AMS est un détecteur de particules qui sera embarqué à bord de la Station Spatiale Internationale début 2008. Avec son trajectomètre en silicium et son calorimètre électromagnétique, il pourra détecter les photons entre 1 GeV et 300 GeV. <br />Dans la première partie de cette thèse, nous donnons les résultats obtenus lors de l'analyse des données d'un test sur faisceau du calorimètre électromagnétique. A l'aide d'un logiciel de simulation rapide, nous évaluons les capacités de détection d'AMS en gamma. Nous donnons des prédictions de flux pour différents types de sources astrophysiques et pour un halo de matière noire supersymétrique au centre galactique.<br />HETE-2 est un satellite actuellement en fonctionnement qui est conçu pour détecter et localiser les sursauts gamma. Du fait des énergies mises en jeu, ce type de source pourrait être utilisé pour tester des domaines de la physiques inaccessibles aux accélérateurs. <br />Dans la deuxième partie de la thèse, nous étudions les courbes de lumières de douze sursauts gamma observés par le détecteur FREGATE à bord d'HETE-2 et pour lesquels une mesure du redshift est disponible. En étudiant les écarts temporels entre des photons de différentes énergies, nous pouvons déterminer une limite inférieure sur l'échelle de gravitation quantique de Eqg > 10^15 GeV.

No description available.

Au delà de la simple définition formelle d'un trou noir comme solution des équations d'Einstein dans le vide, il existe, comme l'a souligné Kip Thorne, depuis 1971 et l'observation du système binaire Cygnus X1, jusqu'aux hypothèses les plus récentes relatives à l'existence de trous noirs supermassifs au centre de nombreuses galaxies, des indices observationnels confortant leur existence dans l'Univers et motivant ainsi leur étude. En physique, nous le savons, pour obtenir des informations essentielles sur les interactions entre particules fondamentales, atomes, molécules, etc..., ainsi que sur la structure des objets composés, nous devons procéder à des expériences de collision ou plus précisément de diffusion. C'est ce qui constitue précisément l'objet de ce travail de thèse. En effet, en analysant comment un trou noir interagit avec son environnement, nous sommes en droit d'attendre des informations essentielles sur ces ''objets invisibles''. Cette étude sera également très utile pour comprendre, notamment, le signal que l'on devrait recevoir, prochainement, par le biais de la nouvelle génération de détecteurs d'ondes gravitationnelles. Ce travail se concentre donc principalement sur les phénomènes sous-jacents aux processus de diffusion par des trous noirs, i.e. les phénomènes de résonance et d'absorption. Toute l'originalité de cette étude repose sur le fait que nous proposons de nous intéresser à ces phénomènes du point de vue d'une théorie semiclassique dite " théorie du moment angulaire complexe ", mettant ainsi au cœur de la physique des trous noirs les concepts de matrice S ainsi que les techniques relatives aux pôles de Regge, tel que l'a suggéré implicitement Chandrasekhar au milieu des années soixante-dix. Cette approche nous permet de donner une interprétation physique, simple et intuitive, des phénomènes de résonance et d'absorption d'un champ, en l'occurrence d'un champ scalaire, massif ou non, par des trous noirs.

