263,413 research outputs found
BIOMECHANICS OF LONGSWINGS PRECEDING TKACHEV ON UNEVEN BARS
No full textChanges in the rules governing the separation of uneven bars have allowed female gymnasts to perform the Tkachev in both directions. The aim of this study was to compare the similarities in the preparatory longswing during the outward (O) and inward (I) Tkachevs. Video recordings of the Tkachevs (O=5, I=5) were collected from the 2000 Sydney Olympic Games. A 37° greater range of movement was found at the hips during the I Tkachev. In the more conventional O technique changes in the hip angle were smaller (23°) and occurred over a greater circle angle. This study has identified differences in what appear to be very similar skills. Further inter-segmental coordination and joint kinetic analyses may provide insight into the performance of these release and regrasp skills
BBN with light dark matter
No full textEffects of light millicharged dark matter particles on primordial nucleosynthesis are considered. It is shown that if the mass of such particles is much smaller than the electron mass, they lead to strong overproduction of Helium-4. An agreement with observations can be achieved by non-vanishing lepton asymmetry. Baryon-to-photon ratio at BBN and neutrino-to-photon ratio both at BBN and at recombination are noticeably different as compared to the standard cosmological model. The latter ratio and possible lepton asymmetry could be checked by Planck. For higher mass of new particles the effect is much less pronounced and may even have opposite sign
Dark matter and generation of galactic magnetic fields
No full textA new scenario for creation of galactic magnetic fields is proposed which is operative at the cosmological epoch of the galaxy formation, and which relies on unconventional properties of dark matter. Namely, it requires existence of feeble but long range interaction between the dark matter particles and electrons. In particular, millicharged dark matter particles or mirror particles with the photon kinetic mixing to the usual photon can be considered. We show that in rotating protogalaxies circular electric currents can be generated by the interactions of free electrons with dark matter particles in the halo, while the impact of such interactions on galactic protons is considerably weaker. The induced currents may be strong enough to create the observed magnetic fields on the galaxy scales with the help of moderate dynamo amplification. In addition, the angular momentum transfer from the rotating gas to dark matter component could change the dark matter profile and formation of cusps at galactic centers would be inhibited. The global motion of the ionized gas could produce sufficiently large magnetic fields also in filaments and galaxy clusters
Reconciling Planck results with low redshift astronomical measurements
No full textWe show that emerging tension between the direct astronomical measurements at low redshifts and cosmological parameters deduced from the Planck measurements of the cosmic microwave background anisotropies can be alleviated if the dark matter consists of two fractions, the stable part being dominant with a smaller unstable fraction. The latter constitutes about 5-10 per cent at the recombination epoch if it has decayed by now
Deposition of Coke in Pyrolysis of Vacuum Gasoil after Hydrocracking
No full textLyakhnovich, I.Z., Tkachev, S.M. Deposition of Coke in Pyrolysis of Vacuum Gasoil after Hydrocracking. Chemistry and Technology of Fuels and Oils 38, 233–236 (2002). https://doi.org/10.1023/A:102027771725
Justification of the Courant–Friedrich's hypothesis in the case of a weak shock. Part I. Presentation of solution to linear problem
No full textAbstractAs is well known, two solutions of the problem of a supersonic stationary inviscid nonheatconducting gas flow onto a planar infinite wedge are theoretically possible: the solution with a strong shock (the flow speed behind the shock is subsonic) and the solution with a weak shock (the flow speed behind the shock is supersonic). Unlike the well-studied case of a strong shock that is generically unstable [A.M. Blokhin, D.L. Tkachev, L.O. Baldan, Study of the stability in the problem on flowing around a wedge. The case of strong wave, J. Math. Anal. Appl. 319 (2006) 248–277; A.M. Blokhin, D.L. Tkachev, Yu.Yu. Pashinin, Stability condition for strong shock waves in the problem of flow around an infinite plane wedge, Nonlinear Anal. Hybrid Syst. 2 (2008) 1–17], R. Courant and K.O. Friedrichs [R. Courant, K.O. Friedrichs, Supersonic Flow and Shock Waves, Interscience Publishers, New York, 1948] assumed that the solution with a weak shock is asymptotically stable by Lyapunov. Presentation of classical solution to the corresponding problem which is found in the present paper is the first step on the way to justification of Courant–Friedrichs hypothesis on linear level
MUSCULOSKELETAL WORK PRECEDING THE TKACHEV ON UNEVEN BARS
