Theory of Wetting-Induced Fluid Entrainment by Advancing Contact Lines on Dry Surfaces

We report on the onset of fluid entrainment when a contact line is forced to advance over a dry solid of arbitrary wettability. We show that entrainment occurs at a critical advancing speed beyond which the balance between capillary, viscous, and contact-line forces sustaining the shape of the interface is no longer satisfied. Wetting couples to the hydrodynamics by setting both the morphology of the interface at small scales and the viscous friction of the front. We find that the critical deformation that the interface can sustain is controlled by the friction at the contact line and the viscosity contrast between the displacing and displaced fluids, leading to a rich variety of wetting-entrainment regimes. We discuss the potential use of our theory to measure contact-line forces using atomic force microscopy and to study entrainment under microfluidic conditions exploiting colloid-polymer fluids of ultralow surface tension.

Spontaneous aggregation and global polar ordering in squirmer suspensions

We have developed numerical simulations of three dimensional suspensions of active particles to characterize the capabilities of the hydrodynamic stresses induced by active swimmers to promote global order and emergent structures in active suspensions. We have considered squirmer suspensions embedded in a fluid modeled under a Lattice Boltzmann scheme. We have found that active stresses play a central role to decorrelate the collective motion of squirmers and that contractile squirmers develop significant aggregates.

The 2010 May Flaring Episode of Cygnus X-3 in Radio, X-rays, and γ-rays

In 2009, Cygnus X-3 (Cyg X-3) became the first microquasar to be detected in the GeV γ-ray regime, via the satellites Fermi and AGILE. The addition of this new band to the observational toolbox holds promise for building a more detailed understanding of the relativistic jets of this and other systems. We present a rich data set of radio, hard and soft X-ray, and γ-ray observations of Cyg X-3 made during a flaring episode in 2010 May. We detect a ~3 day softening and recovery of the X-ray emission, followed almost immediately by a ~1 Jy radio flare at 15 GHz, followed by a 4.3σ γ-ray flare (E > 100 MeV) ~1.5 days later. The radio sampling is sparse, but we use archival data to argue that it is unlikely the γ-ray flare was followed by any significant unobserved radio flares. In this case, the sequencing of the observed events is difficult to explain in a model in which the γ-ray emission is due to inverse Compton scattering of the companion star's radiation field. Our observations suggest that other mechanisms may also be responsible for γ-ray emission from Cyg X-3.

Symmetries of the free Schrödinger equation in the non-commutative plane

We study all the symmetries of the free Schr odinger equation in the non-commu- tative plane. These symmetry transformations form an infinite-dimensional Weyl algebra that appears naturally from a two-dimensional Heisenberg algebra generated by Galilean boosts and momenta. These infinite high symmetries could be useful for constructing non-relativistic interacting higher spin theories. A finite-dimensional subalgebra is given by the Schröodinger algebra which, besides the Galilei generators, contains also the dilatation and the expansion. We consider the quantization of the symmetry generators in both the reduced and extended phase spaces, and discuss the relation between both approaches.

Symmetries of the free Schrödinger equation in the non-commutative plane

We study all the symmetries of the free Schrödinger equation in the non-commu- tative plane. These symmetry transformations form an infinite-dimensional Weyl algebra that appears naturally from a two-dimensional Heisenberg algebra generated by Galilean boosts and momenta. These infinite high symmetries could be useful for constructing non-relativistic interacting higher spin theories. A finite-dimensional subalgebra is given by the Schröodinger algebra which, besides the Galilei generators, contains also the dilatation and the expansion. We consider the quantization of the symmetry generators in both the reduced and extended phase spaces, and discuss the relation between both approaches.

Implementation of population balances in simulation of gas-liquid reactors using a CFD-PBM coupled approach

In bubbly flow simulations, bubble size distribution is an important factor in determination of hydrodynamics. Beside hydrodynamics, it is crucial in the prediction of interfacial area available for mass transfer and in the prediction of reaction rate in gas-liquid reactors such as bubble columns. Solution of population balance equations is a method which can help to model the size distribution by considering continuous bubble coalescence and breakage. Therefore, in Computational Fluid Dynamic simulations it is necessary to couple CFD and Population Balance Model (CFD-PBM) to get reliable distribution. In the current work a CFD-PBM coupled model is implemented as FORTRAN subroutines in ANSYS CFX 10 and it has been tested for bubbly flow. This model uses the idea of Multi Phase Multi Size Group approach which was previously presented by Sha et al. (2006) [18]. The current CFD-PBM coupled method considers inhomogeneous flow field for different bubble size groups in the Eulerian multi-dispersed phase systems. Considering different velocity field for bubbles can give the advantageof more accurate solution of hydrodynamics. It is also an improved method for prediction of bubble size distribution in multiphase flow compared to available commercial packages.

