Results 1 to 10 of about 174,781 (254)

No short hair behaviors of ultra-compact stars

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
In the black hole spacetime, a no short hair theorem was proved, which states that the effective radius of black hole hairs must extend beyond the null circular orbit.
Yan Peng
doaj   +2 more sources

Innermost Stable Circular Orbit of a Spinning Particle in Kerr Spacetime [PDF]

open access: green, 1997
We study stability of a circular orbit of a spinning test particle in a Kerr spacetime. We find that some of the circular orbits become unstable in the direction perpendicular to the equatorial plane, although the orbits are still stable in the radial ...
A. Abromovici   +28 more
core   +4 more sources

Geometric Calibration of Parameters in the Perpendicular-Orbit Circular Scanning Satellite Camera

open access: yesRemote Sensing
Perpendicular-orbit circular scanning satellites overcome the conflict between ground resolution and width observed in traditional optical satellites by using a perpendicular-orbit circular scanning imaging method and splicing along the orbit, achieving ...
Xufeng Zhang   +3 more
doaj   +3 more sources

Design Method of Orthogonal Circular Orbit Satellite Constellation Based on Geometric Analysis [PDF]

open access: yesJisuanji gongcheng, 2020
Orthogonal circular orbit constellation combines the advantages of polar orbit constellation and equatorial orbit constellation to achieve continuous global coverage,improving the coverage performance of pure polar orbit constellation at low and middle ...
BAO Xiang, LEI Lei, SHEN Gaoqing, LI Zhilin
doaj   +1 more source

Coplanar multi-turn rendezvous in near-circular orbit using a low-thrust engine

open access: yesRUDN Journal of Engineering Research, 2022
The authors describe an algorithm that allows calculating the parameters of maneuvers performed on several turns by the low-thrust engine, which ensure the flight of the active spacecraft to the specified vicinity of the target space object. The movement
Andrey A. Baranov, Adilson Pedro Olivio
doaj   +1 more source

Methodology for creating software and mathematical support for modeling the spacecraft dynamic operations

open access: yesRUDN Journal of Engineering Research, 2021
The basis for ensuring a high level of reliability and safety in dynamic operations is a comprehensive experimental development of products in conditions as close to the real conditions of operation as possible with the use of mathematical and simulation
Veniamin V. Malyshev   +3 more
doaj   +1 more source

Orbit Decomposition Method for Rotordynamic Coefficients Identification of Annular Seals

open access: yesApplied Sciences, 2021
The elliptical orbit whirl model is widely used to identify the frequency-dependent rotordynamic coefficients of annular seals. The existing solution technique of an elliptical orbit whirl model is the transient computational fluid dynamics (CFD) method.
Mingjie Zhang   +3 more
doaj   +1 more source

Lyapunov exponent, ISCO and Kolmogorov–Senai entropy for Kerr–Kiselev black hole

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
Geodesic motion has significant characteristics of space-time. We calculate the principle Lyapunov exponent (LE), which is the inverse of the instability timescale associated with this geodesics and Kolmogorov–Senai (KS) entropy for our rotating Kerr ...
Monimala Mondal   +2 more
doaj   +1 more source

Bound on Photon Circular Orbits in General Relativity and Beyond

open access: yesGalaxies, 2021
The existence of a photon circular orbit can tell us a lot about the nature of the underlying spacetime, since it plays a pivotal role in the understanding of the characteristic signatures of compact objects, namely the quasi-normal modes and shadow ...
Sumanta Chakraborty
doaj   +1 more source

To Circularize or Not To Circularize?—Orbital Evolution of Satellite Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2003
We investigated the orbital evolution of satellite galaxies using numerical simulations. It has been long believed that the orbit suffers circularization due to the dynamical friction from the galactic halo during orbital decay. This circularization was confirmed by numerous simulations where dynamical friction is added as external force. However, some
Hashimoto, Yoshikazu   +2 more
openaire   +2 more sources

Home - About - Disclaimer - Privacy