Stabilizing All Geometric Moduli in Heterotic Calabi-Yau Vacua

(2011)

Authors:

Lara B Anderson, James Gray, Andre Lukas, Burt Ovrut

Continuum Random Combs and Scale Dependent Spectral Dimension

ArXiv 1101.4174 (2011)

Authors:

Max R Atkin, Georgios Giasemidis, John F Wheater

Abstract:

Numerical computations have suggested that in causal dynamical triangulation models of quantum gravity the effective dimension of spacetime in the UV is lower than in the IR. In this paper we develop a simple model based on previous work on random combs, which share some of the properties of CDT, in which this effect can be shown to occur analytically. We construct a definition for short and long distance spectral dimensions and show that the random comb models exhibit scale dependent spectral dimension defined in this way. We also observe that a hierarchy of apparent spectral dimensions may be obtained in the cross-over region between UV and IR regimes for suitable choices of the continuum variables. Our main result is valid for a wide class of tooth length distributions thereby extending previous work on random combs by Durhuus et al.

Continuum Random Combs and Scale Dependent Spectral Dimension

(2011)

Authors:

Max R Atkin, Georgios Giasemidis, John F Wheater

Finite fermion mass effects in pseudoscalar Higgs production via gluon-gluon fusion

(2011)

Authors:

Fabrizio Caola, Simone Marzani

Mixed dark matter from technicolor

Physical Review D Particles Fields Gravitation and Cosmology 83:1 (2011)

Authors:

A Belyaev, MT Frandsen, S Sarkar, F Sannino

Abstract:

We study natural composite cold dark matter candidates which are pseudo-Nambu-Goldstone bosons (pNGB) in models of dynamical electroweak symmetry breaking. Some of these can have a significant thermal relic abundance, while others must be mainly asymmetric dark matter. By considering the thermal abundance alone we find a lower bound of mW on the pNGB mass when the (composite) Higgs is heavier than 115 GeV. Being pNGBs, the dark matter candidates are in general light enough to be produced at the LHC. © 2011 American Physical Society.