Results 41 to 50 of about 1,482,374 (348)
Analytical performance modelling of adaptive wormhole routing in the star interconnection network [PDF]
The star graph was introduced as an attractive alternative to the well-known hypercube and its properties have been well studied in the past. Most of these studies have focused on topological properties and algorithmic aspects of this network.
Kiasari, A.E. +2 more
core +1 more source
Predictions for neutron stars from holographic nuclear matter
We discuss masses, radii, and tidal deformabilities of neutron stars constructed from the holographic Witten-Sakai-Sugimoto model. Using the same model for crust and core of the star, we combine our theoretical results with the latest astrophysical ...
Nicolas Kovensky, Aaron Poole, Andreas Schmitt
doaj +1 more source
To appear in the proceedings of Conference C12-08 ...
Dexheimer, V., Schramm, S., Stone, J.
openaire +2 more sources
Telework in the post-pandemic scenario: structural elements driving the implementation of the model
The objective of this study was to identify the structural guiding elements for the implementation of a telecommuting model in the post-pandemic scenario.
Hericson Caprioli +1 more
doaj +1 more source
Indicators of Mass in Spherical Stellar Atmospheres
Mass is the most important stellar parameter, but it is not directly observable for a single star. Spherical model stellar atmospheres are explicitly characterized by their luminosity ($L_\star$), mass ($M_\star$) and radius ($R_\star$), and observations
Dinshaw, Rayomond +2 more
core +1 more source
How galactic environment regulates star formation [PDF]
In a new simple model I reconcile two contradictory views on the factors that determine the rate at which molecular clouds form stars-internal structure versus external, environmental influences-providing a unified picture for the regulation of star ...
van der Wel, Sharon Meidt
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Insights on Skyrme parameters from GW170817
The binary neutron-star merger event, GW170817, has cast a new light on nuclear physics research. Using a neutron-star model that includes a crust equation of state (EoS), we calculate the properties of a 1.4 solar-mass neutron star.
C.Y. Tsang +4 more
doaj +1 more source
The rolling shutter effect decreases the accuracy of the attitude measurement of star trackers when they work in rolling shutter exposure mode, especially under dynamic conditions.
Zongqiang Fu +6 more
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Time distribution and loss of scaling in granular flow
Two cellular automata models with directed mass flow and internal time scales are studied by numerical simulations. Relaxation rules are a combination of probabilistic critical height (probability of toppling $p$) and deterministic critical slope ...
Tadic, Bosiljka
core +1 more source
Truncated post-Newtonian neutron star model [PDF]
As a preliminary step towards simulating binary neutron star coalescing problem, we test a post-Newtonian approach by constructing a single neutron star model. We expand the Tolman-Oppenheimer-Volkov equation of hydrostatic equilibrium by the power of $c^
F. A. Rasio +34 more
core +2 more sources

