Investigations of certain eco-physiological characteristics of the broad and long-pincered crayfish in connection with their interspecific relationships. [Translation from: Lietuvas TSR Mokslu Akademijos Darbai, C Serija 2(40), 279-286, 1966.]

The results are described of eco-physiological investigations of the broad-pincered (Astacus astacus L.J.) crayfish and the long-pincered (Astacus astacus Esch.) crayfish, conducted in 1963—64 in the Institute of Zoology and Parasitology of the Academy of Science of the Lithuanian SSR, for the purpose of studying the interspecific relationship of these two species. In the course of the investigation were determined: the influence of the temperature of the environment on the consumption of oxygen by full grown individuals of both species and on the respiratory movements of the scaphognathites, the threshold temperatures and the saturation of the water by oxygen, the diel activity in the winter period.

Fundamental aspects of the feeding of the amphipod Gammarus (R.) balcanicus (Crustacea, Amphipoda). [Translation from: Nauchn.Dokl.vyssh.Shkoly (Biol.Nauk) 1970(7) 12-16, 1970]

The amphipods are major food items for many commercial fishes, and they are used as protein food for agricultural animals. In the present paper are presented the results of four-year observations on the feeding of Gammarus balcanicus in nature and in an aquarium. Among the studied aspects were the dependence of daily food ration on sex and physiological state (with and without eggs) and feeding on different kinds of plant food. The study concludes that Gammarus balcanicus willingly feed on soft half-decayed plant residues; into their ration also enters food of animal origin. In contrast to other amphipods, G. balcanicus eats representatives of its own species very rarely, and only dead or immobile ones.

Toward Understanding Astrophysical Phenomena

Fast radio bursts (FRBs), a novel type of radio pulse, whose physics is not yet understood at all. Only a handful of FRBs had been detected when we started this project. Taking account of the scant observations, we put physical constraints on FRBs. We excluded proposals of a galactic origin for their extraordinarily high dispersion measures (DM), in particular stellar coronas and HII regions. Therefore our work supports an extragalactic origin for FRBs. We show that the resolved scattering tail of FRB 110220 is unlikely to be due to propagation through the intergalactic plasma. Instead the scattering is probably caused by the interstellar medium in the FRB's host galaxy, and indicates that this burst sits in the central region of that galaxy. Pulse durations of order $\ms$ constrain source sizes of FRBs implying enormous brightness temperatures and thus coherent emission. Electric fields near FRBs at cosmological distances would be so strong that they could accelerate free electrons from rest to relativistic energies in a single wave period. When we worked on FRBs, it was unclear whether they were genuine astronomical signals as distinct from `perytons', clearly terrestrial radio bursts, sharing some common properties with FRBs. Recently, in April 2015, astronomers discovered that perytons were emitted by microwave ovens. Radio chirps similar to FRBs were emitted when their doors opened while they were still heating. Evidence for the astronomical nature of FRBs has strengthened since our paper was published. Some bursts have been found to show linear and circular polarizations and Faraday rotation of the linear polarization has also been detected. I hope to resume working on FRBs in the near future. But after we completed our FRB paper, I decided to pause this project because of the lack of observational constraints.