Στη γραμμική εκδοχή της γενικής θεωρίας της σχετικότητας, θεωρεί κανείς τις διαταραχές κάποιας μετρικής γύρω από κάποιο χωροχρονικό υπόβαθρο. Κρατώντας όρους διαταραχών μέχρι και πρώτης τάξεως, οδηγείται κανείς στις γραμμικές εξισώσεις Einstein. Σε αυτό το πλαίσιο αποδεικνύεται μια σχέση δυισμού ανάμεσα στα διάφορα στοιχεία του τανυστή Weyl, αντίστοιχη με το δυισμό ανάμεσα στην ηλεκτρική και τη μαγνητική ροή της ηλεκτρομαγνητικής θεωρίας του Maxwell. Στην εργασία αυτή κάνουμε μία ανασκόπηση της έρευνας που έχει γίνει μέχρι τώρα αναφορικά με αυτές τις σχέσεις δυισμού. Πιο συγκεκριμένα, εξετάζουμε την ισχύ των σχέσεων στον Anti-de Sitter χωρόχρονο και επισημαίνουμε το τρόπο με τον οποίο κατασκευάζει κανείς δυικές δομές από τις εκφράσεις για τις διαταραχές. Επίσης, χρησιμοποιώντας τη τεχνική της ολογραφικής επανακανονικοποίησης, εξετάζουμε το σύμμορφο σύνορο του χωροχρόνου. Βρίσκουμε εκεί μια σχέση δυισμού ανάμεσα στα στοιχεία του τανυστή ενέργειας-ορμής και του τανυστή Cotton της αντίστοιχης Chern - Simons θεωρίας, η οποία αποδεικνύεται ότι είναι άμεση συνέπεια του δυισμού στο AdS υπόβαθρο. Τέλος, εφαρμόζουμε την ίδια συλλογιστική στο Schwarzschild - Anti-de Sitter υπόβαθρο, όπου η παρουσία της μελανής οπής διαφοροποιεί τις συνοριακές συνθήκες του προβλήματος. Λόγω αυτού του γεγονός δεν μπορεί να πει κανείς με σιγουριά εάν μπορούν να διατυπωθούν σχέσεις δυισμού σε αυτή τη περίπτωση. Παρόλα αυτά βρίσκουμε ότι ισχύουν σχέσεις δυισμού στο σύμμορφο σύνορο παρόμοιες με αυτές του AdS υποβάθρου, πράγμα που σημαίνει ότι στο σύστημα παραμένει κάποια συμμετρία από τη γραμμική θεωρία. Η εργασία καταλήγει σε σχόλια και μία εκτενή συζήτηση για τις πιθανές μελλοντικές κατευθύνσεις. / In the linear version of the general theory of relativity, one considers metric perturbations around a fixed background. Keeping terms up to first order of perturbation leads to the linearized Einstein equations. In this framework it has been proved that a duality between the various elements of the Weyl tensor holds. This duality is similar to the one between the electric and magnetic fluxes of Maxwell's electromagnetism. In the present work we review the status of these dualities for non trivial backgrounds. We examine the Anti-de Sitter background, where we point out the way to explicitly construct dual configurations using the metric perturbation expressions. Using the holographic renormalization technique, we examine the conformal boundary where a duality between the components of the energy-momentum tensor and the Cotton tensor of the corresponding Chern - Simons theory holds. It is then proved that this duality is a direct consequence of the electric/magnetic duality in the bulk, in the case of the AdS background. Finally, we apply same procedure to the Schwarzschild - Anti-de Sitter background, where the presence of the black hole changes the boundary conditions of the problem. This simple fact makes it impossible say whether such a duality exists in this case. Nevertheless, we find that a duality similar to that of the AdS background still holds for the conformal boundary, which means that there is a remnant of symmetry from the linear theory. We conclude with comments and a extensive discussion on possible future directions.

Submitted by Vasti Diniz (vastijpa@hotmail.com) on 2017-09-12T12:08:23Z No. of bitstreams: 1 arquivototal.pdf: 3631858 bytes, checksum: 8e326a8bf5b797bf3b1919d031583614 (MD5) / Made available in DSpace on 2017-09-12T12:08:23Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 3631858 bytes, checksum: 8e326a8bf5b797bf3b1919d031583614 (MD5) Previous issue date: 2017-07-19 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / In this work, we consider a charged massive fermionic quantum field in the idealized cosmic string spacetime and in the presence of a magnetic field confined in a cylindrical tube of finite radius. Three distinct configurations for the magnetic fields are taken into account: (i) a cylindrical shell of radius a, (ii) a magnetic field proportional to 1/r and (iii) a constant magnetic field. In these three cases, the axis of the infinitely long tube of radius a coincides with the cosmic string. Our main objectives in this paper are to analyze vacuum expected values (VEVs) of the current density, jP, fermionic condensate (FC) e and the VEV of the fermionic energy-momentum tensor, Ti". In order to do that, we explicitly construct the complete set of normalized wave-functions for each configuration of magnetic field. We show that in the region outside the tube, the current density, the FC and the VEV of the energy-momentum tensor are decomposed into two parts: the first ones correspond to the zero-thickness magnetic flux contributions, and the seconds are induced by the non-trivial structure of the magnetic field, named core-induced contributions. The latter present specific forms depending on the magnetic field configuration considered. We also show that the VEV of