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Springer - Dust-Gas Instabilities in Protoplanetary Disks Book

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Description

How planets form remains a fundamental question in astrophysics. This Springer thesis investigates the formation scenarios of planetesimals, which are the kilometer-sized precursors to planets. While these mechanisms are still a subject of debate, this book explores specific disk instabilities that offer potential explanations for their origin. By utilizing linear analyses and numerical simulations, the text examines how a disk evolves through the development of instabilities. It also introduces a new instability driven by dust coagulation. This research provides a technical look at the processes governing protoplanetary disks and the transition from dust to larger bodies.

Key Features

This Springer thesis explores the long-standing astrophysical question of how planets form.

The text focuses on the formation scenarios of planetesimals, the kilometer-sized precursors to planets.

Research presented includes linear analyses and numerical simulations to study disk evolution.

The book introduces a new instability driven by dust coagulation within protoplanetary disks.

This academic work addresses how disk instabilities explain the origin of planetesimals.

Product Specifications

Format
paperback
Domain
Amazon UK
Release Date
27 April 2023
Listed Since
30 March 2023

Barcode

No barcode data available

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