8,157 research outputs found

    Large Gravitational Wave Background Signals in Electroweak Baryogenesis Scenarios

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    The bubble wall velocity in an electroweak first order phase transition is a key quantity both for electroweak baryogenesis and for the production of a stochastic background of gravitational waves that may be probed in the future through gravitational wave experiments like LISA or BBO. We show that, contrary to the conclusion drawn from previous studies, it is actually possible to generate a potentially large gravitational wave signal while satisfying the requirements for viable electroweak baryogenesis, once the effects of the hydrodynamics of bubble growth are taken into account. Then, the observation of a large gravitational wave background from the electroweak phase transition would not necessarily rule out electroweak baryogenesis as the mechanism having generated the observed baryon asymmetry of the universe.Comment: 6 pages. References added. Accepted for publication in Phys. Rev.

    Some Cosmological Implications of Hidden Sectors

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    We discuss some cosmological implications of extensions of the Standard Model with hidden sector scalars coupled to the Higgs boson. We put special emphasis on the conformal case, in which the electroweak symmetry is broken radiatively with a Higgs mass above the experimental limit. Our refined analysis of the electroweak phase transition in this kind of models strengthens the prediction of a strongly first-order phase transition as required by electroweak baryogenesis. We further study gravitational wave production and the possibility of low-scale inflation as well as a viable dark matter candidate.Comment: 23 pages, 8 figures; some comments added, published versio

    Transition from Mott insulator to superconductor in GaNb4_{4}Se8_{8} and GaTa4_{4}Se8_{8} under high pressure

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    Electronic conduction in GaM4_{4}Se8_{8} (M=Nb;Ta) compounds with the fcc GaMo4_{4}S8_{8}-type structure originates from hopping of localized unpaired electrons (S=1/2) among widely separated tetrahedral M4_{4} metal clusters. We show that under pressure these systems transform from Mott insulators to a metallic and superconducting state with TC_{C}=2.9 and 5.8K at 13 and 11.5GPa for GaNb4_{4}Se8_{8} and GaTa4_{4}Se8_{8}, respectively. The occurrence of superconductivity is shown to be connected with a pressure-induced decrease of the MSe6_{6} octahedral distortion and simultaneous softening of the phonon associated with MSe-bonds.Comment: 10 pages, 5 figure

    Flight Tests, Performances and Flight Certification of a Twin-Engine Light Aircraft

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    This paper deals with flight test activities performed on P2006T, a twin-engine light aircraft recently designed and produced by Tecnam. Research activities and flight tests have been conducted during the flight certification of P2006T for the normal category under CS-23. All the acquired data and flight results presented have been focused on both aircraft certification and on aircraft performances, stability and flight qualities measurement. The data have been acquired through a light, accurate and reliable flight instrumentation available at DIAS (Department of Aerospace Engineering). Some flight data about aircraft leveled speed, stall speed, climb characteristics and ground performances (take-off and landing) will be presented. After preliminary flight tests, winglets have been designed and added to the final configuration in order to obtain good climb performances also in OEI (One Engine Inoperative) conditions. Accurate stall tests have been performed in all configurations and influence of both entry-rate and load factor on stall speed have been highlighted. Excellent ground performances have been measured with short take-off and landing distances compared with similar airplanes. All measured flight performances can be considered very good for this aircraft category and have been used to demonstrate aircraft safety and to obtain CS23 certification

    Virtual liver biopsy: image processing and 3D visualization

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    Effect of temperature and illumination on the electrical characteristics of polymer-fullerene bulk-heterojunction solar cells

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    The current-voltage characteristics of ITO/PEDOT:PSS/OC1C10-PPV:PCBM/Al solar cells were measured in the temperature range 125-320 K under variable illumination, between 0.03 and 100 mW cm(-2) (white light), with the aim of determining the efficiency-limiting mechanism(s) in these devices, and the temperature and/or illumination range(s) in which these devices demonstrate optimal performance. (ITO: indium tin oxide; PEDOT:PSS: poly(styrene sulfonate)-doped poly(ethylene dioxythiophene); OC1C10-PPV: poly[2-methoxy-5-(3,7-dimethyl octyloxy)-1,4-phenylene vinylene]; PCBM: phenyl-C-61 butyric acid methyl ester.) The short-circuit current density and the fill factor grow monotonically with temperature until 320 K. This is indicative of a thermally activated transport of photogenerated charge carriers, influenced by recombination with shallow traps. A gradual increase of the open-circuit voltage to 0.91 V was observed upon cooling the devices down to 125 K. This fits the picture in which the open-circuit voltage is not limited by the work-function difference of electrode materials used. The overall effect of temperature on solar-cell parameters results in a positive temperature coefficient of the power conversion efficiency, which is 1.9% at T = 320 K and 100 mW cm(-2) (2.5% at 0.7 mW cm(-2)). The almost-linear variation of the short-circuit current density with light intensity confirms that the internal recombination losses are predominantly of monomolecular type under short-circuit conditions. We present evidence that the efficiency of this type of solar cell is limited by a light-dependent shunt resistance. Furthermore, the electronic transport properties of the absorber materials, e.g., low effective charge-carrier mobility with a strong temperature dependence, limit the photogenerated current due to a high series resistance, therefore the active layer thickness must be kept low, which results in low absorption for this particular composite absorber

