Current gravitational wave (GW) detections rely on the existence of libraries of theoretical waveforms. Consequently, finding new physics with GWs requires libraries of nonstandard models, which are computationally de...
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Current gravitational wave (GW) detections rely on the existence of libraries of theoretical waveforms. Consequently, finding new physics with GWs requires libraries of nonstandard models, which are computationally demanding. We discuss how deep learning frameworks can be used to generate new waveforms “learned” from a simulation dataset obtained, say, from numerical relativity simulations. Concretely, we use the WaveGAN architecture of a generative adversarial network (GAN). As a proof of concept we provide this neural network (NN) with a sample of (>500) waveforms from the collisions of exotic compact objects (Proca stars), obtained from numerical relativity simulations. Dividing the sample into a training and a validation set, we show that after a sufficiently large number of training epochs the NN can produce from 12% to 25% of the synthetic waveforms with an overlapping match of at least 95% with the ones from the validation set. We also demonstrate that a NN can be used to predict the overlapping match score, with 90% accuracy, of new synthetic samples. These are encouraging results for using GANs for data augmentation and interpolation in the context of GWs, to cover the full parameter space of, say, exotic compact binaries, without the need for intensive numerical relativity simulations.
We investigate quasitopological black holes in (2+1) dimensions in the context of electromagnetic-generalized-quasitopological gravities (EM-GQT). For three different families of geometries of quasitopological nature,...
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We investigate quasitopological black holes in (2+1) dimensions in the context of electromagnetic-generalized-quasitopological gravities (EM-GQT). For three different families of geometries of quasitopological nature, we study the causal structure and their response to a probe scalar field. To linear order, we verify that the scalar field evolves stably, decaying in different towers of quasinormal modes. The studied black holes are either charged geometries (regular and singular) or a regular Bañados-Teitelboim-Zanelli (BTZ)-like black hole, both coming from the EM-GQT theory characterized by nonminimal coupling parameters between gravity and a background scalar field. We calculate the quasinormal modes applying different numerical methods with convergent results between them. The oscillations demonstrate a very peculiar structure for charged black holes: in the intermediate and near extremal cases, a particular scaling arises, similar to that of the rotating BTZ geometry, with the modes being proportional to the distance between horizons. For the single horizon black hole solution, we identify the presence of different quasinormal families by analyzing the features of that spectrum. In all three considered geometries, no instabilities were found.
Marketing is an area that has always been updated over time, considering it fundamental to adapt to the changes and evolution of the market and consumers. Consequently, the enlargement of marketing to new areas has be...
Marketing is an area that has always been updated over time, considering it fundamental to adapt to the changes and evolution of the market and consumers. Consequently, the enlargement of marketing to new areas has been a growing reality. Based on this reality and within the scope of Religious Marketing, a study was carried out for the Parish of Poiares, in Portugal. The general objective was to characterize the profile of the parishioners, with the intention of subsequently defining strategies and implementing religious marketing tactics in the context of the parish of Poiares. To this end, an empirical work of qualitative nature was carried out, through the application of a questionnaire survey to a non-probabilistic convenience sample of 120 individuals. This empirical work had as its main objectives to understand the level of spirituality/involvement of the parishioners and the factors that register their greater or lesser satisfaction.
The optimization of cognitive radio(CR)system using an enhanced firefly algorithm(EFA)is presented in this *** Firefly algorithm(FA)is a nature-inspired algorithm based on the unique light-flashing behavior of *** has...