the energy-momentum tensor is diagonal, obeys the conservation condition and its trace is expressed in terms of the fermionic condensate. / Nesta Tese, consideramos urn campo fermiônico massivo e carregado no espaço-tempo de uma corda cósmica ideal na presença de um campo magnético confinado em um tubo cilindrico de raio finito a. Levamos em conta três configurações para o campo magnético: (i) uma casca cilindrica de raio a, (ii) um campo magnetico proporcional a 1/r e (iii) urn campo magnetico constante. Nos três casos, o eixo de simetria da corda cósmica coincide corn o eixo de simetria do tubo cilindrico de campo magnetico, dispostos ao longo do eixo z. Nossos principais objetivos nesta Tese sao analisar os valores esperados no yam° (VEV) da densidade de corrente, ji", do condensado fermionico (FC) e o VEV do tensor energia-momento (TEM), Ti". Para isto, construfmos urn conjunto completo de fungoes de onda de Dirac normalizadas para cada configuragao de campo magnetic° e mostramos que na regiao fora do tubo, a densidade de corrente, o CF e o VEV do TEM sao decompostos como a soma de duas partes. A primeira corresponde a contribuigao da linha de fluxo magnetic° que corre ao longo da corda cOsmica ideal, e a segunda contribuigao é induzida devido a estrutura nao trivial de campo magnetic°. Mostramos tambem que o VEV do tensor energia-momento é diagonal, obedece a condigao de conservagao e que seu trago é expresso ern termos do condensado fermionico.

Submitted by Vasti Diniz (vastijpa@hotmail.com) on 2017-09-18T12:28:21Z No. of bitstreams: 1 arquivototal.pdf: 2590482 bytes, checksum: a72ba5c8c44731f3cffe38777111a92d (MD5) / Made available in DSpace on 2017-09-18T12:28:21Z (GMT). No. of bitstreams: 1 arquivototal.pdf: 2590482 bytes, checksum: a72ba5c8c44731f3cffe38777111a92d (MD5) Previous issue date: 2011-04-14 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES / Aspects of the physics of nematic liquid crystals are studied in this thesis from the viewpoint of riemannian geometry through analogue models of gravitation. The topics chosen for study were: geometric and wave optics, elastic waves, hydrodynamics and heat conduction. The main analogue model used is based on the interpretation of Fermat’s principle as a process to obtain null geodesics, where the liquid crystalline material is seen as a riemannian manifold. This approach predicts that the metric effectively felt by the light ray depends on the configuration of molecules in the liquid crystal and on the parallel and perpendicular refractive indexes to the axis of symmetry of the liquid-cristal molecule. It is known that, for the particular case of the existence of topological defects within the material, effective metric similar to cosmological defects (like global monopoles and cosmic strings) are obtained. This thesis develops itself on the situation where there are topological defects of hedgehog type and (k = 1, c = 0) disclination type in the nematic phase of the liquid crystalline material. The first problem studied, as a review, deals with the wave optics, with respect to the light diffracted by the cited defects. Since plane waves of small wavelength have identical trajectories to light rays, the use of analog model is therefore justified. Thus, we show that light scattered by these defects generates a characteristic diffraction pattern, being the location given by an algebraic expression dependent on the parallel and perpendicular refractive indexes to the axis of symmetry of the molecule. We also show how theses patterns depend on the temperature of the material. The second studied problem deals with the geometrical optics and hydrodynamics of the nematic liquid crystals. From a molecular configuration similar to a (k = 1, c = 0) disclination, we let the material flow radially towards the axis of the defect. Then, using the hydrodynamic fact that velocity gradients in the material locally change the refractive index of the molecule, we find the velocity profile that must exist around the defect so that the metric actually experienced by light traveling in the plane perpendicular to the axis the defect is the Schwarzschild one in the equatorial plane, with the Schwarzschild radius interior to the object. We found that the absolute values of the velocity of liquid crystalline fluid can be order of a few meters per second, differing greatly from the values obtained by Gordon metric for an isotropic fluid under identical conditions. The third studied problem deals with the elastic oscillations in the presence of topological defects. Similarly to the first problem, the trajectory of the sound is obtained by an elastic version of Fermat’s principle and, then, compared with a null geodesic. We show how topological defects influence the sound trajectories and the sound diffracted by them. The fourth problem deals with the heat conduction in the vicinity of defects. Considering that the defects come from an