On the origin of the inertia: the modified Newtonian dynamics theory

The sameness between the inertial mass and the gravitational mass is an assumption and not a consequence of the equivalent principle is shown. In the context of the Sciama’s inertia theory, the sameness between the inertial mass and the gravitational mass is discussed and a certain condition which must be experimentally satisfied is given. The inertial force proposed by Sciama, in a simple case, is derived from the Assis’ inertia theory based in the introduction of a Weber type force. The origin of the inertial force is totally justified taking into account that the Weber force is, in fact, an approximation of a simple retarded potential, see [18, 19]. The way how the inertial forces are also derived from some solutions of the general relativistic equations is presented. We wonder if the theory of inertia of Assis is included in the framework of the General Relativity. In the context of the inertia developed in the present paper we establish the relation between the constant acceleration a0 , that appears in the classical Modified Newtonian Dynamics (M0ND) theory, with the Hubble constant H0 , i.e. a0 ≈ cH0 .

The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010

SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.

A Database of >20 keV Electron Green's Functions of Interplanetary Transport at 1 AU

We use interplanetary transport simulations to compute a database of electron Green's functions, i.e., differential intensities resulting at the spacecraft position from an impulsive injection of energetic (>20 keV) electrons close to the Sun, for a large number of values of two standard interplanetary transport parameters: the scattering mean free path and the solar wind speed. The nominal energy channels of the ACE, STEREO, and Wind spacecraft have been used in the interplanetary transport simulations to conceive a unique tool for the study of near-relativistic electron events observed at 1 AU. In this paper, we quantify the characteristic times of the Green's functions (onset and peak time, rise and decay phase duration) as a function of the interplanetary transport conditions. We use the database to calculate the FWHM of the pitch-angle distributions at different times of the event and under different scattering conditions. This allows us to provide a first quantitative result that can be compared with observations, and to assess the validity of the frequently used term beam-like pitch-angle distribution.

Spectral energy distribution of the gamma-ray microquasar LS 5039

The microquasar LS 5039 has recently been detected as a source of very high energy (VHE) $\gamma$-rays. This detection, that confirms the previously proposed association of LS 5039 with the EGRET source 3EG~J1824$-$1514, makes of LS 5039 a special system with observational data covering nearly all the electromagnetic spectrum. In order to reproduce the observed spectrum of LS 5039, from radio to VHE $\gamma$-rays, we have applied a cold matter dominated jet model that takes into account accretion variability, the jet magnetic field, particle acceleration, adiabatic and radiative losses, microscopic energy conservation in the jet, and pair creation and absorption due to the external photon fields, as well as the emission from the first generation of secondaries. The radiative processes taken into account are synchrotron, relativistic Bremsstrahlung and inverse Compton (IC). The model is based on a scenario that has been characterized with recent observational results, concerning the orbital parameters, the orbital variability at X-rays and the nature of the compact object. The computed spectral energy distribution (SED) shows a good agreement with the available observational data.

Kuplivan leijukerroksen poltto- ja lämpötekninen tarkastelu

Työn tavoitteena oli luoda menetelmä leijukerroskattilan petin lämpötilojen ja toiminta-alueen arvioimiseksi annetuilla lähtötiedoilla. Toimintatapana oli tutkia polttoaineen ominaisuuksien ja kattilan geometrian vaikutuksia petin energiataseeseen ja tätä kautta petin lämpötilaan kattilan ajotapa huomioiden. Työn teoriaosassa esitellään aluksi biopolttoaineiden ominaisuuksia ja leijukerroskattilan toimintaa petin toimintaympäristön selvittämiseksi. Teoriaosan lopussa käsitellään perusteellisesti petin hydrodynamiikkaa ja reaktiokinettikkaa sekä petin alueen mekaanista mitoitusta. Lisäksi polttoaineen syöttötapa ja palaminen petissä tuodaan esille. Tutkimusosassa selvitetään petin energiatasemallin määrittämistä teoriaan ja diplomityön aikana eri kattiloilla suoritettuihin mittauksiin perustuen. Mittauksista on erillinen selvitys seitsemännessä kappaleessa. Lopuksi kuvaillaan petin energiatasetta mallintavan menetelmän toimintaa sekä siihen syötettäviä lähtötietoja. Tuloksena on saatu suppealla alueella toimiva laajennettavissa oleva petin energiataseen malli. Menetelmän testaamiseen käytetään mittaustietoa kahdelta kattilalta, joita ei olla käytetty petin energiatasemallin virityksessä.

Measurement of a Structured Backflow in an Open Small Channel Induced by Surface-Tension Gradients

We present experiments in which the laterally confined flow of a surfactant film driven by controlled surface tension gradients causes the subtended liquid layer to self-organize into an inner upstream microduct surrounded by the downstream flow. The anomalous interfacial flow profiles and the concomitant backflow are a result of the feedback between two-dimensional and three-dimensional microfluidics realized during flow in open microchannels. Bulk and surface particle image velocimetry data combined with an interfacial hydrodynamics model explain the dependence of the observed phenomena on channel geometry.

