964 resultados para Einstein-Elevator


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We propose a very long baseline atom interferometer test of Einstein's equivalence principle (EEP) with ytterbium and rubidium extending over 10m of free fall. In view of existing parametrizations of EEP violations, this choice of test masses significantly broadens the scope of atom interferometric EEP tests with respect to other performed or proposed tests by comparing two elements with high atomic numbfers. In the first step, our experimental scheme will allow us to reach an accuracy in the Eotvos ratio of 7 . 10(-13). This achievement will constrain violation scenarios beyond our present knowledge and will represent an important milestone for exploring a variety of schemes for further improvements of the tests as outlined in the paper. We will discuss the technical realisation in the new infrastructure of the Hanover Institute of Technology (HITec) and give a short overview of the requirements needed to reach this accuracy. The experiment will demonstrate a variety of techniques, which will be employed in future tests of EEP, high-accuracy gravimetry and gravity gradiometry. It includes operation of a force-sensitive atom interferometer with an alkaline earth-like element in free fall, beam splitting over macroscopic distances and novel source concepts.

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This project, realized at the company ABER Ltd, describes the process followed for the developing of an electronic control system for a hydraulic elevator. The previous control system was based on relay logic, and the company wanted to change it to a microcontroller based technology. To do so, different approaches were studied and finally the selected technology for the development was the Raspberry Pi. After, the software needed for all the elevator types was developed, and the interface hardware was selected. In the end, several test were made to adjust the software and the hardware and to prove the good operation of the system.

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The second generation of large scale interferometric gravitational wave (GW) detectors will be limited by quantum noise over a wide frequency range in their detection band. Further sensitivity improvements for future upgrades or new detectors beyond the second generation motivate the development of measurement schemes to mitigate the impact of quantum noise in these instruments. Two strands of development are being pursued to reach this goal, focusing both on modifications of the well-established Michelson detector configuration and development of different detector topologies. In this paper, we present the design of the world's first Sagnac speed meter (SSM) interferometer, which is currently being constructed at the University of Glasgow. With this proof-of-principle experiment we aim to demonstrate the theoretically predicted lower quantum noise in a Sagnac interferometer compared to an equivalent Michelson interferometer, to qualify SSM for further research towards an implementation in a future generation large scale GW detector, such as the planned Einstein telescope observatory.

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We report the suitability of an Einstein-Podolsky-Rosen entanglement source for Gaussian continuous-variable quantum key distribution at 1550 nm. Our source is based on a single continuous-wave squeezed vacuum mode combined with a vacuum mode at a balanced beam splitter. Extending a recent security proof, we characterize the source by quantifying the extractable length of a composable secure key from a finite number of samples under the assumption of collective attacks. We show that distances in the order of 10 km are achievable with this source for a reasonable sample size despite the fact that the entanglement was generated including a vacuum mode. Our security analysis applies to all states having an asymmetry in the field quadrature variances, including those generated by superposition of two squeezed modes with different squeezing strengths.

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Dissertação (mestrado)—Universidade de Brasília, Faculdade de Tecnologia, Departamento de Engenharia Mecânica, 2015.

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In many instances of holographic correspondences between a d-dimensional boundary theory and a (. d+. 1)-dimensional bulk, a direct argument in the boundary theory implies that there must exist a simple and precise relation between the Euclidean on-shell action of a (. d-. 1)-brane probing the bulk geometry and the Euclidean gravitational bulk action. This relation is crucial for the consistency of holography, yet it is non-trivial from the bulk perspective. In particular, we show that it relies on a nice isoperimetric inequality that must be satisfied in a large class of Poincaré-Einstein spaces. Remarkably, this inequality follows from theorems by Lee and Wang.