addition or removal of portion of the material, letting the medium relaxes elastically, effective metric of the space disturbed by the defect are found, with expressions similar to those obtained by the analogous model based on Fermat’s principle. These metrics generate a modified thermal conductivity tensor, allowing the study of the temperature field in this situation. We show that, depending on the values of parallel and perpendicular thermal conductivity to the axis of symmetry of the molecule and on the defect in question, the temperature gradient can be accentuated or attenuated on the defect, allowing control of the response thermal temperature of the material, according to the presence of defects. Encouraging a greater understanding of the physics of liquid crystals and its use as a background in analogue models of gravity is the main theme of each analyzed problem. / Aspectos da física dos cristais líquidos nemáticos são estudados nesta tese do ponto de vista da geometria riemannina, por meio de modelos análogos de gravitação. Os tópicos escolhidos para estudo foram: óptica geométrica e ondulatória, ondas elásticas, hidrodinâmica e condução de calor. O principal modelo análogo empregado baseia-se na interpretação do princípio de Fermat como um processo de obtenção de geodésicas nulas, onde o material líquido-cristalino é visto como sendo uma variedade riemanniana. Esta abordagem prevê que a métrica efetivamente sentida pelo raio luminoso dependa da configuração das moléculas dentro do cristal líquido e dos índices de refração paralelo e perpendicular ao eixo de simetria da molécula líquido-cristalina. É sabido que, para o caso especial da existência de defeitos topológicos dentro do material, métricas efetivas semelhantes às de defeitos cosmológicos (como monopolos globais e cordas cósmicas) são obtidas. Esta tese desenrola-se sobre a situação onde existem defeitos topológicos do tipo ouriço e do tipo desclinação (k = 1, c = 0) na fase nemática do material líquido-cristalino. O primeiro problema estudado, em caráter de revisão, trata da óptica ondulatória, no que concerne a difração de luz pelos defeitos citados. Uma vez que ondas planas de comprimento de onda pequeno possuem trajetórias idênticas aos raios luminosos, o emprego do modelo análogo é justificado. Assim, mostramos que a luz espalhada por esses defeitos gera padrões de difração bem característicos, sendo a localização dada por expressão algébrica dependente dos índices de refração paralelo e perpendicular ao eixo de simetria da molécula líquido-cristalina. Também mostramos de que forma esses padrões dependem da temperatura do material. O segundo problema estudado trata da óptica geométrica e da hidrodinâmica dos cristais líquidos nemáticos. A partir de uma configuração de moléculas semelhantes à de uma desclinação (k = 1, c = 0), permitimos que o material flua radialmente na direção do eixo do defeito. Em seguida, fazendo uso do fato hidrodinâmico de que gradientes de velocidade no material modificam localmente os índices de refração da molécula, encontramos o perfil de velocidade que deve existir em torno do defeito para que a métrica efetivamente sentida pela luz, que viaja no plano perpendicular ao eixo do defeito, seja a de Schwarzschild no plano equatorial, com raio de Schwarzschild interior ao objeto. Encontramos que os valores absolutos da velocidade de fluido líquido-cristalino podem ser da ordem de alguns metros por segundo, diferindo enormemente dos valores obtidos pela métrica de Gordon para um fluido isotrópico em condições idênticas. O terceiro problema estudado aborda as oscilações elásticas na presença de defeitos. Semelhantemente ao primeiro problema, a trajetória do som é obtida por uma versão elástica do princípio de Fermat e, então, comparada com uma geodésica nula. Mostramos como defeitos topológicos influenciam nas trajetórias sonoras, assim como no som difratado por eles. O quarto problema trata da condução de calor na vizinhança de defeitos. Considerando que os defeitos são resultantes de uma adição ou remoção de porção de material, dando-se seguimento a uma relaxação elástica do meio, métricas efetivas do espaço perturbado pelo defeito são encontradas, com expressões semelhantes às obtidas pelo modelo análogo baseado no princípio de Fermat. Essas métricas geram um tensor condutividade térmica modificado, dando cabo ao estudo do campo de temperatura nessa situação. Mostramos que, dependendo dos valores da condutividade térmica perpendicular e paralela ao eixo de simetria da molécula líquido-cristalina e do defeito em questão, o gradiente de temperatura pode ser acentuado ou atenuado sobre o defeito, permitindo o controle da resposta térmica do material à temperatura, de acordo com a presença de defeitos. Suscitar um entendimento maior da física dos cristais líquidos e de seu emprego como background em modelos análogos de gravitação é o tema principal de cada um dos problemas analisados.