The pulsar triple system, J0733+1715, has its orbital parameters fitted to high accuracy owing to the precise timing of the central $\ms$ pulsar. The two orbits are highly hierarchical, namely $P_{\mathrm{orb,1}}\ll P_{\mathrm{orb,2}}$, where 1 and 2 label the inner and outer white dwarf (WD) companions respectively. Moreover, their orbital planes almost coincide, providing a unique opportunity to study secular interaction associated purely with eccentricity beyond the solar system. Secular interaction only involves effect averaged over many orbits. Thus each companion can be represented by an elliptical wire with its mass distributed inversely proportional to its local orbital speed. Generally there exists a mutual torque, which vanishes only when their apsidal lines are parallel or anti-parallel. To maintain either mode, the eccentricity ratio, $e_1/e_2$, must be of the proper value, so that both apsidal lines precess together. For J0733+1715, $e_1\ll e_2$ for the parallel mode, while $e_1\gg e_2$ for the anti-parallel one. We show that the former precesses $\sim 10$ times slower than the latter. Currently the system is dominated by the parallel mode. Although only a little anti-parallel mode survives, both eccentricities especially $e_1$ oscillate on $\sim 10^3\yr$ timescale. Detectable changes would occur within $\sim 1\yr$. We demonstrate that the anti-parallel mode gets damped $\sim 10^4$ times faster than its parallel brother by any dissipative process diminishing $e_1$. If it is the tidal damping in the inner WD, we proceed to estimate its tidal quantity parameter ($Q$) to be $\sim 10^6$, which was poorly constrained by observations. However, tidal damping may also happen during the preceding low-mass X-ray binary (LMXB) phase or hydrogen thermal nuclear flashes. But, in both cases, the inner companion fills its Roche lobe and probably suffers mass/angular momentum loss, which might cause $e_1$ to grow rather than decay.

Several pairs of solar system satellites occupy mean motion resonances (MMRs). We divide these into two groups according to their proximity to exact resonance. Proximity is measured by the existence of a separatrix in phase space. MMRs between Io-Europa, Europa-Ganymede and Enceladus-Dione are too distant from exact resonance for a separatrix to appear. A separatrix is present only in the phase spaces of the Mimas-Tethys and Titan-Hyperion MMRs and their resonant arguments are the only ones to exhibit substantial librations. When a separatrix is present, tidal damping of eccentricity or inclination excites overstable librations that can lead to passage through resonance on the damping timescale. However, after investigation, we conclude that the librations in the Mimas-Tethys and Titan-Hyperion MMRs are fossils and do not result from overstability.

Rubble piles are common in the solar system. Monolithic elements touch their neighbors in small localized areas. Voids occupy a significant fraction of the volume. In a fluid-free environment, heat cannot conduct through voids; only radiation can transfer energy across them. We model the effective thermal conductivity of a rubble pile and show that it is proportional the square root of the pressure, $P$, for $P\leq \epsy^3\mu$ where $\epsy$ is the material's yield strain and $\mu$ its shear modulus. Our model provides an excellent fit to the depth dependence of the thermal conductivity in the top $140\,\mathrm{cm}$ of the lunar regolith. It also offers an explanation for the low thermal inertias of rocky asteroids and icy satellites. Lastly, we discuss how rubble piles slow down the cooling of small bodies such as asteroids.

Electromagnetic (EM) follow-up observations of gravitational wave (GW) events will help shed light on the nature of the sources, and more can be learned if the EM follow-ups can start as soon as the GW event becomes observable. In this paper, we propose a computationally efficient time-domain algorithm capable of detecting gravitational waves (GWs) from coalescing binaries of compact objects with nearly zero time delay. In case when the signal is strong enough, our algorithm also has the flexibility to trigger EM observation {\it before} the merger. The key to the efficiency of our algorithm arises from the use of chains of so-called Infinite Impulse Response (IIR) filters, which filter time-series data recursively. Computational cost is further reduced by a template interpolation technique that requires filtering to be done only for a much coarser template bank than otherwise required to sufficiently recover optimal signal-to-noise ratio. Towards future detectors with sensitivity extending to lower frequencies, our algorithm's computational cost is shown to increase rather insignificantly compared to the conventional time-domain correlation method. Moreover, at latencies of less than hundreds to thousands of seconds, this method is expected to be computationally more efficient than the straightforward frequency-domain method.

A study of nonlinear phenomena in the propagation of electromagnetic waves in a weakly ionized gas

This thesis is a study of nonlinear phenomena in the propagation of electromagnetic waves in a weakly ionized gas externally biased with a magnetostatic field. The present study is restricted to the nonlinear phenomena rising from the interaction of electromagnetic waves in the ionized gas. The important effects of nonlinearity are wave-form distortion leads to cross modulation of one wave by a second amplitude-modulated wave.