Rheology of high solids surface size starches

Tämän diplomityön tarkoituksena oli tutkia pintaliimatärkkelysten reologista käyttäytymistä korkeissa kuiva-ainepitoisuuksissa. Tarve työn suorittamiselle syntyi kun tutkittiin pintaliimausta filminsiirtopuristimella tavallista korkeammissa kuiva-ainepitoisuuksissa, sileän sauvan ollessa applikointilaitteena. Koska applikointi sileällä sauvalla tapahtuu hydrodynaamisten periaatteiden mukaisesti, sen käyttö edellyttää pintaliimojen reologisten ominaisuuksien tarkkaa tuntemusta ja hallintaa.Kiinnostuksen kohteena olevat ominaisuudet olivat tärkkelysten kuiva-ainepitoisuuden (8 – 30 %) vaikutus viskositeettiin eri lämpötiloissa (20, 30, 40 ja 50 ºC), leikkausnopeus alueella 1 s-1 - 700 000 s-1. Myös tärkkelysten myötörajat määritettiin tutkimuksessa. Viskositeetti eri leikkausnopeusalueilla mitattiin seuraavilla laitteilla: Bohlin VOR (matalat leikkausnopeudet ja myötöraja) ja Hercules HiShear (keskitason leikkausnopeudet) reometrit sekä Eklund kapillaariviskometri (korkeat leikkausno-peudet). Analysoidut tärkkelykset olivat kaksi anionista matalaviskoottista peruna (tärkkelys A) ja ohra (tärkkelys C) tärkkelystä, sekä yksi kationinen korkeaviskoottinen peruna tärkkelys (tärkkelys B). Tutkittujen tärkkelysten Brookfield viskositeetit (100 rpm) olivat (10 % liuos, 60 °C:ssa) tärkkelys A ja C: 25 ± 5 mPas ja tärkkelys B: 100 ± 20 mPas.Tärkkelysliuosten kuiva-ainepitoisuuden noustessa muuttui virtauskäyttäytyminen Newtoniaalisesta leikkausohenevaksi. Leikkausoheneva käyttäytyminen oli voimakkainta tärkkelys B:n kohdalla. Viskositeetti – lämpötila riippuvuus korkeissa leikkausnopeuksissa (esim. 500 000 s-1) oli vähäisempää, mitä oli oletettavissa Brookfield viskositeettiarvojen perusteella. Kaikki tarkkelykset osoittautuivat tiksotrooppisiksi, myös tiksotrooppisuus lisääntyi kuiva-ainepitoisuuden kasvaessa. Tärkkelysten myötörajat osoittautuivat odottamattoman alhaisiksi, kuitenkin varsinkin tärkkelys B:n myötörajat olivat selvästi riippuvaisia lämpötilasta ja kuiva-ainepitoisuudesta. Tutkittujen tärkkelysten virtauskäyttäytyminen oli kirjallisuudessa esitetyn kaltaista. Tärkkelysmolekyylien ketjun pituus oli tärkein tärkkelyksen reologisia ominaisuuksia määrittävä tekijä; mitä matalampi on tärkkelyksen molekyylimassa, sitä matalammat ovat viskositeetti ja myötöraja. Pintaliimauksessa tärkkelysmolekyylien ketjunpituudella on suuri vaikutus ajettavuuteen ja lopputuotteen ominaisuuksiin. Haasteellista pintaliimatärkkelyksen valinnassa on sellaisen yhdistelmän löytäminen, jossa sopivan reologisen käyttäytymisen omaava tärkkelys ja pintaliimatulle paperille tai kartongille asetetut vaatimukset kohtaavat.

From Full stopping to transparency in a holographic model of heavy ion collisions

We numerically simulate planar shock wave collisions in anti-de Sitter space as a model for heavy ion collisions of large nuclei. We uncover a crossover between two different dynamical regimes as a function of the collision energy. At low energies the shocks first stop and then explode in a manner approximately described by hydrodynamics, in close similarity with the Landau model. At high energies the receding fragments move outwards at the speed of light, with a region of negative energy density and negative longitudinal pressure trailing behind them. The rapidity distribution of the energy density at late times around midrapidity is not approximately boost invariant but Gaussian, albeit with a width that increases with the collision energy.

Kiertoleijukattilan tulipesän lämmönsiirtoprofiilien määritys ja mallinnus

Tämä diplomityö on osa projektia, joka tähtää ylikriittisellä painealueella toimivan läpivirtaustekniikkaan perustuvan kiertoleijukattilan toteuttamiseen. Diplomityössä määritetään mittausten perusteella vaaka- ja pystysuuntaisia lämmönsiirtoprofiileja kaupallisen kiertoleijukattilan tulipesässä. Lisäksi samaisen kattilan tulipesä mallinnetaan ja mallin parametrejä säädetään niin, että mallin tulokset saadaan vastaamaan mitattuja tuloksia mahdollisimman hyvin. Työn tavoitteena on antaa lisätietoa tulipesässä vapautuvan lämpötehon jakautumisesta tulipesän eri osien kesken. Diplomityön kirjallisuuskatsauksessa käsitellään kiertoleijukattilan tulipesän perusilmiöitä kuten leijutusta, lämmönsiirtoa, hydrodynamiikkaa ja palamista sekä tutustutaan muutamiin tulipesämalleihin. Lisäksi tarkastellaan ylikriittisen läpivirtauskattilan tarjoamia etuja perinteisiin kattilaratkaisuihin nähden. Diplomityössä on myös esitelty työhön liittyvä mittausprojekti.