Gotowe bibliografie tematyczne / Galilean 4-space

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Gotowa bibliografia na temat „Galilean 4-space”

Autor: Grafiati

Data publikacji: 3 czerwca 2025

Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Galilean 4-space"

Yılmaz, Süha, and Yasin Unluturk. "On spherical indicatrices of curves in Galilean 4-space G₄." Journal of the Indonesian Mathematical Society 25, no. 2 (2019): 154–70. http://dx.doi.org/10.22342/jims.25.2.473.154-170.

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In this study, we indroduce spherical indicatrices of curves in four dimensional Galilean space. Moreover, we characterize these curves in terms of Frenet-Serret vector fields in four dimensional Galilean space. Frenet-Serret apparatus of these curves are obtained in terms of base curve's Frenet invariants. Additionally, some theorems are given regarding characterizations of spherical indicatrices of curves in four dimensional Galilean space.

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Öztekin, Handan. "Special Bertrand Curves in 4D Galilean Space." Mathematical Problems in Engineering 2014 (2014): 1–7. http://dx.doi.org/10.1155/2014/318458.

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The generalization of Bertrand curves in Galilean 4-space is introduced and the characterization of the generalized Bertrand curves is obtained. Furthermore, it is proved that no special curve is a classical Bertrand curve in Galilean 4-space such that the notion of classical Bertrand curve is definite only in three-dimensional spaces.

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Gün Bozok, Hülya, Sezin Aykurt Sepet, and Mahmut Ergüt. "Motions of Curves in 4-Dimensional Galilean Space G4." Asian-European Journal of Mathematics 14, no. 09 (2021): 2150153. http://dx.doi.org/10.1142/s1793557121501539.

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In this paper, we investigate the flow of curve and its equiform geometry in 4-dimensional Galilean space. We obtain that the Frenet equations and curvatures of inextensible flows of curves and its equiformly invariant vector fields and intrinsic quantities are independent of time. We find that the motions of curves and its equiform geometry can be defined by the inviscid and stochastic Burgers’ equations in 4-dimensional Galilean space.

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Lieske, J. H. "Galilean Satellites and the Galileo Space Mission." International Astronomical Union Colloquium 165 (1997): 13–20. http://dx.doi.org/10.1017/s0252921100046327.

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AbstractThe Galileo spacecraft arrived at Jupiter in December 1995 to start its two-year mission of exploring the Jovian system. The spacecraft will complete eleven orbits around Jupiter and have ten more close encounters with the outer three Galilean satellites, after the initial close approach to Io on December 7, 1995. Since the Io encounter occurred closer to Io than originally designed, the spacecraft energy change was greater than nominally planned and resulted in an initial spacecraft orbital period about 7 days less than that designed in the nominal tour. A 100-km change in the Io-enco

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Yoon, Dae Won. "On the inclined curves in Galilean 4-space." Applied Mathematical Sciences 7 (2013): 2193–99. http://dx.doi.org/10.12988/ams.2013.13196.

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Elzawy, M., and S. Mosa. "Smarandache curves in the Galilean 4-space G4." Journal of the Egyptian Mathematical Society 25, no. 1 (2017): 53–56. http://dx.doi.org/10.1016/j.joems.2016.04.008.

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Korkmaz, Fatma Bulut, and Mehmet Bektaandş. "Second Binormal Motions of Inextensible Curves in 4-dimensional Galilean Space." Applied Mathematics and Nonlinear Sciences 5, no. 1 (2020): 249–54. http://dx.doi.org/10.2478/amns.2020.1.00022.

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AbstractIn our study, we give the associated evolution equations for curvature and torsion as a system of partial differential equations. In addition, we study second binormal motions of inextensible curves in 4-dimensional Galilean space.

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OTHMAN, A. A., M. DE MONTIGNY, and F. C. KHANNA. "GALILEAN COVARIANT DIRAC EQUATION WITH A WOODS–SAXON POTENTIAL." International Journal of Modern Physics E 22, no. 12 (2013): 1350092. http://dx.doi.org/10.1142/s0218301313500924.