No full textThe purpose of this study was to identify the mechanics of traditional outward facing (O) and newer inward facing (I) Tkachev on uneven bars. Images of ten straddle Tkachevs (O=5, I=5) performed at the Sydney Olympic Games, 2000 were recorded with twin video cameras (50Hz). Manual digitising and 3D DLT reconstruction techniques were combined with inertia modelling to develop customised profiles for the ten gymnasts. Inverse dynamics analyses were used to quantify hip and shoulder joint kinetics, and segmental and bar energy exchanges from the horizontal position on the downswing to bar release. There was evidence that more energy was stored in and recovered from the bar in the inward technique. The role of the hips remained similar for both skills, but a large shoulder flexion rather than extension occurred in the inward technique close to release
Going Beyond Counting First Authors in Author Co-citation Analysis
No full textThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
Bisimilar stochastic systems
No full textStochastic systems have been widely investigated and employed in numerousapplications in different areas such as finance, biology and engineering asthey allow accounting for imprecisions so often faced in every practical tasks. Often that task would require to find the best action sequence in order to optimize the outcome. When the model is small, one can efficiently employ algorithmic techniques to synthesize such a control policy. Hence, in case of more complex models, instead of solving control tasks there directly, one may want to approximate them with simpler ones and then use those algorithms. This method is called abstraction for it abstracts the original “physical” model to an “abstract” one, only needed to ease the computations. Ideally, this abstract model is somewhat similar to the original one, as we want to extrapolate results achieved over the former to the setting of the latter. One way this similarity can be ensured is by means of the (bi)simulation methods, that give sufficient conditions to the closeness of behaviors of the two systems being compared. Such techniques became popular in discrete non-stochastic models, then advanced to continuous ones and started making steps to discrete stochastic systems. Yet, definite results were not achieved for abstractions of continuous stochastic models. There were trials to extend ideas from continuous non-stochastic framework, or discrete stochastic one, but they were mostly fragmentary. This thesis brings those methods together to build a unified framework and shows immediate benefits of doing this.To define the closeness between the systems we look at their path-wise properties, which cover most of the tasks whose relevance was praised in the literature. That comprises both additive cost-like criteria and formal specifications, e.g. encoded by LTL formulae of the kind “reach the goal set through the safe set while avoiding dangerous states”. We derive guarantees on the approximation error and suggest how to build an abstraction for a given tolerance level. These guarantees work mostly for the finite time horizon properties, hence for the rest we develop task-dependent solution methods, further connecting with the existing literature. Besides those concrete results, we also put some effort in developing the conceptual side of the bisimulation framework for stochastic systems. For example, we know how important it is to choose a definition of behavior here, since bisimiliarity is useful as long as it guarantees closeness of behaviors one is interested in.We hence stress the importance of keeping in mind the final goal while extrapolating abstract solution methods, and show which issues may arise when this goal is forgotten. We also extend the framework we deal with beyond bisimulation of stochastic systems only, providing a formalization of approximate relations and their connections with pseudo-metrics, proving several theorems in probabilistic approximation, whose generality is greater than the scope of this thesis, and also provide a category-theoretical basis for bisimulations of stochastic systems, hence opening one more door from which this problem can be approached.Team Bart De Schutte
Production of Massive Fermions at Preheating and Leptogenesis
No full textWe present a complete computation of the inflaton decay into very massive fermions during preheating. We show that heavy fermions are produced very efficiently up to masses of order 10^{17}-10^{18} GeV; the accessible mass range is thus even broader than the one for heavy bosons. We apply our findings to the leptogenesis scenario, proposing a new version of it, in which the massive right-handed neutrinos, responsible for the generation of the baryon asymmetry, are produced during preheating. We also discuss other production mechanisms of right-handed neutrinos in the early Universe, identifying the neutrino mass parameters for which the observed baryon asymmetry is reproduced
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