A presente dissertação tem como objeto de estudo sistemas da física da matéria condensada que sejam capazes de simular sistemas gravitacionais, tais como buracos negros e universos em expansão, onde processos quânticos tomam parte. Neste estudo nos debruçamos principalmente sobre o modelo do fluido e condensados de Bose-Einstein. No modelo do fluido exploramos a geometria efetiva que surge e os problemas de back-reaction e dos modos trans-planckianos de campos quânticos. No modelo baseado em condensados exploramos sua faceta cosmológica e a possibilidade de campos maciços. Além destes dois modelos de grande relevância na literatura, ainda expomos os análogos em cordas elásticas e os baseados em ondas na superfícies de fluidos e uma análise geral baseada no formalismo lagrangeano para campos. / This dissertation has as object of study systems of condensate-matter physics which can simulate gravitational systems like black holes and expanding universes where quantum processes take place. In this study we lay attention mainly on the fluid model and on Bose-Einstein-condensate-based models. In the fluid model we explore the features of the emergent geometry and other problems like the back-reaction and the trans-planckian modes of quantum fields. In the condensate-based models we explore their cosmological aspects and the possibility for massive fields. Moreover, we shall present two other models, the elastic string and the surface-wave-based models in fluids, and a very general analysis based on the Lagrangean formalism for fields.

Submitted by isabela.moljf@hotmail.com (isabela.moljf@hotmail.com) on 2017-07-05T11:27:51Z No. of bitstreams: 1 rafaelleitefernandes.pdf: 295519 bytes, checksum: 990b7a9657e1e2be2738bb9b3dd7cf04 (MD5) / Approved for entry into archive by Adriana Oliveira (adriana.oliveira@ufjf.edu.br) on 2017-08-08T15:19:39Z (GMT) No. of bitstreams: 1 rafaelleitefernandes.pdf: 295519 bytes, checksum: 990b7a9657e1e2be2738bb9b3dd7cf04 (MD5) / Made available in DSpace on 2017-08-08T15:19:39Z (GMT). No. of bitstreams: 1 rafaelleitefernandes.pdf: 295519 bytes, checksum: 990b7a9657e1e2be2738bb9b3dd7cf04 (MD5) Previous issue date: 2013-02-27 / CAPES - Coordenação de Aperfeiçoamento de Pessoal de Nível Superior / Neste trabalho vamos mostrar que o sistema chamado de “mundo brana” para representar o nosso Universo, introduzido por Randall-Sundrum (RS) no fim dos anos noventa, pode ser na verdade representado por branas curvas no espaço de de Sitter e Anti-de Sitter. Originalmente o sistema RS representaria um Universo com cinco dimensões onde o modelo padrão ficaria confinado em uma brana e os grávitons ficariam confinados na outra brana. Este sistema foi construído com uma métrica de Minkowski “torcida” com cinco dimensões onde os grávitons, responsáveis pelo campo gravitacional no modelo padrão, se deslocariam através da quinta dimensão, que por sua vez é infinita. E a ação padrão da relatividade geral, a ação de Einstein-Hilbert, foi a utilizada por RS. Neste trabalho de dissertação de mestrado vamos adotar uma ação modificada usada atualmente para explicar efeitos cosmológicos como a energia escura e a expansão do Universo por exemplo, ou seja, a ação com uma gravitação modificada chamada de f(R). Aqui vamos usar uma f(R) totalmente generalizada e suas consequências cosmológicas e viabilidade serão analisadas. Finalmente, vamos demonstrar que as partículas do modelo padrão estão confinadas nesta brana curva. Os resultados obtidos aqui generalizam totalmente outros resultados obtidos na literatura atual sobre mundo brana com branas grossas e são por isso, originais e serão submetidos à publicação. / In this work we will show that the so-called “brane world” framework introduced by Randall-Sundrum (RS), to represent our Universe, at the late nineties can be represented in fact by bent branes in de Sitter and Anti-de Sitter space with a generalized model for gravity. At the beginning, the RS scenario represent a Universe in five dimensions where the Standard Model is confined in one brane and the gravitons were confined in the another one. This model was build with a warped Minkowski metric with five dimensions where the gravitons, which are responsible by the gravitational field, are able to move through the fifth dimension, which is infinity. The standard general relativity action, namely, the Einstein-Hilbert action, was the one used by RS. In this Master dissertation we will adopt a modified action used at present to explain some cosmological effects like dark energy and Universe expansion, for example, i.e., we will use an action with a modified gravitation called f(R). However, here we will use a generalized f(R) and their cosmological consequences and viability will be analyzed. Finally, we will show that the particles of the Standard Model are confined at this bent brane. The results obtained here generalize altogether the others results obtained in the current literature concerning braneworlds with thick branes and are, consequently, new ones, which will be published elsewhere.

