Results 71 to 80 of about 17,955,789 (263)

Jovian Trojan N-Body Simulations

open access: yes
The Jovian Trojans are two swarms of asteroids, one ahead and one behind the orbit of Jupiter. These data are simulations of these objects over the 4.5 gya of the the solar system.
Holton, Timothy A.
core   +1 more source

Self‐Regulated Learning Meets AI: Reinterpreting Self‐Regulation, Co‐Regulation, and Socially Shared Regulation in Human–AI Interaction

open access: yesNew Directions for Adult and Continuing Education, EarlyView.
ABSTRACT Advancing artificial intelligence (AI) has transformed learning and work, yet higher education and professional development programs have not systematically equipped learners for AI‐prevalent environments. This lack of preparation creates uncertainty regarding control, responsibility, trust, and accountability.
Moon‐Heum Cho, Jerusalem Merkebu
wiley   +1 more source

N-body simulations of close encounters between open star clusters

open access: yesAstronomy & Astrophysics
Context. In the Milky Way, close encounters between open clusters (OCs) of non-common origin are not rare. However, the dynamical processes governing close encounters between OCs remain poorly understood and may differ significantly from those observed ...
Zhu Zhanpeng, Li Zhongmu, Zhang Shaohua
doaj   +1 more source

Predictive Ability of Plasma p‐tau217 for β‐Amyloid Status: A Prospective Multicenter Study

open access: yesAnnals of Clinical and Translational Neurology, EarlyView.
ABSTRACT Objective Plasma tau phosphorylated at threonine 217 (p‐tau217) measured with fully automated platforms has shown high accuracy for Alzheimer's disease (AD) diagnosis, but real‐world multicenter data remain limited. We aimed to validate the diagnostic performance of p‐tau217 for identifying AD pathology in a real‐world multicenter cohort ...
Miquel Massons   +33 more
wiley   +1 more source

Detecting irregular orbits in gravitational N-body simulations [PDF]

open access: yes, 2008
We present a qualitative diagnostic based on the continuous wavelet transform, for the detection of irregular behaviour in time series of particle simulations. We apply the method to three qualitatively different gravitational 3-body encounters.
Kruip, C.J.H.   +5 more
core   +1 more source

Comparing the Effect of Semi‐Immersive Virtual Reality, Computerized Cognitive Training, and Traditional Rehabilitation on Cognitive Function in Multiple Sclerosis: A Randomized Clinical Trial

open access: yesAnnals of Clinical and Translational Neurology, EarlyView.
ABSTRACT Background Cognitive impairment is a common non‐motor symptom in Multiple Sclerosis (MS), negatively affecting autonomy and Quality of Life (QoL). Innovative rehabilitation strategies, such as semi‐immersive virtual reality (VR) and computerized cognitive training (CCT), may offer advantages over traditional cognitive rehabilitation (TCR ...
Maria Grazia Maggio   +8 more
wiley   +1 more source

Dark matter with n-body numerical simulations

open access: yesRevista Mexicana de Física E, 2020
The development of numerical N-body simulations have allowed studying the formation process and evolution of galaxies at different scales. This paper presents the fundamental concepts of N-body systems applied to the cosmological evolution of the ¤-Cold Dark Matter (¤CDM) model. To perform structure formation in the Universe, we provide an introduction
Chacon, Jazhiel   +2 more
openaire   +3 more sources

Comments on the size of the simulation box in cosmological N-body simulations [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2005
N-Body simulations are a very important tool in the study of formation of large scale structures. Much of the progress in understanding the physics of high redshift universe and comparison with observations would not have been possible without N-Body simulations.
Bagla, J. S., Ray, Suryadeep
openaire   +2 more sources

Orbital Stability and Secular Dynamics of the Proxima Centauri Planetary System

open access: yesThe Astrophysical Journal
The two innermost planets of the Proxima Centauri system are separated by just 0.02 au, inducing strong gravitational interactions between them. We assess this interaction by leveraging fast orbital stability indicators and find that orbital stability is
Joseph R. Livesey   +2 more
doaj   +1 more source

Multimass schemes for collisionless N-body simulations [PDF]

open access: yes, 2008
We present a general scheme for constructing Monte Carlo realizations of equilibrium, collisionless galaxy models with known distribution function (DF) f 0.
Mimi Zhang, John Magorrian
core   +1 more source

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