The nonlinear effects are assumed to be small so that a perturbation method can be used. Boltzmann’s kinetic equation with an appropriate expression for the collision term is solved by expanding the electron distribution function into spherical harmonics in velocity space. In turn, the electron convection current density and the conductivity tensors of the nonlinear ionized gas are found from the distribution function. Finally, the expression for the current density and Maxwell’s equations are employed to investigate the effects of nonlinearity on the propagation of electromagnetic waves in the ionized gas, and also on the reflection of waves from an ionized gas of semi-infinite extent.

Mössbauer effect investigations of the hyperfine interactions and relaxation phenomena in salts of thulium

Two new phenomena have been observed in Mössbauer spectra: a temperature-dependent shift of the center of gravity of the spectrum, and an asymmetric broadening of the spectrum peaks. Both phenomena were observed in thulium salts. In the temperature range 1˚K ≤ T ≤ 5˚K the observed shift has an approximate inverse temperature dependence. We explain this on the basis of a Van Vleck type of interaction between the magnetic moment of two nearly degenerate electronic levels and the magnetic moment of the nucleus. From the size of the shift we are able to deduce an “effective magnetic field” H = (6.0 ± 0.1) x 10⁶ Gauss, which is proportional to ‹r^-3›_M‹G|J|E› where ‹r^-3›_M is an effective magnetic radial integral for the 4f electrons and |G› and |E› are the lowest 4f electronic states in Tm Cl₃·6H₂O. From the temperature dependence of the shift we have derived a preliminary value of 1 cm^-1 for the splitting of these two states. The observed asymmetric line broadening is independent of temperature in the range 1˚K ≤ T ≤ 5˚K, but is dependent on the concentration of thulium ions in the crystal. We explain this broadening on the basis of spin-spin interactions between thulium ions. From size and concentration dependence of the broadening we are able to deduce a spin-spin relaxation time for Tm Cl₃·6H₂O of the order of 10^-11 sec.

Observations on the physiological development of trout eggs [Translation from: Roux. Arch. f. Entwicklungsmechanik der Organismen, 114. 771, 1929]

The osmotic pressure of the perivitelline fluid and the yolk of trout (Salmo trutta) eggs were measured separately by the Drucker-Schrein method. The permeability of the egg membrane and the variations in the osmotic pressure of the eggs when placed in salt solutions were also investigated.

Analisis de las entidades no lucrativas del Pais Vasco dedicadas a la protección animal

This Final Project Grade, whose title is “Analysis of the non-lucrative entities of the Basque Country dedicated to animal protection”, has as main purpose the study of the historical, theoretical and legal context in which these institutions develop their activity, focusing in those which occur in the Basque Country.

I. The effect of droplet solidification upon two-phase flow in a rocket nozzle. II. A kinetic theory investigation of some condensation-evaporation phenomena by a moment method

Part I:

The perturbation technique developed by Rannie and Marble is used to study the effect of droplet solidification upon two-phase flow in a rocket nozzle. It is shown that under certain conditions an equilibrium flow exists, where the gas and particle phases have the same velocity and temperature at each section of the nozzle. The flow is divided into three regions: the first region, where the particles are all in the form of liquid droplets; a second region, over which the droplets solidify at constant freezing temperature; and a third region, where the particles are all solid. By a perturbation about the equilibrium flow, a solution is obtained for small particle slip velocities using the Stokes drag law and the corresponding approximation for heat transfer between the particle and gas phases. Singular perturbation procedure is required to handle the problem at points where solidification first starts and where it is complete. The effects of solidification are noticeable.

Part II:

When a liquid surface, in contact with only its pure vapor, is not in the thermodynamic equilibrium with it, a net condensation or evaporation of fluid occurs. This phenomenon is studied from a kinetic theory viewpoint by means of moment method developed by Lees. The evaporation-condensation rate is calculated for a spherical droplet and for a liquid sheet, when the temperatures and pressures are not too far removed from their equilibrium values. The solutions are valid for the whole range of Knudsen numbers from the free molecule to the continuum limit. In the continuum limit, the mass flux rate is proportional to the pressure difference alone.