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We derive and solve the Galilean covariant Dirac equation, also called "Lévy-Leblond equation", for spin-½ particles in a Woods–Saxon potential. We obtain this wave equation with a Galilean covariant approach, which is based on a (4+1)-dimensional manifold with light-cone coordinates followed by a reduction to the (3+1)-dimensional Galilean space-time. We apply the Pekeris approximation and exploit the Nikiforov–Uvarov method to find the energy eigenvalues and eigenfunctions.

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ALTIN, Mustafa, Ahmet KAZAN, and Hacı Bayram KARADAĞ. "Hypersurface families with Smarandache curves in Galilean 4-space." Communications Faculty Of Science University of Ankara Series A1Mathematics and Statistics 70, no. 2 (2021): 744–61. http://dx.doi.org/10.31801/cfsuasmas.794779.

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PAVLOTSKY, I. P., and M. STRIANESE. "IRREVERSIBILITY IN CLASSICAL MECHANICS AS A CONSEQUENCE OF POINCARÉ GROUP." International Journal of Modern Physics B 10, no. 21 (1996): 2675–85. http://dx.doi.org/10.1142/s0217979296001185.

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In the post-Galilean approximation of Poincaré Group (i.e. in the approximation in which the corrections of order O (c−2), c denoting the light velocity, to the Galilei group are taken in account) the Lagrangians are singular on a submanifold of the phase space. It is a local singularity, which differs from the ones considered by Dirac. The dynamical properties are essentially peculiar on the studied singular surfaces.1–4 In particular, on some submanifolds of the singular manifold the velocities are not determined uniquely: in each point of the submanifold we get the infinite set of component

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Części książek na temat "Galilean 4-space"

Pearle, Philip. "Supplement to Chapter 4." In Introduction to Dynamical Wave Function Collapse. Oxford University PressOxford, 2024. http://dx.doi.org/10.1093/oso/9780198901372.003.0011.

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Abstract This chapter supplements Chapter 4. It introduces the quantum field operators that create and annihilate a particle at a particular position. These quantum field operators are useful in calculating here the universal mean energy increase of any object. This completes the calculation started in Chapter 4, where the results obtained here are utilized. Next, Galilean-invariance of non-relativistic CSL is proved, that is, time-translation invariance, space-translation invariance and boost-invariance.

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Streszczenia konferencji na temat "Galilean 4-space"

Meyssignac, Benoit, Maria Hakuba, Tim Boyer, and Jérôme Benveniste. "First Earth Energy Imbalance Assessment WCRP-ESA Workshop Summary and Recommendations Executive Brief." In First Earth Energy Imbalance Assessment WCRP-ESA Workshop. ESA, 2023. http://dx.doi.org/10.5270/wcrp-esa-eeia-2023.final_report_brief.

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The first edition of the Earth Energy Imbalance Assessment Workshop series was organized by the European Space Agency (ESA) with the support from CNES and 4 others institutions, and took place on 15 to 17 May 2023 at ESA-ESRIN in Frascati (Italy). The workshop brought together 61 scientists from 14 countries. The workshop engaged a wide community with expertise in radiometric remote sensing, satellite altimetry, space gravimetry, ocean in situ measurements and ocean reanalysis to assess and intercompare estimates of Earth's energy imbalance and their time variability and uncertainties. This do

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Wiedermann, Georg, Tobias Rudolph, Marianna Vitelli, Stefan Winkler, and Razvan Luzi. "The MetOp-SG Satellite Attitude Control System - Challenges and Solutions." In ESA 12th International Conference on Guidance Navigation and Control and 9th International Conference on Astrodynamics Tools and Techniques. ESA, 2023. http://dx.doi.org/10.5270/esa-gnc-icatt-2023-033.

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Mission and Program Overview MetOp-SG is a European polar satellite system consisting of a constellation of two complementary satellites (SAT-A and SAT-B). The purpose of the mission is to provide observations and measurements for numerical weather prediction and climate monitoring, based on a total of ten instruments flown across the two satellites. MetOp-SG is the follow-on system to the first generation series of MetOp satellites, which currently provide operational meteorological observations from polar orbit. MetOp-SG is a collaborative programme between ESA and EUMETSAT with a total of s

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