Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Miguel Preto"'
Publikováno v:
Energies, Vol 17, Iss 12, p 2987 (2024)
Incorporating renewables in the power grid presents challenges for stability, reliability, and operational efficiency. Integrating energy storage systems (ESSs) offers a solution by managing unpredictable loads, enhancing reliability, and serving the
Externí odkaz:
https://doaj.org/article/ae32745bf3714762a2eafb7dbed79756
Autor:
Nuno Miguel Preto Gomes, Pedro Matos, Patricia Pereira Amoedo, Andre Cerejeira, Luis Lemos, Maria Joao Cruz, Paulo Santos, Filomena Azevedo
Publikováno v:
Indian Journal of Dermatology, Vol 67, Iss 4, Pp 458-459 (2022)
Externí odkaz:
https://doaj.org/article/d028d3ed9663495d9388a4e38393a8ce
Publikováno v:
Administrative Sciences
Volume 13
Issue 2
Pages: 34
Volume 13
Issue 2
Pages: 34
The aim of this study is to test the multidimensional construct of the Entrepreneurial University (EU), and therefore to confirm whether EU factors make a positive contribution to regional competitiveness. Data were collected from ten Portuguese Publ
Autor:
Marcos, Pedro Miguel Preto
Economia e Gestão Internacional
Master in International Business
Master in International Business
Externí odkaz:
http://hdl.handle.net/10216/52229
Publikováno v:
The Astrophysical Journal. 695:455-468
This paper studies the formation and evolution of binary supermassive black holes (SMBHs) in rotating galactic nuclei, focusing on the role of stellar dynamics. We present the first N-body simulations that follow the evolution of the SMBHs from kilop
Publikováno v:
The Astrophysical Journal. 613:L109-L112
We present a clear N-body realization of the growth of a Bahcall-Wolf f ~ E^0.25 (rho ~ 1/r^1.75) density cusp around a massive object ("black hole") at the center of a stellar system. Our N-body algorithm incorporates a novel implementation of Mikko
Autor:
Scott Tremaine, Miguel Preto
Publikováno v:
The Astronomical Journal. 118:2532-2541
Symplectic integration algorithms are well-suited for long-term integrations of Hamiltonian systems because they preserve the geometric structure of the Hamiltonian flow. However, this desirable property is generally lost when adaptive timestep contr
Hierarchy of models: From qualitative to quantitative analysis of circadian rhythms in cyanobacteria
Autor:
Madalena Chaves, Miguel Preto
Publikováno v:
Chaos: An Interdisciplinary Journal of Nonlinear Science
Chaos: An Interdisciplinary Journal of Nonlinear Science, AIP, 2013, 23 (2), pp.025113. ⟨10.1063/1.4810922⟩
Chaos: An Interdisciplinary Journal of Nonlinear Science, American Institute of Physics, 2013, 23 (2), pp.025113. ⟨10.1063/1.4810922⟩
Chaos: An Interdisciplinary Journal of Nonlinear Science, 2013, 23 (2), pp.025113. ⟨10.1063/1.4810922⟩
Chaos: An Interdisciplinary Journal of Nonlinear Science, AIP, 2013, 23 (2), pp.025113. ⟨10.1063/1.4810922⟩
Chaos: An Interdisciplinary Journal of Nonlinear Science, American Institute of Physics, 2013, 23 (2), pp.025113. ⟨10.1063/1.4810922⟩
Chaos: An Interdisciplinary Journal of Nonlinear Science, 2013, 23 (2), pp.025113. ⟨10.1063/1.4810922⟩
International audience; A hierarchy of models, ranging from high to lower levels of abstraction, is proposed to construct "minimal" but predictive and explanatory models of biological systems. Three hierarchical levels will be considered: Boolean net
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eed05e34158a1a849958d821747b9612
https://hal.inria.fr/hal-00850373/file/chaves-preto-chaos2013.pdf
https://hal.inria.fr/hal-00850373/file/chaves-preto-chaos2013.pdf
Autor:
Miguel Preto, Pau Amaro-Seoane
Publikováno v:
Classical and Quantum Gravity
Classical and Quantum Gravity, IOP Publishing, 2011, 28 (9), pp.94017. ⟨10.1088/0264-9381/28/9/094017⟩
Classical and quantum gravity
Classical and Quantum Gravity, IOP Publishing, 2011, 28 (9), pp.94017. ⟨10.1088/0264-9381/28/9/094017⟩
Classical and quantum gravity
One of the most interesting sources of gravitational waves (GWs) for LISA is the inspiral of compact objects on to a massive black hole (MBH), commonly referred to as an "extreme-mass ratio inspiral" (EMRI). The small object, typically a stellar blac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11f9dcbf116ffff4129dc77b062d9ea6
https://hal.archives-ouvertes.fr/hal-00694883
https://hal.archives-ouvertes.fr/hal-00694883