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Dust-gas instabilities in protoplane...

Tominaga, Ryosuke.

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Dust-gas instabilities in protoplanetary disks = toward understanding planetesimal formation /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Dust-gas instabilities in protoplanetary disks/ by Ryosuke Tominaga.
Reminder of title:	toward understanding planetesimal formation /
Author:	Tominaga, Ryosuke.
Published:	Singapore :Springer Nature Singapore : : 2022.,
Description:	xii, 116 p. :ill. (chiefly col.), digital ;24 cm.
Notes:	"Doctoral thesis accepted by Nagoya University, Nagoya, Japan."
[NT 15003449]:	Introduction -- Revision of Macroscopic Equations for Dust Diffusion -- Numerical Simulations of Secular Instabilities -- Coagulation Instability in Protoplanetary Disks -- Summary and Future Prospects.
Contained By:	Springer Nature eBook
Subject:	Protoplanetary disks. -
Online resource:	https://doi.org/10.1007/978-981-19-1765-3
ISBN:	9789811917653

Dust-gas instabilities in protoplanetary disks = toward understanding planetesimal formation /
Tominaga, Ryosuke.

Dust-gas instabilities in protoplanetary diskstoward understanding planetesimal formation /[electronic resource] :by Ryosuke Tominaga. - Singapore :Springer Nature Singapore :2022. - xii, 116 p. :ill. (chiefly col.), digital ;24 cm. - Springer theses,2190-5061. - Springer theses..

"Doctoral thesis accepted by Nagoya University, Nagoya, Japan."

Introduction -- Revision of Macroscopic Equations for Dust Diffusion -- Numerical Simulations of Secular Instabilities -- Coagulation Instability in Protoplanetary Disks -- Summary and Future Prospects.

How planets form is one of the long-standing questions in astrophysics. In particular, formation scenarios of planetesimals which are kilometer-sized bodies and a precursor of planets are still unclear and under debate although some promising mechanisms have been proposed. This book highlight disk instabilities that have the potential to explain the origin of planetesimals. Using linear analyses and numerical simulations, it addresses how a disk evolves through the development of instabilities, and also presents a new instability driven by dust coagulation. As a result, the simulation demonstrates a scenario of planetesimal formation: A successive development of multiple instabilities triggers planetesimal formation in resulting dusty rings.

ISBN: 9789811917653

Standard No.: 10.1007/978-981-19-1765-3doiSubjects--Topical Terms:

3526149
Protoplanetary disks.

LC Class. No.: QB603.O74 / T65 2022

Dewey Class. No.: 523.4

Dust-gas instabilities in protoplanetary disks = toward understanding planetesimal formation /
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520 $a How planets form is one of the long-standing questions in astrophysics. In particular, formation scenarios of planetesimals which are kilometer-sized bodies and a precursor of planets are still unclear and under debate although some promising mechanisms have been proposed. This book highlight disk instabilities that have the potential to explain the origin of planetesimals. Using linear analyses and numerical simulations, it addresses how a disk evolves through the development of instabilities, and also presents a new instability driven by dust coagulation. As a result, the simulation demonstrates a scenario of planetesimal formation: A successive development of multiple instabilities triggers planetesimal formation in resulting dusty rings.
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