A posteriori inclusion of parton density functions in NLO QCD final-state calculations at hadron colliders: The APPLGRID Project

Sissa Medialab Srl (2010) 051

A Unified Theory of Matter Genesis: Asymmetric Freeze-In

ArXiv 1010.0245 (2010)

Authors:

Lawrence J Hall, John March-Russell, Stephen M West

Abstract:

We propose a unified theory of dark matter (DM) genesis and baryogenesis. It explains the observed link between the DM density and the baryon density, and is fully testable by a combination of collider experiments and precision tests. Our theory utilises the "thermal freeze-in" mechanism of DM production, generating particle anti-particle asymmetries in decays from visible to hidden sectors. Calculable, linked, asymmetries in baryon number and DM number are produced by the feeble interaction mediating between the two sectors, while the out-of-equilibrium condition necessary for baryogenesis is provided by the different temperatures of the visible and hidden sectors. An illustrative model is presented where the visible sector is the MSSM, with the relevant CP violation arising from phases in the gaugino and Higgsino masses, and both asymmetries are generated at temperatures of order 100 GeV. Experimental signals of this mechanism can be spectacular, including: long-lived metastable states late decaying at the LHC; apparent baryon-number or lepton-number violating signatures associated with these highly displaced vertices; EDM signals correlated with the observed decay lifetimes and within reach of planned experiments; and a prediction for the mass of the dark matter particle that is sensitive to the spectrum of the visible sector and the nature of the electroweak phase transition.

A Unified Theory of Matter Genesis: Asymmetric Freeze-In

(2010)

Authors:

Lawrence J Hall, John March-Russell, Stephen M West

Stabilizing the Complex Structure in Heterotic Calabi-Yau Vacua

(2010)

Authors:

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

Systematic effects in the extraction of the WMAP haze

Journal of Cosmology and Astroparticle Physics 2010:10 (2010)

Authors:

P Mertsch, S Sarkar

Abstract:

The extraction of a 'haze' from the WMAP microwave skymaps is based on subtraction of known foregrounds, viz. free-free (bremsstrahlung), thermal dust and synchrotron, each traced by other skymaps. While the 408 MHz all-sky survey is used for the synchrotron template, the WMAP bands are at tens of GHz where the spatial distribution of the radiating cosmic ray electrons ought to be quite different because of the energy-dependence of their diffusion in the Galaxy. The systematic uncertainty this introduces in the residual skyrnap is comparable to the claimed haze and can, for certain source distributions, have a very similar spectrum and latitudinal profile and even a somewhat similar morphology. Hence caution must be exercised in interpreting the haze as a physical signature of, e.g., dark matter annihilation in the Galactic centre. © 2010 IOP Publishing Ltd and SISSA.