3,527 research outputs found
Is there Correlation between Fine Structure and Dark Energy Cosmic Dipoles?
We present a detailed analysis (including redshift tomography) of the cosmic
dipoles in the Keck+VLT quasar absorber and in the Union2 SnIa samples. We show
that the fine structure constant cosmic dipole obtained through the Keck+VLT
quasar absorber sample at level is anomalously aligned with the
corresponding dark energy dipole obtained through the Union2 sample at
level. The angular separation between the two dipole directions is
. We use Monte Carlo simulations to find the
probability of obtaining the observed dipole magnitudes with the observed
alignment, in the context of an isotropic cosmological model with no
correlation between dark energy and fine structure constant . We find
that this probability is less than one part in . We propose a simple
physical model (extended topological quintessence) which naturally predicts a
spherical inhomogeneous distribution for both dark energy density and fine
structure constant values. The model is based on the existence of a recently
formed giant global monopole with Hubble scale core which also couples
non-minimally to electromagnetism. Aligned dipole anisotropies would naturally
emerge for an off-centre observer for both the fine structure constant and for
dark energy density. This model smoothly reduces to \lcdm for proper limits of
its parameters. Two predictions of this model are (a) a correlation between the
existence of strong cosmic electromagnetic fields and the value of and
(b) the existence of a dark flow on Hubble scales due to the repulsive gravity
of the global defect core (`Great Repulser') aligned with the dark energy and
dipoles. The direction of the dark flow is predicted to be towards the
spatial region of lower accelerating expansion. Existing data about the dark
flow are consistent with this prediction.Comment: 14 pages 11 figures (two column revtex). Aceepted in Phys. Rev. D (to
appear). Significant extensions (mostly on section 4 on the theoretical
model), added references, corrected typos. The data, updated mathematica and
C program files used for the numerical analysis may be downloaded from
http://leandros.physics.uoi.gr/defsdipole
Electroweak and supersymmetry breaking from the Higgs discovery
We will explore the consequences on the electroweak breaking condition, the
mass of supersymmetric partners and the scale at which supersymmetry is broken,
for arbitrary values of the supersymmetric parameters tan(beta) and the stop
mixing X_t, which follow from the Higgs discovery with a mass m_H\simeq 126 GeV
at the LHC. Within the present uncertainty on the top quark mass we deduce that
radiative breaking requires tan(beta) \gtrsim 7 for maximal mixing X_t\simeq
\sqrt{6}, and tan(beta) \gtrsim 20 for small mixing X_t\lesssim 1. The scale at
which supersymmetry is broken \mathcal M can be of order the unification or
Planck scale only for large values of tan(beta) and negligible mixing X_t\simeq
0. On the other hand for maximal mixing and large values of tan(beta)
supersymmetry should break at scales as low as \mathcal M\simeq 10^5 GeV. The
uncertainty in those predictions stemming from the uncertainty in the top quark
mass, i.e. the top Yukawa coupling, is small (large) for large (small) values
of tan(beta). In fact for tan(beta)=1 the uncertainty on the value of \mathcal
M is of several orders of magnitude.Comment: 16 pages, 7 figures; v2: numerical typo corrected in codes, and 2
loop radiative corrections added. Some conclusions slightly change
General Focus Point in the MSSM
The minimal supersymmetric extension of the Standard Model (SM) is a well
motivated scenario for physics beyond the SM, which allows a perturbative
description of the theory up to scales of the order of the Grand Unification
scale, where gauge couplings unify. The Higgs mass parameter is insensitive to
the ultraviolet physics and is only sensitive to the scale of soft
supersymmetry breaking parameters. Present collider bounds suggest that the
characteristic values of these parameters may be significantly larger than the
weak scale. Large values of the soft breaking parameters, however, induce large
radiative corrections to the Higgs mass parameter and therefore the proper
electroweak scale may only be obtained by a fine tuned cancellation between the
square of the holomorphic \mu-parameter and the Higgs supersymmetry breaking
square mass parameter. This can only be avoided if there is a correlation
between the scalar and gaugino mass parameters, such that the Higgs
supersymmetry breaking parameter remains of the order of the weak scale. The
scale at which this happens is dubbed as focus point. In this article, we
define the general conditions required for this to happen, for different values
of the messenger scale at which supersymmetry breaking is transmitted to the
observable sector, and for arbitrary boundary conditions of the sfermion,
gaugino, and Higgs mass parameters. Specific supersymmetry breaking scenarios
in which these correlations may occur are also discussed.Comment: 19 pages, 9 figures, new refs. adde
Gauged Axions and their QCD Interactions
We present a brief overview of axion models associated to anomalous abelian
(gauge) symmetries, discussing their main phenomenological features. Among
these, the mechanism of vacuum misalignment introduced at the QCD and at the
electroweak phase transitions, with the appearance of periodic potentials,
responsible for the generation of a mass for these types of axions.Comment: 8 pages, 6 figures. Presented at QCD@Work - International Workshop on
QCD - Theory and Experiment 20-23 June 2010 Martina Franca - Valle d'Itria -
Italy, to appear in the AIP Conference Proceedings Series 201
Relic Densities of Dark Matter in the U(1)-Extended NMSSM and the Gauged Axion Supermultiplet
We compute the dark matter relic densities of neutralinos and axions in a
supersymmetric model with a gauged anomalous U(1) symmetry, kinetically mixed
with of hypercharge. The model is a variant of the USSM (the U(1)
extended NMSSM), containing an extra U(1) symmetry and an extra singlet in the
superpotential respect to the MSSM, where gauge invariance is restored by
Peccei-Quinn interactions using a Stuckelberg multiplet. This approach
introduces an axion (Im b) and a saxion (Re b) in the spectrum and generates an
axino component for the neutralino. The Stuckelberg axion (Im b) develops a
physical component (the gauged axion) after electroweak symmetry breaking. We
classify all the interactions of the Lagrangian and perform a complete
simulation study of the spectrum, determining the neutralino relic densities
using micrOMEGAs. We discuss the phenomenological implications of the model
analyzing mass values for the axion from the milli-eV to the MeV region. The
possible scenarios that we analyze are significantly constrained by a
combination of WMAP data, the exclusion limits from direct axion searches and
the veto on late entropy release at the time of nucleosynthesis.Comment: 43 pages, 11 figures. Revised final version, accepted for publication
in Phys. Rev.