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Simplifying the Einstein field equation by assuming the cosmological principle yields a set of differential equations which governs the dynamics of the universe as described in the cosmological standard model. The cosmological principle assumes the space appears the same everywhere and in every direction and moreover, the principle has earned its position as a fundamental assumption in cosmology by being compatible with the observations of the 20th century. It was not until the current century when observations in cosmological scales showed significant deviation from isotropy and homogeneity implying the violation of the principle. Among these observations are the inconsistency between local and non-local Hubble parameter evaluations, baryon acoustic features of the Lyman-α forest and the anomalies of the cosmic microwave background radiation. As a consequence, cosmological models beyond the cosmological principle have been studied vastly; after all, the principle is a hypothesis and as such should frequently be tested as any other assumption in physics. In this thesis, the effects of inhomogeneity and anisotropy, arising as a consequence of discarding the cosmological principle, is investigated. The geometry and matter content of the universe becomes more cumbersome and the resulting effects on the Einstein field equation is introduced. The cosmological standard model and its issues, both fundamental and observational are presented. Particular interest is given to the local Hubble parameter, supernova explosion, baryon acoustic oscillation, and cosmic microwave background observations and the cosmological constant problems. Explored and proposed resolutions emerging by violating the cosmological principle are reviewed. This thesis is concluded by a summary and outlook of the included research papers.

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Experiments with ultracold atoms in optical lattice have become a versatile testing ground to study diverse quantum many-body Hamiltonians. A single-band Bose-Hubbard (BH) Hamiltonian was first proposed to describe these systems in 1998 and its associated quantum phase-transition was subsequently observed in 2002. Over the years, there has been a rapid progress in experimental realizations of more complex lattice geometries, leading to more exotic BH Hamiltonians with contributions from excited bands, and modified tunneling and interaction energies. There has also been interesting theoretical insights and experimental studies on “un- conventional” Bose-Einstein condensates in optical lattices and predictions of rich orbital physics in higher bands. In this thesis, I present our results on several multi- band BH models and emergent quantum phenomena. In particular, I study optical lattices with two local minima per unit cell and show that the low energy states of a multi-band BH Hamiltonian with only pairwise interactions is equivalent to an effec- tive single-band Hamiltonian with strong three-body interactions. I also propose a second method to create three-body interactions in ultracold gases of bosonic atoms in a optical lattice. In this case, this is achieved by a careful cancellation of two contributions in the pair-wise interaction between the atoms, one proportional to the zero-energy scattering length and a second proportional to the effective range. I subsequently study the physics of Bose-Einstein condensation in the second band of a double-well 2D lattice and show that the collision aided decay rate of the con- densate to the ground band is smaller than the tunneling rate between neighboring unit cells. Finally, I propose a numerical method using the discrete variable repre- sentation for constructing real-valued Wannier functions localized in a unit cell for optical lattices. The developed numerical method is general and can be applied to a wide array of optical lattice geometries in one, two or three dimensions.

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We describe the construction and characterization of a new apparatus that can produce degenerate quantum gases of strontium. The realization of degenerate gases is an important first step toward future studies of quantum magnetism. Three of the four stable isotopes of strontium have been cooled into the degenerate regime. The experiment can make nearly pure Bose-Einstein condensates containing approximately 1x10^4 atoms, for strontium-86, and approximately 4x10^5 atoms, for strontium-84. We have also created degenerate Fermi gases of strontium-87 with a reduced temperature, T/T_F of approximately 0.2. The apparatus will be able to produce Bose-Einstein condensates of strontium-88 with straightforward modifications. We also report the first experimental and theoretical results from the strontium project. We have developed a technique to accelerate the continuous loading of strontium atoms into a magnetic trap. By applying a laser addressing the 3P1 to 3S1 transition in our magneto-optical trap, the rate at which atoms populate the magnetically-trapped 3P2 state can be increased by up to 65%. Quantum degenerate gases of atoms in the metastable 3P0 and 3P2 states are a promising platform for quantum simulation of systems with long-range interactions. We have performed an initial numerical study of a method to transfer the ground state degenerate gases that we can currently produce into one of the metastable states via a three-photon transition. Numerical simulations of the Optical Bloch equations governing the three-photon transition indicate that >90% of a ground state degenerate gas can be transferred into a metastable state.