Physiological ecology of the ciliated protozoon Loxodes

Loxodes faces special problems in living close to the oxic-anoxic boundary. In tightly-stratified ponds like Priest Pot its optimum environment may be quite narrow and it can be displaced by the slightest turbulence. Loxodes cannot sense an O sub(2) gradient directly but its ability to perceive gravity allows it to make relatively long vertical migrations. It is also sensitive to light and oxygen and it uses these environmental cues to modulate the parameters of its random motility: in the dark, it aggregates at a low O sub(2) tension and in bright light it aggregates in anoxic water. The oxic-anoxic boundary is also a zone where O sub(2) may be a scarce and transient resource, but Loxodes) can switch to nitrate respiration and exploit the pool of nitrate that often exists close to the base of the oxycline.

Behavior ecology of the Humboldt squid, Dosidicus gigas: insights from an animal-borne video and data logging system

Dosidicus gigas is a large pelagic cephalopod of the eastern Pacific that has recently undergone an unexpected, significant range expansion up the coast of North America. The impact that such a range expansion is expected to have on local fisheries and marine ecosystems has motivated a thorough study of this top predator, a squid whose lifestyle has been quite mysterious until recently. Unfortunately, Dosidicus spends daylight hours at depths prohibitive to making observations without significant artificial interference. Observations of this squid‟s natural behaviors have thus far been considerably limited by the bright illumination and loud noises of remotely-operated-vehicles, or else the presence of humans from boats or with SCUBA. However, recent technological innovations have allowed for observations to take place in the absence of humans, or significant human intrusion, through the use of animal-borne devices such as National Geographic‟s CRITTERCAM. Utilizing the advanced video recording and data logging technology of this device, this study seeks to characterize unknown components of Dosidicus gigas behavior at depth. Data from two successful CRITTERCAM deployments reveal an assortment of new observations concerning Dosidicus lifestyle. Tri-axial accelerometers enable a confident description of Dosidicus orientation during ascents, descents, and depth maintenance behavior - previously not possible with simple depth tags. Video documentation of intraspecific interactions between Dosidicus permits the identification of ten chromatic components, a previously undescribed basal chromatic behavior, and multiple distinct body postures. And finally, based on visualizations of spermatophore release by D. gigas and repetitive behavior patterns between squid pairs, this thesis proposes the existence of a new mating behavior in Dosidicus. This study intends to provide the first glimpse into the natural behavior of Dosidicus, establishing the groundwork for a comprehensive ethogram to be supported with data from future CRITTERCAM deployments. Cataloguing these behaviors will be useful in accounting for Dosidicus‟ current range expansion in the northeast Pacific, as well as to inform public interest in the impacts this expansion will have on local fisheries and marine ecosystems.

Relógios biológicos e padrões de alimentação em camundongos normais e com sobrepeso

