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Related papers: Stringy multifield quintessence and the Swampland

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We describe some recent progress in understanding and formulating string theory which is based on extensive studies of strings in lower (D=2) dimension. At the center is a large $W_{\infty}$ symmetry that appears most simply in the matrix…

High Energy Physics - Theory · Physics 2007-05-23 A. Jevicki

We review recent progress in string cosmology, where string dualities are applied so as to obtain complete cosmological evolutions, free of any essential singularities. Two classes of models are analyzed. The first class consists of string…

High Energy Physics - Theory · Physics 2013-05-28 Costas Kounnas , Nicolaos Toumbas

In a previous paper (hep-th/0509067) using matrix model, we showed that closed string tachyons can resolve spacelike singularity in one particular class of Misner space (with anti-periodic boundary conditions for fermions around the spatial…

High Energy Physics - Theory · Physics 2008-11-26 Jian-Huang She

We extend the swampland from effective field theories (EFTs) inconsistent with quantum gravity to EFTs inconsistent with quantum supergravity. This enlarges the swampland to include EFTs that become inconsistent when the gravitino is…

High Energy Physics - Theory · Physics 2021-09-29 Edward W. Kolb , Andrew J. Long , Evan McDonough

This is a set of lectures on the gauge/string duality and non-critical strings, with a particular emphasis on the discretized, or matrix model, approach. After a general discussion of various points of view, I describe the recent…

High Energy Physics - Theory · Physics 2007-05-23 Frank Ferrari

I discuss cosmological models either derived from, or inspired by, string theory or M-theory. In particular I discuss solutions in the low-energy effective theory and the role of the dilaton, moduli and antisymmetric form fields in the…

High Energy Physics - Theory · Physics 2009-11-07 David Wands

The status of string theory is reviewed, and major recent developments - especially those in going beyond perturbation theory in the string theory and quantum field theory frameworks - are discussed. This analysis helps better understand…

High Energy Physics - Theory · Physics 2010-12-17 A. Marshakov

Supersymmetry breaking in string theory is expected to occur when moduli fields acquire non-trivial expectation values. In the early universe these fields start out displaced from their final destinations. I present some recent ideas about…

High Energy Physics - Theory · Physics 2007-05-23 R. Brustein

Taking into account the recently proposed poly-instanton corrections to the superpotential and combining the race-track with a KKLT respectively LARGE Volume Scenario in an intricate manner, we show that we gain exponential control over the…

High Energy Physics - Theory · Physics 2009-02-23 Ralph Blumenhagen , Sebastian Moster , Erik Plauschinn

Quantum Field Theory (QFT) introduced us to the notion that a causal diamond in space-time corresponded to a subsystem of a quantum mechanical system defined on the global space-time. Work by Jacobson\cite{ted95}, Fischler and…

High Energy Physics - Theory · Physics 2025-09-23 T. Banks

String theory has no parameter except the string scale $M_S$, so the Planck scale $M_\text{Pl}$, the supersymmetry-breaking scale, the EW scale $m_\text{EW}$ as well as the vacuum energy density (cosmological constant) $\Lambda$ are to be…

High Energy Physics - Theory · Physics 2021-01-25 Yu-Cheng Qiu , S. -H. Henry Tye

String theory axions appear to be promising candidates for explaining cosmological constant via quintessence. In this paper, we study conditions on the string compactifications under which axion quintessence can happen. For sufficiently…

High Energy Physics - Theory · Physics 2007-05-23 Peter Svrcek

There are effective field theories that cannot be embedded in any UV complete theory. We consider scalar effective field theories, with and without dynamical gravity, in $D$-dimensional anti-de Sitter (AdS) spacetime with large radius and…

High Energy Physics - Theory · Physics 2022-02-16 Sandipan Kundu

Recently, many works have tried to realize cosmological accelerated expansion in string theory models in the asymptotic regions of field space, with a typical scalar potential $V(\varphi)$ having an exponential fall-off $e^{-\gamma\,…

High Energy Physics - Theory · Physics 2023-11-17 David Andriot , Dimitrios Tsimpis , Timm Wrase

The fundamental string length, which is an essential part of string theory, explicitly breaks scale invariance. However, in field theory we demonstrated recently that the gravitational constant, which is directly related to the string…

High Energy Physics - Theory · Physics 2015-06-22 Itzhak Bars , Paul Steinhardt , Neil Turok

We analyze AdS and dS swampland conjectures in a three-dimensional higher spin theory with self-interacting matter, which contains conformal gravity and is almost topological. A theory of a similar type was proposed as the effective theory…

High Energy Physics - Theory · Physics 2022-01-20 Rafael Álvarez-García , Ralph Blumenhagen , Christian Kneissl , Andriana Makridou , Lorenz Schlechter

We study the nonlinear realization of supersymmetry in a dynamical/cosmological background in which derivative terms like kinetic terms are finite. Starting from linearly realized theories, we integrate out heavy modes without neglecting…

High Energy Physics - Theory · Physics 2022-02-24 Shuntaro Aoki , Takahiro Terada

We construct a model of quintessence in string theory based on the idea of axion monodromy as discussed by McAllister, Silverstein and Westphal arXiv:0808.0706. In the model, the quintessence field is an axion whose shift symmetry is broken…

High Energy Physics - Theory · Physics 2011-04-22 Sudhakar Panda , Yoske Sumitomo , Sandip P. Trivedi

Recent observations suggest that the accelerated expansion of the Universe at late times is caused by a temporally changing dark energy component, rather than the constant one in the standard $\Lambda$CDM scenario. In this context…

General Relativity and Quantum Cosmology · Physics 2025-11-05 Artur Alho , Elsa Bernholm , Claes Uggla

We study the cosmological evolution of scalar fields with arbitrary potentials in the presence of a barotropic fluid (matter or radiation) without making any assumption on which term dominates. We determine what kind of potentials V(phi)…

High Energy Physics - Phenomenology · Physics 2013-05-29 A. de la Macorra , G. Piccinelli