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La teoría de Einstein del campo gravitacional conocida como Relatividad General predice la existencia de ondas gravitacionales

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Dissertação de mest. em Física - área de especialização em Física para Ensino, Faculdade de Ciências e Tecnologia, Univ. do Algarve, 2003

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In questa tesi si introduce il concetto di buco nero acustico come l’analogo sonoro di ciò che rappresenta un buco nero in relatività generale. In primo luogo verrà quindi illustrata la teoria della gravitazione di Einstein, per poi entrare nel dettaglio della soluzione di Schwarzschild e della nozione di buco nero. In secondo luogo si dimostrerà come alcuni sistemi, i fluidi disomogenei in movimento, riescano a riprodurre effetti gravitazionali sotto certe condizioni. In particolare si osserverà come il suono che si propaga in questi fluidi lo faccia lungo delle geodetiche determinate da una "metrica acustica" dipendente da velocità e densità del fluido, che verrà ricavata. Ciò che permetterà di stabilire l’analogia sarà un’estensione analitica della soluzione di Schwarzschild, quella di Painlevé-Gullstrand: si potrà infatti identificare (formalmente) l’elemento di linea acustico con l’elemento di linea di Painlevé-Gullstrand. Si troverà che portando la velocità del fluido a una velocità maggiore di quella del suono, nella zona supersonica le onde acustiche non potranno propagarsi controcorrente ma verranno trascinate nella direzione opposta, come i raggi luminosi vengono trascinati verso la singolarità all’interno dell’orizzonte degli eventi di un buco nero. La zona supersonica verrà quindi chiamata buco nero acustico.

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The following text is a business plan for SurfScholar - an advising service to attract international students to get entire academic degrees in Portugal’s most dynamic Surf-City: Lisbon. SurfScholar is presented as a viable business concept with environmental, economic and socio-cultural sustainability as guiding principles. For a variety of reasons, Lisbon is becoming an increasingly popular destination for international student mobility. Additionally, Lisbon and its surrounding coastal areas have been experiencing a recent boom in surf related tourism. The text goes into detail about how SurfScholar combines educational tourism and surf tourism by promoting Lisbon as the perfect destination to be both an international student and a surf tourist. To test the market interest in this concept, a simple website was created with a call-toaction. With minimal marketing, SurfScholar received a robust amount of interest from people around the world. SurfScholar’s mission to is to be at the forefront of linking educational tourism and surf tourism and to explore Portugal’s potential as the premier global destination for this new niche segment of tourism. SurfScholar’s business plan is formatted in accordance with the United States Agency for International Development’s, Sustainable Tourism Enterprise Development: A Business Planning Approach, (Humke & Hilbrunner, n.d).

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El presente estudio de corte descriptivo hace una revisión teórica de 68 artículos de 11 países de Latinoamérica con el fin de dar a conocer el panorama organizacional con relación a la cultura organizacional y el liderazgo en la región y cómo este ha ido evolucionando en el tiempo. La metodología utilizada se enfocó en un conteo de frecuencias usando el modelo de liderazgo y cultura organizacional de Bass y Avolio (Bass, 1999) permitiendo ordenar en tres estilos de liderazgo la información encontrada en la revisión teórica, y a su vez cada uno de los liderazgos con sus creencias, éstas tomadas como variables de la cultura organizacional. Finalmente se encontraron diferentes tipos de tendencias a nivel de los tipos de liderazgo implementados en las organizaciones y la cultura organizacional que se adopta. Se plantea la necesidad de profundizar más y de forma empírica en la temática planteada para que se conozcan las transformaciones que se han dado en el contexto organizacional y el impacto sea mayor en un futuro cercano.