A saudável interação entre o indivíduo e o meio depende do alinhamento entre a dinâmica fisiológica do primeiro e os periódicos movimentos da natureza. A interação entre tais ritmos por sua vez constitui-se em base e derivação do processo de evolução. O comprometimento de tal alinhamento representa um risco para a sobrevivência das espécies. Neste contexto, os organismos alinham seus ritmos fisiológicos a diferentes ciclos externos. Desta forma, ciclos endógenos são coordenados por relógios biológicos que determinam em nosso organismo, específicos ritmos em fase com a natureza, tais como ritmos circadianos (RC), cujo período aproxima-se de 24 horas. O peso corporal, a ingestão de alimentos e o consumo de energia são processos caracterizados pelo RC e a obesidade está associada a uma dessincronização deste processo. A modulação do RC é resultado da expressão dos clock gens CLOCK e BMAL1 que formam um heterodímero responsável pela transcrição gênica de Per1, Per2, Per3, Cry1 e Cry2. As proteínas codificadas por estes genes, uma vez sintetizadas, formam dímeros (PER-CRY) no citoplasma que, a partir de determinada concentração, retornam ao núcleo, bloqueando a ação do heterodímero CLOCK/BMAL1 na transcrição dos próprios genes, formando assim uma alça de retroalimentação negativa de transcrição e tradução. Estes genes asseguram a periodicidade e são significativamente expressos no núcleo supraquiasmático (SCN) do hipotálamo. Para estudar esse processo em camundongos normais e hiperalimentados, saciados e em estado de fome, foi utilizado um método de registro do comportamento alimentar baseado no som produzido pela alimentação dos animais, e a correlação destes estados metabólicos com a expressão de CLOCK, BMAL1, Per1, Per2, Per3, bem como das proteínas Cry1 e Cry2 no SCN, por análise de imagens obtidas em microscopia confocal. Camundongos suíços controle em estado de fome (CF) e saciados (CS) foram comparados com animais hiperalimentados com fome (HF) e saciados (HS). Nenhum grupo demonstrou diferença nos conteúdos CLOCK e BMAL1, indicando capacidade potencial para modular os ritmos biológicos. No entanto, as proteínas Per1, Per2, Per3 e Cry1 apresentaram menor expressão no grupo CS, mostrando uma diferença significativa quando comparados com o grupo CF (P<0,05), diferença esta não encontrada na comparação entre os grupos HF e HS. A quantidade de proteína Cry2 não foi diferente na mesma comparação. Os resultados do estudo indicaram que as alterações dos ritmos endógenos e exógenos, refletido pelo comportamento hiperfágico observado em camundongos hiperalimentados, pode ser devido a um defeito no mecanismo de feedback negativo associado ao dímero Cry-Per, que não bloqueia a transcrição de Per1 Per2, Per3 e Cry1 pelo heterodímero CLOCK-BMAL1.

Spin-related phenomena in magnetic and spin-orbit couppled bose-einstein condensates

129 p.

Estudo da bioenergética mitocondrial de cardiomiócitos de camundongos obesos

A obesidade é uma doença crônica, resultante do excesso de gordura no organismo. O aumento da obesidade no mundo, tem se revelado como um dos fenômenos clínicos e epidemiológicos da atualidade. Estudos populacionais e em modelos animais demonstram que a origem da epidemia da obesidade está relacionada a fatores genéticos, modificações de hábitos nutricionais, redução da atividade física, e alterações nutricionais durante a lactação, desempenhando um papel relevante no desenvolvimento da obesidade, DM2 e cardiomiopatias. As mitocôndrias são os coordenadores centrais do metabolismo energético, assim, alterações funcionais e estruturais dessa organela têm sido associadas à desordens metabólicas. Elas exercem um papel na sobrevivência e função dos cardiomiócitos devido à alta demanda energética do miocárdio. Desta forma, disfunções mitocondriais estão relacionadas com disfunções no miocárdio e conseqüente progressão de cardiomiopatias. Neste estudo, avaliamos a bioenergética e a ultraestrutura de cardiomiócitos de camundongos obesos e controle hiperalimentados durante a lactação. O consumo de oxigênio das fibras cardíacas foi avaliado por respirometria de alta-resolução, utilizando um oxígrafo-2K-Oroboros. A ultraestrutura dos cardiomiócitos foi analisada por microscopia eletrônica de transmissão e o conteúdo das proteínas Carnitina palmitoil transferase 1 (CPT1), Proteína desacopladora 2 (UCP2) , Transportador de glicose 1 e 4 (GLUT1) e (GLUT4), Proteína Kinase ativada por AMP (AMPK) e Proteína kinase ativada por AMP fosforilada p(AMPK) por Western blotting (WB). Além disso, o peso dos animais, a gordura retroperitoneal, epididimal e a glicemia em jejum foram determinadas. Nossos resultados confirmaram que os animais do grupo hiperalimentados (GH), aos 90 dias de vida, apresentaram aumento da massa corporal, de gordura epididimária e retroperitoneal comparado ao grupo controle (GC). As taxas respiratórias foram semelhantes nos dois grupos quando foram utilizados os substratos dos complexos I e II. Entretanto, quando o ácido graxo palmitoil-L-carnitina foi utilizado, a taxa respiratória máxima do GH foi significativamente menor. A análise ultraestrutural dos cardiomiócitos do GH demonstrou intenso dano na matriz mitocondrial e maior presença de gotículas de lipídios, caracterizando deposição ectópica. Os resultados do WB mostraram aumento significativo do conteúdo de CPT1 e UCP2 no GH comparado ao GC. Não foram encontradas diferenças significativas no conteúdo de GLUT1 entre os grupos, entretanto, observamos maior conteúdo do GLUT4 no GH. Além disso, encontramos maior conteúdo de AMPK no GH, ao passo que o conteúdo de pAMPK foi semelhante entre os grupos. Entretanto, a razão pAMPK/AMPK é significativamente menor no GH. Esses resultados sugerem que a hiperalimentação durante a lactação leva a obesidade na vida adulta com alterações na bioenergética e ultraestrutura dos cardiomiócitos.

