Physics 2026-02-09 Alkistis Pourtsidou

We consider a supersymmetric system of D-5-branes compactified on a 5-torus with a self-dual background field strength on a 4-torus and carrying left-moving momentum along a circle. The corresponding supergravity solution describes a…

High Energy Physics - Theory · Physics 2010-11-19 Miguel S. Costa , Malcolm J. Perry

We describe properties of the M-theory five-brane containing $Q$ coincident self-dual strings on its worldvolume. This is the five-brane description of Q membranes ending on the five-brane. In particular, we consider a Maldacena-like low…

High Energy Physics - Theory · Physics 2009-11-07 D. S. Berman , P. Sundell

Motivated by the M-theory compactification physics, we study a type IIA superstring quiver model with an open string axion field associated with the U(1)_{PQ} Peccei-Quinn global symmetry using D6-brane physics. This realization extends the…

High Energy Physics - Theory · Physics 2017-10-24 Adil Belhaj , Salah-Eddine Ennadifi

Quintessence is a canonical scalar field introduced to explain the late-time cosmic acceleration. The cosmological dynamics of quintessence is reviewed, paying particular attention to the evolution of the dark energy equation of state w.…

General Relativity and Quantum Cosmology · Physics 2015-06-15 Shinji Tsujikawa

We derive some consistency conditions for fivebrane in M theory on R^5/Z_2 orbifold from the quantization law for the antisymmetric tensor field. We construct consistent fivebrane configurations in R^5/Z_2 type orbifold that exhibit the…

High Energy Physics - Theory · Physics 2014-11-18 Kentaro Hori

The dark dimension scenario, which is motivated from Swampland principles and predicts a single micron scale extra dimension, suggests a consistent framework for the dark sector of the universe. We consider the implications of this scenario…

High Energy Physics - Theory · Physics 2024-07-18 Naomi Gendler , Cumrun Vafa

We study the dynamics near a 1+1 dimensional intersection of two orthogonal stacks of fivebranes in type IIB string theory, using an open string description valid at weak coupling, and a closed string description valid at strong coupling.…

High Energy Physics - Theory · Physics 2009-11-11 Nissan Itzhaki , David Kutasov , Nathan Seiberg

We study M theory fivebranes to understand the moduli space of vacua of N=1 supersymmetric SO(N_c) gauge theory with N_f flavors in four dimensions. We discuss how the various branches of this theory arise in the string/M theory brane…

High Energy Physics - Theory · Physics 2014-11-18 Changhyun Ahn , Kyungho Oh , Radu Tatar

The QCD axion stands as one of the most promising candidates for resolving the strong CP problem. However, the value of the axion's decay constant $f_a$ and, by extension, its mass $m_a$, remain uncertain within the framework of effective…

High Energy Physics - Phenomenology · Physics 2024-11-01 Qiaoli Yang , Runchao Huang

Consistent frameworks of quantum gravity often predict the existence of large numbers of ultralight pseudoscalar degrees of freedom, forming the phenomenological landscape of the String Axiverse. The complexity of the extra-dimensional…

High Energy Physics - Theory · Physics 2018-11-15 Matthew J. Stott

We provide evidence that slow roll is not possible in any parametrically controlled regime of the moduli space of string theory. This is proven in full generality in the asymptotic limit of the moduli space of type II and heterotic…

High Energy Physics - Theory · Physics 2022-04-20 Michele Cicoli , Francesc Cunillera , Antonio Padilla , Francisco G. Pedro

We review the status of solitons in superstring theory, with a view to understanding the strong coupling regime. These {\it solitonic} solutions are non-singular field configurations which solve the empty-space low-energy field equations…

High Energy Physics - Theory · Physics 2008-11-26 M. J. Duff , Ramzi R. Khuri , J. X. Lu

In this talk we present a model of the universe in which dark energy is modelled explicitely with both a dynamical quintessence field and a cosmological constant. Our results confirm the possibility of a collapsing universe (for a given…

Astrophysics · Physics 2007-05-23 Rolando Cardenas , Tame Gonzalez , Osmel Martin , Israel Quiros

I review the dark energy solutions by a very light pseudoscalar called "quintessential axion". For the explicit breaking terms, we consider both the global anomaly U(1)$_{\rm global}\times$SU(2)$_W^2$ and the potential $\Delta V$. At the…

High Energy Physics - Phenomenology · Physics 2022-08-03 Jihn E. Kim