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The optimization of cognitive radio(CR)system using an enhanced firefly algorithm(EFA)is presented in this *** Firefly algorithm(FA)is a nature-inspired algorithm based on the unique light-flashing behavior of *** has already proved its competence in various optimization prob-lems,but it suffers from slow convergence *** improve the convergence performance of FA,a new variant named EFA is *** effectiveness of EFA as a good optimizer is demonstrated by optimizing benchmark functions,and simulation results show its superior performance compared to biogeography-based optimization(BBO),bat algorithm,artificial bee colony,and *** an application of this algorithm to real-world problems,EFA is also applied to optimize the CR *** is a revolutionary technique that uses a dynamic spectrum allocation strategy to solve the spectrum scarcity ***,it requires optimization to meet specific performance *** results obtained by EFA in CR system optimization are compared with results in the literature of BBO,simulated annealing,and genetic *** results further prove that the proposed algorithm is highly efficient and provides superior results.
作者:
Jorge F. M. DelgadoDepartamento de Matemática
Universidade de Aveiro Center for Research and Development in Mathematics and Applications-CIDMA Campus de Santiago Aveiro 3810-183 Portugal Centro de Astrofísica e Gravitação-CENTRA
Departamento de Física Instituto Superior Técnico-IST Universidade de Lisboa-UL Av. Rovisco Pais 1 Lisboa 1049-001 Portugal
Recently, it has been shown that the radial stability of a light ring (LR) in a spacetime generated by a stationary, axisymmetric, asymptotically flat object with a Z2 symmetry determines the possibility and radial st...
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Recently, it has been shown that the radial stability of a light ring (LR) in a spacetime generated by a stationary, axisymmetric, asymptotically flat object with a Z2 symmetry determines the possibility and radial stability of timelike circular orbits (TCOs) around the LR. In this paper, we generalize this result by also considering the vertical (angular) stability of the orbits through the study of the radial and vertical epicyclic frequencies. We show that the vertical stability of the LR only determines the vertical stability of the TCOs around it. A relation between the sum of the squared epicyclic frequencies and the Ricci tensor is also provided. With such relation, we show that objects with radially and vertically unstable LRs (TCOs) violate the null (strong) energy condition.
In this paper we present the groundwork for an Itô/Malliavin stochastic calculus and Hida's white noise analysis in the context of a supersymmentry with Z3-graded algebras. To this end we establish a ternary ...
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We construct and dynamically evolve dipolar self-interacting scalar boson stars in a model with sextic (+ quartic) self-interactions. The domain of existence of such dipolar Q-stars has a similar structure to that of ...
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We construct and dynamically evolve dipolar self-interacting scalar boson stars in a model with sextic (+ quartic) self-interactions. The domain of existence of such dipolar Q-stars has a similar structure to that of the fundamental monopolar stars of the same model. For the latter it is structured in a Newtonian plus a relativistic branch, wherein perturbatively stable solutions exist, connected by a middle unstable branch. Our evolutions support similar dynamical properties of the dipolar Q-stars that: 1) in the Newtonian and relativistic branches are dynamically robust over time scales longer than those for which dipolar stars without self-interactions are seen to decay; 2) in the middle branch migrate to either the Newtonian or the relativistic branch; 3) beyond the relativistic branch decay to black holes. Overall, these results strengthen the observation, seen in other contexts, that self-interactions can mitigate dynamical instabilities of scalar boson star models.
A convolutional code C over Zpr[D] is a Zpr[D]-submodule of Znpr[D] where Zpr[D] stands for the ring of polynomials with coefficients in Zpr. In this paper we study the list decoding problem of these codes when the tr...
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One of the most important tools used in companies is visual communication. A logo is part of a brand entity and therefore, a way to communicate their values or mission. This work aims to verify whether the different c...
One of the most important tools used in companies is visual communication. A logo is part of a brand entity and therefore, a way to communicate their values or mission. This work aims to verify whether the different colors used in the logo can awaken differentiated emotions in consumers. A questionnaire was prepared with the Facebook logo, varying in color. Through the obtained data, it was possible to conclude that color is a key element of a logo. When a new or reformulated logo is performed, companies should be aware that color could influence consumer perception.
We show that certain vanishing properties defining closed subspaces of generalized Morrey spaces are preserved under the action of various classical operators of harmonic analysis, such as maximal operators, singular-...
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