GMSB with Light Stops
Gauge mediated supersymmetry breaking (GMSB) is an elegant mechanism to
transmit supersymmetry breaking from the hidden to the MSSM observable sector,
which solves the supersymmetric flavor problem. However the smallness of the
generated stop mixing requires superheavy stops to reproduce the experimental
value of the Higgs mass. Two possible ways out are: i) To extend GMSB by direct
superpotential messenger-MSSM Yukawa couplings to generate sizeable mixing,
thus reintroducing the flavor problem; ii) To extend the MSSM Higgs sector with
singlets and/or triplets providing extra tree-level corrections to the Higgs
mass. Singlets will not get any soft mass from GMSB and triplets will
contribute to the parameter which could be an issue. In this paper we
explore the second way by introducing extra supersymmetric triplets with
hypercharges , with a tree-level custodial global symmetry in the Higgs sector protecting the parameter: a
supersymmetric generalization of the Georgi-Machacek model, dubbed as
supersymmetric custodial triplet model (SCTM). The renormalization group
running from the messenger to the electroweak scale mildly breaks the custodial
symmetry. We will present realistic low-scale scenarios (with the NLSP being a
Bino-like neutralino or the right-handed stau) based on general (non-minimal)
gauge mediation and consistent with all present experimental data. Their main
features are: i) Light ( TeV) stops; ii) Exotic couplings ( and ) absent in the MSSM and proportional to the
triplets VEV, ; and, iii) A possible (measurable) universality
breaking of the Higgs couplings .Comment: 21 pages, 9 figures; v2: references adde
Radiation Damping in a Non-Abelian Strongly-Coupled Gauge Theory
We study a `dressed' or `composite' quark in strongly-coupled N=4
super-Yang-Mills (SYM), making use of the AdS/CFT correspondence. We show that
the standard string dynamics nicely captures the physics of the quark and its
surrounding quantum non-Abelian field configuration, making it possible to
derive a relativistic equation of motion that incorporates the effects of
radiation damping. From this equation one can deduce a non-standard dispersion
relation for the composite quark, as well as a Lorentz covariant formula for
its rate of radiation.Comment: 10 pages; based on talks at Quantum Theory and Symmetries 6 and the
XII Mexican Workshop of Particles and Fields
The Plasmid Mobilome of the Model Plant-Symbiont Sinorhizobium meliloti: Coming up with New Questions and Answers
Rhizobia are Gram-negative Alpha- andBetaproteobacteria living in the underground that have theability to associate with legumes for the establishment ofnitrogen-fixing symbioses.Sinorhizobium melilotiinparticularâthe symbiont ofMedicago,Melilotus, andTrigonellaspp.âhas for the past decades served as a model organism forinvestigating, at the molecular level, the biology, biochemistry,and genetics of a free-living and symbiotic soil bacterium ofagricultural relevance. To date, the genomes of seven differentS. melilotistrains have been fully sequenced and annotated,and several other draft genomic sequences are also available(http://www.ncbi.nlm.nih.gov/genome/genomes/1004).The vast amount of plasmid DNA thatS. melilotifrequently bears(up to 45% of its total genome), the conjugative ability of some ofthose plasmids, and the extent of the plasmid diversity hasprovided researchers with an extraordinary system to investigatefunctional and structural plasmid molecular biology within theevolutionary context surrounding a plant-associated modelbacterium. Current evidence indicates that the plasmidmobilome inS. melilotiis composed of replicons varying greatlyin size and having diverse conjugative systems and propertiesalong with different evolutionary stabilities and biological roles.While plasmids carrying symbiotic functions (pSyms) are knownto have high structural stability (approaching that ofchromosomes), the remaining plasmid mobilome (referred to asthe non-pSym,functionally cryptic,oraccessorycompartment)has been shown to possess remarkable diversity and to be highlyactive in conjugation. In light of the modern genomic andcurrent biochemical data on the plasmids ofS. meliloti,the current article revises their main structural components,their transfer and regulatory mechanisms, and their potentialas vehicles in shaping the evolution of the rhizobial genome.Fil: Lagares, Antonio. Consejo Nacional de Investigaciones CientĂficas y TĂ©cnicas. Centro CientĂfico TecnolĂłgico Conicet - La Plata. Instituto de BiotecnologĂa y BiologĂa Molecular. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de BiotecnologĂa y BiologĂa Molecular; ArgentinaFil: SanjuĂĄn Pinilla, Juan. Consejo Superior de Investigaciones CientĂficas. EstaciĂłn Experimental del ZaidĂn; EspañaFil: Pistorio, Mariano. Consejo Nacional de Investigaciones CientĂficas y TĂ©cnicas. Centro CientĂfico TecnolĂłgico Conicet - La Plata. Instituto de BiotecnologĂa y BiologĂa Molecular. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de BiotecnologĂa y BiologĂa Molecular; Argentin
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