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Related papers: Quintessence with two energy scales

200 papers

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

The value of scalar field coupled to gravity should be less than the Planck scale in the consistent theory of quantum gravity. It provides a theoretic constraint on the equation of state parameter for the quintessence. In some cases our…

Astrophysics · Physics 2008-11-26 Qing-Guo Huang

We study some conditions for the hierarchy $m_{3/2} << M_P$ to occur naturally in a generic effective supergravity theory. Absence of fine-tuning and perturbative calculability require that the effective potential has a sliding gravitino…

High Energy Physics - Theory · Physics 2014-11-18 S. Ferrara , C. Kounnas , F. Zwirner

Planck scale physics represents a future challenge, located between particle physics and general relativity. The Planck scale marks a threshold beyond which the old description of spacetime breaks down and conceptually new phenomena must…

High Energy Physics - Phenomenology · Physics 2009-11-10 Sabine Hossenfelder

Quintessence with a potential motivated by supergravity (SUGRA) exhibits several intriguing features. Depending on its initial conditions, it can behave either as dynamical dark energy or effectively as a cosmological constant. Moreover,…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-19 Jincheng Wang , Hongwei Yu , Puxun Wu

We investigate a class of theories involving a symmetric two-tensor field in Minkowski spacetime with a potential triggering spontaneous violation of Lorentz symmetry. The resulting massless Nambu-Goldstone modes are shown to obey the…

General Relativity and Quantum Cosmology · Physics 2015-05-13 Alan Kostelecky , Robertus Potting

We propose a simple, well-motivated and robust alternative to a metastable de Sitter vacuum in string theory, consistent with current observations of dark energy and naturally satisfying conjectured swampland constraints. Inflation ends in…

High Energy Physics - Theory · Physics 2019-01-23 Yessenia Olguin-Trejo , Susha L. Parameswaran , Gianmassimo Tasinato , Ivonne Zavala

A slow-rolling scalar field ($Q\equiv$ Quintessence) with potential energy $V_Q\sim (3\times 10^{-3} {\rm eV})^4$ has been proposed as the origin of accelerating universe at present. We investigate the effective potential of $Q$ in the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Kiwoon Choi

We argue that quintessence may reside in certain corners of the string landscape. It arises as a linear combination of internal space components of higher rank forms, which are axion-like at low energies, and may mix with 4-forms after…

High Energy Physics - Theory · Physics 2009-04-13 Nemanja Kaloper , Lorenzo Sorbo

String and field theory ideas have greatly influenced each other since the so called second string revolution. We review this interrelation paying particular attention to its phenomenological implications. Our guiding principle is the…

High Energy Physics - Phenomenology · Physics 2010-01-08 S. A. Abel , J. Santiago

The search for a theory of quantum gravity faces two great challenges: the incredibly small scales of the Planck length and time, and the possibility that the observed constants of nature are in part the result of random processes. A…

High Energy Physics - Theory · Physics 2015-12-17 Joseph Polchinski

The evolution of the quintessence field during a phase of chaotic inflation is studied. The inflaton and the quintesssence field are described in a supergravity framework where the coupling between the inflaton and quintessence is induced…

Astrophysics · Physics 2008-11-26 Philippe Brax , Jerome Martin

In this letter, it is obtained using dual role of the Ricci scalar (physical as well as geometrical role of the Ricci scalar curvature) in a natural way without any input in the theory for it. In contrast to other models, where an idea for…

Astrophysics · Physics 2007-05-23 S. K. Srivastava

We describe a model of hybrid quintessence in which in addition to the tracker field there is a trigger field which is responsible for ending quintessence. As a result, hybrid quintessence does not suffer from the problems associated with…

High Energy Physics - Phenomenology · Physics 2010-02-03 Edi Halyo

The subject of this thesis is cosmological implications of string compactifications understood in a broad sense. In the first half of the thesis, we will begin by reviewing the four-dimensional description of the tree-level perturbative…

High Energy Physics - Theory · Physics 2022-08-02 Francesc Cunillera

The physics of supersymmetry is reviewed from the perspective of physics at ever increasing energies. Starting from the minimal supersymmetric extension of the Standard Model at the electroweak scale, we proceed to higher energies seeking…

High Energy Physics - Phenomenology · Physics 2016-09-01 J. Lopez

A slow-rolling scalar field (Quintessence) has been proposed as the origin of accelerating universe at present. We discuss some features of quintessence, particularly those related with the {\it flatness} of its potential. We distinguish…

High Energy Physics - Phenomenology · Physics 2007-05-23 Kiwoon Choi

General forms of the K\"ahler and superpotenials that lead to consistent low energy broken Supersymmetry originating from $N=1$ Supergravity have been classified and used for model building since more than three decades. We point out the…

High Energy Physics - Theory · Physics 2018-11-27 Gilbert Moultaka , Michel Rausch de Traubenberg , Damien Tant

In scale-invariant theories of gravity the Planck mass $M_P$, which appears due to spontaneous symmetry breaking, can be the only scale at the classical level. It was argued that the second scale can be generated by a quantum…

High Energy Physics - Theory · Physics 2019-06-24 Andrey Shkerin

We investigate the extent to which quintessence models for dark energy are fine-tuned in the context of recent swampland conjectures. In particular, the issue is whether there is a double fine-tuning in which both $V$ and $|\nabla V|$ are…

High Energy Physics - Theory · Physics 2019-09-06 Mark P. Hertzberg , McCullen Sandora , Mark Trodden