12,318 research outputs found
TeV resonances in top physics at the LHC
We consider the possibility of studying novel particles at the TeV scale with
enhanced couplings to the top quark via top quark pair production at the LHC
and VLHC. In particular we discuss the case of neutral scalar and vector
resonances associated with a strongly interacting electroweak symmetry breaking
sector. We constrain the couplings of these resonances by imposing appropriate
partial wave unitarity conditions and known low energy constraints. We evaluate
the new physics signals via WW -> tt~ for various models without making
approximation for the initial state W bosons, and optimize the acceptance cuts
for the signal observation. We conclude that QCD backgrounds overwhelm the
signals in both the LHC and a 200 TeV VLHC, making it impossible to study this
type of physics in the tt~ channel at those machines.Comment: 15p, add. comments to clarify model, +2 ref., version to appear PR
Inevitability of Plate Tectonics on Super-Earths
The recent discovery of super-Earths (masses less or equal to 10
earth-masses) has initiated a discussion about conditions for habitable worlds.
Among these is the mode of convection, which influences a planet's thermal
evolution and surface conditions. On Earth, plate tectonics has been proposed
as a necessary condition for life. Here we show, that super-Earths will also
have plate tectonics. We demonstrate that as planetary mass increases, the
shear stress available to overcome resistance to plate motion increases while
the plate thickness decreases, thereby enhancing plate weakness. These effects
contribute favorably to the subduction of the lithosphere, an essential
component of plate tectonics. Moreover, uncertainties in achieving plate
tectonics in the one earth-mass regime disappear as mass increases:
super-Earths, even if dry, will exhibit plate tectonic behaviour.Comment: 13 pages, 2 figures and 1 table; in press in ApJ
An analysis of the Sargasso Sea resource and the consequences for database composition
Background: The environmental sequencing of the Sargasso Sea has introduced a huge new resource of genomic information. Unlike the protein sequences held in the current searchable databases, the Sargasso Sea sequences originate from a single marine environment and have been sequenced from species that are not easily obtainable by laboratory cultivation. The resource also contains very many fragments of whole protein sequences, a side effect of the shotgun sequencing method.These sequences form a significant addendum to the current searchable databases but also present us with some intrinsic difficulties. While it is important to know whether it is possible to assign function to these sequences with the current methods and whether they will increase our capacity to explore sequence space, it is also interesting to know how current bioinformatics techniques will deal with the new sequences in the resource.Results: The Sargasso Sea sequences seem to introduce a bias that decreases the potential of current methods to propose structure and function for new proteins. In particular the high proportion of sequence fragments in the resource seems to result in poor quality multiple alignments.Conclusion: These observations suggest that the new sequences should be used with care, especially if the information is to be used in large scale analyses. On a positive note, the results may just spark improvements in computational and experimental methods to take into account the fragments generated by environmental sequencing techniques
T-odd correlations from CP violating anomalous top-quark couplings revisited
We revisit the effect of CP violating anomalous top-quark couplings in
production and decay. We consider production through
gluon fusion (and light annihilation) followed by top-quark decay
into or . We find explicit analytic expressions for all the
triple products generated by the anomalous couplings that fully incorporate all
spin correlations. Our results serve as a starting point for numerical
simulations for the LHC.Comment: minor typos correcte
The Interior Dynamics of Water Planets
The ever-expanding catalog of detected super-Earths calls for theoretical
studies of their properties in the case of a substantial water layer. This work
considers such water planets with a range of masses and water mass fractions (2
to 5 M_Earth, 0.02% to 50% H2 O). First, we model the thermal and dynamical
structure of the near-surface for icy and oceanic surfaces, finding separate
regimes where the planet is expected to maintain a subsurface liquid ocean and
where it is expected to exhibit ice tectonics. Newly discovered exoplanets may
be placed into one of these regimes given estimates of surface temperature,
heat flux, and gravity. Second, we construct a parameterized convection model
for the underlying ice mantle of higher ice phases, finding that materials
released from the silicate iron core should traverse the ice mantle on the
timescale of 0.1 to 100 megayears. We present the dependence of the overturn
times of the ice mantle and the planetary radius on total mass and water mass
fraction. Finally, we discuss the implications of these internal processes on
atmospheric observables.Comment: 9 page 4 figure
On the Expressiveness of Spatial Constraint Systems
In this paper we shall report on our progress using spatial constraint system as an abstract representation of modal and epistemic behaviour. First we shall give an introduction as well as the background to our work. Then, we present our preliminary results on the representation of modal behaviour by using spatial constraint systems. Then, we present our ongoing work on the characterization of the epistemic notion of knowledge. Finally, we discuss about the future work of our research
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