The cosmological constant problem in heterotic-M-theory and the orbifold of time
Andrea Zanzi

TL;DR
This paper explores a string-theoretic approach to the cosmological constant problem using heterotic-M-theory, with a focus on quantum gravity, orbifold time compactification, and the equivalence of gravity and gauge theories.
Contribution
It links the Modified Fujii's Model to heterotic-M-theory, providing a quantum gravity framework with a stringy origin and analyzing the implications of orbifold time compactification.
Findings
Quantum gravity and gauge theory are equivalent in this framework.
The stringy origin of the model offers a finite, quantum description of gravity.
Orbifold time compactification affects the stability of the dilaton potential.
Abstract
Chameleon fields are quantum fields with an increasing mass as a function of the matter density of the environment. Recently chameleon fields have been exploited to solve the cosmological constant problem in the Modified Fujii's Model - MFM [Phys Rev D82 (2010) 044006]. However, gravity has been treated basically at a semiclassical level in that paper. In this article the stringy origin of the MFM is further discussed: as we will see, the MFM can be obtained from heterotic-M-theory. Consequently, a quantum description of gravity is obtained and the theory is finite because we choose the string mass as our UV cut-off. This stringy origin of the MFM creates stronger theoretical grounds for our solution to the cosmological constant problem. In our analysis, time will be compactified on a orbifold and this peculiar compactification of time has a number of consequences. For…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
