TeV-scale gravity in Horava-Witten theory on a compact complex hyperbolic threefold
Chris Austin

TL;DR
This paper explores how compactification of Horava-Witten theory on a hyperbolic threefold can realize TeV-scale gravity via a thick pipe geometry, considering various stabilization mechanisms and implications for Standard Model fitting.
Contribution
It introduces a novel compactification setup on a hyperbolic threefold that achieves TeV-scale gravity and discusses multiple stabilization strategies for the extra dimensions.
Findings
Thick pipe geometry realizes TeV-scale gravity via the ADD mechanism.
Different stabilization methods for the outer boundary are analyzed.
Potential issues in fitting the Standard Model are discussed.
Abstract
The field equations and boundary conditions of Horava-Witten theory, compactified on a smooth compact spin quotient of CH^3, where CH^3 denotes the hyperbolic cousin of CP^3, are studied in the presence of Casimir energy density terms. If the Casimir energy densities near one boundary result in a certain constant of integration taking a value greater than around 10^5 in units of the d = 11 gravitational length, a form of thick pipe geometry is found that realizes TeV-scale gravity by the ADD mechanism, with that boundary becoming the inner surface of the thick pipe, where we live. Three alternative ways in which the outer surface of the thick pipe might be stabilized consistent with the observed value of the effective d = 4 cosmological constant are considered. In the first alternative, the outer surface is stabilized in the classical region and the constant of integration is fixed at…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
