Abstract

We argue that TeVeS-like vector fields appear naturally in certain string theory backgrounds involving D0-branes, as a result of the recoil velocity field, expressing the interaction of neutrino string matter with point-like branes. However, the similarity with TeVeS models is restricted only to the bi-metric properties of space–time, namely the difference of the background metric from the one felt by (some) matter fields interacting, in a topologically non-trivial manner, with the D0-brane defects. In our approach, neutrinos appear as dark matter candidates that could be “captured” by the D0-branes, as a result of stringy properties, and thus couple with the recoil-vector fields. Moreover, we argue in support of a possibly preferential rôle of neutrinos in inducing novel non-perturbative contributions to “vacuum” (dark) energy, in addition to their ordinary dark matter contribution. In fact, the rôle of neutrinos as providing substantial contributions to dark matter and dark energy components of the Universe, suggested by our approach, appears also to be necessitated by the need to reproduce the peaks in the Cosmic Microwave Background radiation spectrum, as claimed recently in the literature. Thus, our framework may be viewed as providing a microscopic explanation of such phenomenological conclusions concerning TeVeS-like, Lorentz-violating models.

Highlights

  • We argue that TeVeS-like vector fields appear naturally in certain string theory backgrounds involving D0-branes, as a result of the recoil velocity field, expressing the interaction of neutrino string matter with point-like branes

  • The above studies are not model independent, as they are based on conventional Einstein/Friedmann-LemaıtreRobertson-Walker (FLRW) cosmologies

  • In nonequilibrium string theory models [2], it is possible to fit the data with the conventional ΛCDM model [3]

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Summary

Introduction

We argue that TeVeS-like vector fields appear naturally in certain string theory backgrounds involving D0-branes, as a result of the recoil velocity field, expressing the interaction of neutrino string matter with point-like branes. World-sheet conformal invariance requires that a target-space metric deformation corresponds to a conformal-dimension-two operator of the σ-model. In the linear-dilaton scenario we employed above, this condition translates to the following metric, which describes the effects of the interaction of the stringy matter excitation with the D-particle defect on the surrounding space-time: gμmνatter = ημν + eΦ − e−Φ uμuν , Φ = −uμX μ .

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