    Effect of fluoridated toothpicks and dental flosses on enamel and dentine and on plaque composition in situ

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    The aim was to evaluate the effect of two toothpicks and two dental flosses on demineralized enamel and dentine and on plaque composition, using an in situ model with simulated approximal spaces within dentures. Fifteen subjects with full dentures were recruited and 14 completed the study. It consisted of two crossover periods, the first comparing a birch toothpick with AmF and a birch toothpick with NaF, and the second comparing a dental floss with AmF + NaF and a dental floss without F. Between these four periods, there was a control period without any approximal cleaning. In small, rectangular sample holders, one enamel and one dentine specimen were embedded, forming a triangular, approximal-like space. Two sample holders were mounted in the premolar-molar region of the upper or lower dentures. The subjects used the toothpicks or dental flosses 3 times/day for 4 weeks. The results showed that all toothpicks and dental flosses inhibited further demineralization compared to the control period ( p <0.001). The dental flosses were somewhat more effective in this respect than the toothpicks, especially in dentine. There were relatively small numerical differences between AmF and NaF toothpicks, but in favour of NaF regarding mineral gain ( p <0.05). The fluoridated floss gave somewhat less lesion depth in dentine than the non-fluoridated floss ( p <0.01). Toothpicks and flosses resulted in lower counts of microorganisms in plaque compared to the control period ( p <0.001); the AmF toothpick gave a more pronounced reduction than the NaF toothpick ( p <0.001). Copyright (C) 2005 S. Karger AG, Basel

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    The Effect of Maja Fruit [Aegle Marmelos (L) Correa] on Inflammation Markers Involved in the Aging Process

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    Background: Aging is a process that every living creature will pass through and involves various factors. Increased inflammatory factors can be caused by hypoxia which forms Reactive Oxygen Species (ROS) and damages macromolecules and causes the acceleration of the aging process. Maja plants, empirically have long been used as medicinal plants, research on Maja leaves shows anti-inflammatory and antioxidant potential.Objective: The purpose of this study was to find out and understand the potential of Maja fruit in the presence of inflammatory markers of IL-6 and TNF-α which are involved in the aging process.Methods: This research was in vivo experimental, using male experimental animals Sprague Dawley rats divided into 8 groups (n = 4), and divided into 2 groups (fed with Maja ethanol extract (400 mg/ kg/day, 14 days) and not force-fed). Each group was divided into 4 subgroups (normoxia, hypoxia (O2 8%, N2 92%) for 3, 7 and 14 days). At the end of the trial period, animal blood was examined for IL-6 and TNF-α concentrations using the ELISA method.Results: The results showed an increase in levels of IL-6 and TNF-α both in the group fed and not fed in line with the duration of hypoxia when compared with controls. However, groups that are not force-fed show a higher pattern compared to those who are force-fed.Conclusion : The ethanol extract of Maja fruit can help slow down the aging process

    Non-adiabatic radiative collapse of a relativistic star under different initial conditions

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    We examine the role of space-time geometry in the non-adiabatic collapse of a star dissipating energy in the form of radial heat flow, studying its evolution under different initial conditions. The collapse of a star with interior comprising of a homogeneous perfect fluid is compared with that of a star filled with inhomogeneous imperfect fluid with anisotropic pressure. Both the configurations are spherically symmetric, however, in the latter case, the physical space t=constantt= constant of the configurations is assumed to be inhomogeneous endowed with spheroidal or pseudo-spheroidal geometry. It is observed that as long as the collapse is shear-free, its evolution depends only on the mass and size of the star at the onset of collapse.Comment: To appear in Pramana- j. of physic
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