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Related papers: de Sitter State in Heterotic String Theory

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The states of a single photon in four-dimensional de Sitter (dS) spacetime form a Unitary Irreducible Representation (UIR) of SO(1,4), which we call the photon UIR. While in flat spacetime photons are intimately tied to gauge symmetry, we…

High Energy Physics - Theory · Physics 2025-12-03 Manuel Loparco , Joao Penedones , Yannis Ulrich

We propose a complete microscopic definition of the Hilbert space of minimal higher spin de Sitter quantum gravity and its Hartle-Hawking vacuum state. The fundamental degrees of freedom are $2N$ bosonic fields living on the future…

High Energy Physics - Theory · Physics 2017-11-29 Dionysios Anninos , Frederik Denef , Ruben Monten , Zimo Sun

Perturbative gravity in global de Sitter space is subject to so-called linearization stability constraints: If they are to couple consistently to the gravitational field, quantum states must be invariant under the de Sitter isometries.…

General Relativity and Quantum Cosmology · Physics 2009-01-16 Donald Marolf , Ian A. Morrison

We consider a general dynamical, spherically symmetric background in the cubic subclass of Horndeski theory and obtain the quadratic action for the perturbations using the DPSV approach. We analyse the stability conditions for high-energy…

High Energy Physics - Theory · Physics 2025-06-03 S. Mironov , M. Sharov

In order for spacetimes with static extra dimensions to have 4-dimensional de Sitter expansion they must have at least positive curvature, warping sourced by the 4-d expansion, or violate the null energy condition everywhere in the extra…

High Energy Physics - Theory · Physics 2019-08-28 Saurya Das , S. Shajidul Haque , Bret Underwood

In $D=3,4,6$ and 10 space--time dimensions considered is a string model invariant under transformations of $N=1$ space--time supersymmetry and $n=D-2$ local worldsheet supersymmetry with the both Virasoro constraints solved in the twistor…

High Energy Physics - Theory · Physics 2015-06-26 Igor A. Bandos , Martin Cederwall , Dmitrij P. Sorokin , Dmitrij V. Volkov

We consider the Euclidean vacuum for linearized gravity on the global de Sitter space, obtained from the Euclidean Green's function on the 4-sphere. We use the notion of Calder\'on projectors to recover a quantum state for the Lorentzian…

Mathematical Physics · Physics 2026-03-17 Christian Gérard , Michał Wrochna

We revisit the issue of uplifting the potential to de Sitter (dS) vacua in type IIB flux compactifications of Kachru, Kallosh, Linde and Trivedi (KKLT). We shed light on some tension between two constraints on dS vacua in type IIB string…

High Energy Physics - Theory · Physics 2016-07-06 Nana Cabo Bizet , Shinji Hirano

We employ holographic duality to compute $\langle T_{\mu \nu} \rangle$ in strongly coupled $\mathcal N = 4$ supersymmetric Yang-Mills theory and then study evolution of the semiclassical Einstein field equations sourced by $\langle T_{\mu…

High Energy Physics - Theory · Physics 2020-11-11 Paul M. Chesler , Abraham Loeb

We present a 4-dimensional back reaction analysis of de Sitter space for a conformally coupled scalar field in the presence of vacuum energy initialized in the Bunch-Davies vacuum. In contrast to the usual semi-classical prescription, as…

General Relativity and Quantum Cosmology · Physics 2018-09-25 Tommi Markkanen

In the model of de Sitter gauge theory of gravity, the empty homogenous and isotropic spacetimes with constant curvature scalar and nonvanishing homogenous and isotropic torsion must have de Sitter metrics. The static de Sitter spacetime…

General Relativity and Quantum Cosmology · Physics 2009-11-05 Chao-Guang Huang , Meng-Sen Ma

Maximally symmetric curved-brane solutions are studied in dilatonic braneworld models which realise the self-tuning of the effective four-dimensional cosmological constant. It is found that no vacua in which the brane has de Sitter or…

High Energy Physics - Theory · Physics 2019-04-01 Jewel Kumar Ghosh , Elias Kiritsis , Francesco Nitti , Lukas T. Witkowski

The strong coupling regime of four-dimensional N=2 supersymmetric vacua of the heterotic string is analyzed from a dual domain wall perspective. Using modular invariance, we compute a closed form for the non-perturbative corrections to the…

High Energy Physics - Theory · Physics 2026-03-27 Mirjam Cvetič , Max Wiesner

Recent results on classical and quantum strings in a variety of black hole and cosmological spacetimes, in various dimensions, are presented. The curved backgrounds under consideration include the $2+1$ black hole anti de Sitter spacetime…

High Energy Physics - Theory · Physics 2016-08-15 A. L. Larsen , N. Sánchez

We quantize linearized Einstein-Hilbert gravity on de Sitter backgrounds in a covariant gauge. We verify the existence of a maximally-symmetric (i.e.de Sitter-invariant) Hadamard state $\Omega$ for all globally hyperbolic de Sitter…

General Relativity and Quantum Cosmology · Physics 2013-07-04 Ian A. Morrison

Exact and explicit string solutions in de Sitter spacetime are found. (Here, the string equations reduce to a sinh-Gordon model). A new feature without flat spacetime analogy appears: starting with a single world-sheet, several (here two)…

High Energy Physics - Theory · Physics 2009-10-22 H. J. de Vega , A. V. Mikhailov , N. Sanchez

Instabilities of two dimensional (1+1) de Sitter space induced by interacting fields are studied. As for the case of flat Minkowski space, several interacting fermion models can be translated into free boson ones and vice versa. It is found…

High Energy Physics - Theory · Physics 2014-11-20 Myron Bander

The r\^ole of string loop corrections on the existence of de Sitter vacua and the moduli stabilization problem is examined in type IIB effective theories. The fundamental building blocks are a minimum of three intersecting D7 brane stacks,…

High Energy Physics - Theory · Physics 2022-11-21 Vasileios Basiouris , George K. Leontaris

We perform string quantization in anti de Sitter (AdS) spacetime. The string motion is stable, oscillatory in time with real frequencies $\omega_n= \sqrt{n^2+m^2\alpha'^2H^2}$ and the string size and energy are bounded. The string…

High Energy Physics - Theory · Physics 2009-10-28 A. L. Larsen , N. Sanchez

Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a recently developed braneworld construction and known Anti-de Sitter (AdS) vacua to compute an explicit effective dS cosmology in three…

High Energy Physics - Theory · Physics 2022-02-16 Filip Landgren