The Predictive Power of Computational Astrophysics as a Discovery Tool (IAU S362)

Herausgeber: Bisikalo, Dmitry; Wiebe, Dimitri; Boily, Christian

• Gebundenes Buch

Produktbeschreibung

Computational astrophysics combines modern computational methods, novel hardware designs, advanced algorithms, original software implementations, and new technologies, to discover new phenomena and to make predictions in astronomy. IAU S362 summarizes these developments through astronomers in diverse fields sharing their best practice.

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Produktdetails

• Proceedings of the International Astronomical Union Symposia and Colloquia
• Verlag: Cambridge University Press
• Seitenzahl: 434
• Erscheinungstermin: 27. Oktober 2023
• Englisch
• Abmessung: 250mm x 175mm x 28mm
• Gewicht: 846g
• ISBN-13: 9781108490665
• ISBN-10: 1108490662
• Artikelnr.: 65175445

Inhaltsangabe

Early structure formation in the THESAN radiation-magneto-hydrodynamics
simulations Enrico Garaldi; Simulations of dark matter with frequent
self-interactions Moritz Fischer; Simulations of the reionization of the
clumpy intergalactic medium with a novel particle-based two-moment
radiative transfer scheme Tsang Keung Chan; Favoured inflationary models by
SFC baryogenesis Mariana Panayotova; The effect of non-Gaussian primordial
perturbations on large-scale structure Greco Peña; The complex evolution of
supermassive black holes in cosmological simulations Peter Johansson;
Nature of star formation in first galaxies Mahavir Sharma; The formation of
Supersonically Induced Gas Objects (SIGOs) with H2 cooling Yurina Nakazato;
An idealized setup for cosmological evolution of baryonic gas in isolated
halos Shashank Dattathri; Detecting cosmic filamentary network with
stochastic Bisous mode Moorits Mihkel Muru; Absorption spectra from
galactic wind models: a framework to link PLUTO simulations to TRIDENT
Benedetta Casavecchia; Hydrodynamic simulations and time-dependent
photoionization modeling of starburst-driven superwinds Ashkbiz Danehkar;
Numerical modelling of X-shaped radio galaxies using back-flow model Gourab
Giri; Radiation magnetohydrodynamic simulations of soft x-ray emitting
regions in active galactic nuclei Taichi Igarashi; Cold gas in outflow:
Evidence for delayed positive AGN feedback Yu Qiu; A new code for
relativistic hydrodynamics and its application to FR II radio jets
Jeongbhin Seo; Studying magnetic field amplification in interacting
galaxies using numerical simulations Simon Selg; X-ray spectral and image
spatial models of NGC 3081 with Chandra data Iryna Vavilova; Simulating
star formation in spiral galaxies Steven Rieder; The CNN classification of
galaxies by their image morphological peculiarities Iryna Vavilova;
Velocity-space substructures and bar resonances in an N-body Milky Way
Tetsuro Asano; Fate of escaping orbits in barred galaxies Debasish Mondal;
Dynamical evolution modeling of the Collinder 135 & UBC 7 binary star
cluster Maryna Ishchenko; Multiparticle collision simulations of dense
stellar systems and plasmas Pierfrancesco Di Cintio; A novel generative
method for star clusters from hydrodynamical simulations Stefano
Torniamenti; Stellar population photometric synthesis with AI of S-PLUS
galaxies Vitor Cernic; Clustering stellar pairs to detect extended stellar
structures Sergey Sapozhnikov; Kinetic modeling of auroral events at solar
and extrasolar planets Valery Shematovich; Stellar activity effects on the
atmospheric escape of hot Jupiters Hiroto Mitani; Study of the non-thermal
atmospheric loss for exoplanet ¿ Men c Anastasia Avtaeva; Multi-component
MHD model for hydrogen-helium extended envelope of hot Jupiter Yuliya
Gladysheva; Modeling stellar jitter for the detection of Earth-mass
exoplanets via precision radial velocity measurements Samuel Granovsky;
Thermal atmospheric escape of close-in exoplanets Eugenia Kalinicheva;
Inference of magnetic fields and space weather hazards of rocky extrasolar
planets from a dynamical geophysical model Varnana M. Kumar; Hydrodynamical
simulations of misaligned accretion discs in binary systems: Companions
tear discs Suzan Dogan; Hybrid magnetic structures around spinning black
holes connected to a surrounding accretion disk Ileyk El Mellah; Mass
ejection from neutron-star mergers Masaru Shibata; Merging of spinning
binary black holes in globular clusters Margaryta Sobolenko; Predicting the
expansion of supernova shells using deep learning toward highly resolved
galaxy simulations Keiya Hirashima; Toward realistic models of core
collapse supernovae: A brief review Anthony Mezzacappa; Hot spot drift in
synchronous and asynchronous polars: synthesis of light curves Andrey
Sobolev; The predictive power of numerical simulations in the study
accretion an