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

The Predictive Power of Computational Astrophysics as a Discovery Tool (IAU S362)（Proceedings of the International Astronomical Union Symposia and Colloquia）

计算天体物理学的预测能力作为发现工具（IAU S362）
天体物理学

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作者

Dmitry Bisikalo

出版社

Cambridge University Press

出版时间

2022年09月01日

装帧

精装

ＩＳＢＮ

9781108490665

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页码

400

开本

247x174mm

语种

英文

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暂无评分

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图书简介

A new paradigm for scientific discovery through computational tools now permeates every aspect of astronomical research. Computational astrophysics combines modern computational methods, novel hardware designs, advanced algorithms, original software implementations, and associated technologies to discover new phenomena and to make predictions in astronomy. The proceedings of IAU Symposium 362 summarizes ongoing developments in computational astrophysics through astronomers in diverse fields sharing their knowledge and approaches. It focuses on computational methods applied to speed up and broaden the scope of scientific studies, such as finding trends in observational data, high performance computing, automated search algorithms, and model predictability. Experts discuss a palette of challenging informational and technical developments, with the goal of coordinating their efforts and the improvement of techniques in pursuit of a wide range of astronomical studies, including fluid dynamics in star and galaxy evolution, exoplanets, gravitational waves, numerical relativity, data mining, and much more.

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

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