Efeito da superalimentação neonatal sobre a função adrenal e o desenvolvimento da microesteatose hepática em ratos adultos

O estado nutricional e hormonal em fases iniciais de desenvolvimento (gestação e lactação) está relacionado a alterações epigenéticas, que podem levar ao desenvolvimento de doenças. A obesidade infantil está relacionada com a ocorrência da obesidade na idade adulta, resistência à insulina e maior risco cardiometabólico. Em estudos experimentais, a superalimentação neonatal causa obesidade e aumenta o risco de doenças cardiovasculares. Estes animais apresentam obesidade visceral, hiperfagia, hiperleptinemia e hipertensão na idade adulta. Previamente, demonstramos que a hiperleptinemia neonatal causa hiperfunção da medula adrenal e microesteatose na idade adulta. No presente estudo avaliamos a função adrenal de ratos adultos obesos no modelo de superalimentação neonatal por redução do tamanho da ninhada e a sensibilidade as catecolaminas no tecido adiposo visceral (TAV) e no fígado. Ao nascimento todas as ninhadas tiveram seu número de filhotes ajustados para 10. Para induzir a superalimentação neonatal, o tamanho da ninhada foi reduzido de dez para três filhotes machos no terceiro dia de lactação até o desmame (SA), enquanto que o grupo controle permaneceu com 10 filhotes durante toda a lactação. Após o desmame, os ratos tiveram livre acesso à dieta padrão e água até 180 dias (1 animal de cada ninhada, n = 7). O TAV e as glândulas adrenais foram pesadas. As contrações hormonais séricas, o conteúdo hepático de glicogênio e triglicerídeos foram avaliados por kits comerciais. O conteúdo e a secreção de catecolaminas adrenais foram avaliados utilizando o método do trihidroxindol. O conteúdo dos hormônios eixo hipotálamo-hipófise-córtex adrenal, das enzimas da via de síntese das catecolaminas na glândula adrenal, ADRB2 no fígado e ADRB3 no TAV foram determinados por Western blotting ou imunohistoquímica. As diferenças foram consideradas significativas quando p <0,05. Aos 180 dias de vida, o grupo SA apresentou maior massa corporal (+15%), maior consumo alimentar (+15%) e maior adiposidade visceral (+79%). Os hormônios do eixo hipotálamo-hipófise-córtex-adrenal não foram alterados. O grupo SA apresentou maior expressão de tirosina hidroxilase e de DOPA descarboxilase (+31% e 90%, respectivamente); conteúdo de catecolaminas adrenais (absoluta: 35% e relativa: 40%), e secreção de catecolaminas, tanto basal quanto estimulada por cafeína (+35% e 43%, respectivamente). O conteúdo ADRB3 no TAV não foi alterado nos grupo SA, entretanto o ADRB2 no fígado apresentou-se menor (-45%). O grupo SA apresentou maior conteúdo de glicogênio e triglicerídeos no fígado (+79% e +49%, respectivamente), além de microesteatose. A superalimentação neonatal resulta em hiperativação adrenomedular e aparentemente está associada a preservação da sensibilidade às catecolaminas no VAT. Adicionalmente sugerimos que o maior conteúdo de glicogênio e triglicerídeos hepático seja devido a menor sensibilidade as catecolaminas. Tal perfil pode contribuir para a disfunção metabólica hepática e hipertensão arterial que são características deste modelo de obesidade programada.