L'expansion accélérée de l'univers est devenu un fait établi que personne ne pouvait prévoir il y a encore une vingtaine d'années. Pour expliquer l'accélération cosmique, l'univers doit être composé de $75%$ d'énergie noire, une matière hypothétique à pression négative. Une alternative aussi vertigineuse consiste à modifier la relativité générale d'Einstein à l'échelle cosmique.Mes travaux de thèse portent sur la contrainte des modèles d'énergie noire et de gravité modifiée avec les données observationnelles provenant de la croissance linéaire des structures cosmologiques. Une méthode basée sur une nouvelle paramétrisation de l'index de croissance des perturbations linéaires cosmologiques permet d'analyser un grand nombre de modèles "accélératoires" en même temps. Nous avons évalué et validé cette méthode par une analyse systématique de sa précision et de sa performance. Mes résultats montrent que le modèle standard de la cosmologie (le modèle $Lambda$CDM) reste en accord avec les données actuelles. Dans une étude approfondie, nous simulons les contraintes possibles avec les futures sondes cosmologiques de "précision" comme Euclid. Pour analyser encore plus de modèles en même temps, nous introduisons la théorie effective des champs de l'énergie noire (EFT) dans le formalisme développé auparavant. La EFT est un formalisme prometteur qui permet d'explorer d'une manière complète tous les modèles gravitationnels non-standards résultant de l'addition d'un degré de liberté supplémentaire dans l'équation d'Einstein. Nous proposons une paramétrisation de cette théorie que nous confrontons avec les données actuelles et futures. / The accelerated expansion of the universe has become an established fact that nobody could foresee until twenty years ago. To explain the cosmic acceleration, the universe must be composed by $75%$ of dark energy, a hypothetical form of matter with negative pressure. Alternatively, Einstein's field equation must be modified on cosmic scales. During my thesis I have worked on the constraint of dark energy and modified gravity models with data coming from the observed growth rate of cosmic structures. We have introduced a method based on a new parametrization of the growth index of linear cosmological perturbations. An advantage is the possibility of a concurrent analysis of multiple accelerating models. We have evaluated and validated the method in a systematic precision and performance check. My results show that the standard model of cosmology (the $Lambda$CDM model) remains consistent with current data. In an ongoing study, we have simulated future constraints for upcoming cosmological 'precision' probes like Euclid.In a second step, we introduce the effective field theory of dark energy (EFT) into our formalism. The EFT is a promising framework that allows to explore in a complete way all non-standard gravitational models that result from adding one degree of freedom in Einstein's field equation. Another advantage is its neat split of background and perturbation observables. We propose a parametrization of the EFT that we confront with current and simulated future constraints.

Föreliggande studie undersöker tre mellanstadielärares språkbruk både i kommunikativa metoder och planering av lektionsinnehåll. Studien utgår från två frågeställningar som behandlar hur lärarna använder och resonerar om sitt språkbruk i förhållande till kommunikativa metoder. Data samlades in genom observationer och intervjuer. I studien används legitimation code theorys semantiska vågor som teoretisk utgångspunkt och analysmetod. Lärarnas språkbruk analyseras därmed utifrån semantisk densitet och semantisk gravitation. Studiens resultat skildrar de tre deltagande lärarnas syn på vilka kommunikativa aspekter som främjar elevers lärande såsom kooperativa metoder eller relationell kommunikation. Vidare framgår även att eleverna har stor inverkan på lektionsplaneringen och de kommunikativa metoderna som lärarna tillämpar. Studien åskådliggör hur lärare motiverar elever till lärande genom att använda kommunikativa metoder som är anpassade efter deras elevgrupper. Slutligen belyser studien ytterligare utvecklingsmöjligheter och hur den kommunikativa kompetensen i skolan kan studeras ur andra perspektiv.