Neuronal Parameter Space Exploration

2015 ◽  
pp. 2058-2060
Author(s):  
Wafa Soofi
Keyword(s):  
Parameter Space ◽  
Space Exploration ◽  
Neuronal Parameter

Rapid Characterization and Parameter Space Exploration of Perovskites Using an Automated Routine

2019 ◽  
Vol 22 (1) ◽  
pp. 6-17 ◽  
Author(s):  
Elisabeth Reinhardt ◽  
Ahmed M. Salaheldin ◽  
Monica Distaso ◽  
Doris Segets ◽  
Wolfgang Peukert
Keyword(s):  
Parameter Space ◽  
Space Exploration ◽  
Rapid Characterization

scholarly journals Parameter space exploration of the minimal SU(5) unification

2021 ◽  
Vol 104 (1) ◽  
Author(s):  
Ilja Doršner ◽  
Emina Džaferović-Mašić ◽  
Shaikh Saad
Keyword(s):  
Parameter Space ◽  
Space Exploration

scholarly journals InSituNet: Deep Image Synthesis for Parameter Space Exploration of Ensemble Simulations

2019 ◽  
pp. 1-1 ◽  
Author(s):  
Wenbin He ◽  
Junpeng Wang ◽  
Hanqi Guo ◽  
Ko-Chih Wang ◽  
Han-Wei Shen ◽  
...  
Keyword(s):  
Parameter Space ◽  
Space Exploration ◽  
Image Synthesis ◽  
Ensemble Simulations ◽  
Deep Image

scholarly journals Constraining protoplanetary discs with exoplanetary dynamics: Kepler-419 as an example

2020 ◽  
Vol 499 (1) ◽  
pp. 106-115
Author(s):  
Mohamad Ali-Dib ◽  
Cristobal Petrovich
Keyword(s):  
Parameter Space ◽  
Time Scale ◽  
Space Exploration ◽  
Semimajor Axis ◽  
Higher Order ◽  
Mean Motion Resonances ◽  
Close Encounters ◽  
Natural Result ◽  
Core Accretion ◽  
Orbital Migration

ABSTRACT We investigate the origins of Kepler-419, a peculiar system hosting two nearly coplanar and highly eccentric gas giants with apsidal orientations liberating around anti-alignment, and use this system to place constraints on the properties of their birth protoplanetary disc. We follow the proposal by Petrovich, Wu, & Ali-Dib that these planets have been placed on these orbits as a natural result of the precessional effects of a dissipating massive disc and extend it by using direct N-body simulations and models for the evolution of the gas discs, including photoevaporation. Based on a parameter space exploration, we find that in order to reproduce the system the initial disc mass had to be at least 95 MJup and dissipate on a time-scale of at least 104 yr. This mass is consistent with the upper end of the observed disc masses distribution, and the dissipation time-scale is consistent with photoevaporation models. We study the properties of such discs using simplified 1D thin-disc models and show that they are gravitationally stable, indicating that the two planets must have formed via core accretion and thus prone to disc migration. We hence finally investigate the sensitivity of this mechanism to the outer planet’s semimajor axis, and find that the nearby 7:1, 8:1, and 9:1 mean-motion resonances can completely quench this mechanism, while even higher order resonances can also significantly affect the system. Assuming the two planets avoid these high-order resonances and close encounters, the dynamics seems to be rather insensitive to planet c semimajor axis, and thus orbital migration driven by the disc.

scholarly journals THE DEUTERIUM FRACTIONATION TIMESCALE IN DENSE CLOUD CORES: A PARAMETER SPACE EXPLORATION

2015 ◽  
Vol 804 (2) ◽  
pp. 98 ◽  
Author(s):  
Shuo Kong ◽  
Paola Caselli ◽  
Jonathan C. Tan ◽  
Valentine Wakelam ◽  
Olli Sipilä
Keyword(s):  
Parameter Space ◽  
Space Exploration ◽  
Dense Cloud ◽  
Cloud Cores

Parameter space exploration of short-pulse laser-driven ion acceleration via ensemble simulations and neural networks

2021 ◽  
Author(s):  
Blagoje Z. Djordjevic ◽  
Andreas Kemp ◽  
Joohwan Kim ◽  
Scott Wilks ◽  
Raspberry Simpson ◽  
...  
Keyword(s):  
Neural Networks ◽  
Pulse Laser ◽  
Parameter Space ◽  
Short Pulse ◽  
Space Exploration ◽  
Ion Acceleration ◽  
Ensemble Simulations ◽  
Short Pulse Laser
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