國立高雄大學圖資館 |

Language: English

Back

Dust-gas instabilities in protoplanetary diskstoward understanding planetesimal formation /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Dust-gas instabilities in protoplanetary disksby 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."
Contained By:	Springer Nature eBook
Subject:	Protoplanetary disks.
Online resource:	https://doi.org/10.1007/978-981-19-1765-3
ISBN:	9789811917653$q(electronic bk.)

Dust-gas instabilities in protoplanetary diskstoward 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$q(electronic bk.)

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

876509
Protoplanetary disks.

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

Dewey Class. No.: 523.4

Dust-gas instabilities in protoplanetary diskstoward understanding planetesimal formation /
LDR:02117nmm a2200349 a 4500 001 621599
003 DE-He213
005 20220425133602.0
006 m d
007 cr nn 008maaau
008 221121s2022 si s 0 eng d
020 $a 9789811917653$q(electronic bk.)
020 $a 9789811917646$q(paper)
024 7 $a 10.1007/978-981-19-1765-3 $2 doi
035 $a 978-981-19-1765-3
040 $a GP $c GP
041 0 $a eng
050 4 $a QB603.O74 $b T65 2022
072 7 $a PGS $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGS $2 thema
082 0 4 $a 523.4 $2 23
090 $a QB603.O74 $b T657 2022
100 1 $a Tominaga, Ryosuke. $3 922898
245 1 0 $a Dust-gas instabilities in protoplanetary disks $h [electronic resource] : $b toward understanding planetesimal formation / $c by Ryosuke Tominaga.
260 $a Singapore : $b Springer Nature Singapore : $b Imprint: Springer, $c 2022.
300 $a xii, 116 p. : $b ill. (chiefly col.), digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5061
500 $a "Doctoral thesis accepted by Nagoya University, Nagoya, Japan."
505 0 $a Introduction -- Revision of Macroscopic Equations for Dust Diffusion -- Numerical Simulations of Secular Instabilities -- Coagulation Instability in Protoplanetary Disks -- Summary and Future Prospects.
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.
650 0 $a Protoplanetary disks. $3 876509
650 0 $a Planets $x Origin. $3 278624
650 1 4 $a Planetary Science. $3 920190
650 2 4 $a Astrophysics. $3 225419
650 2 4 $a Computational Physics and Simulations. $3 913439
710 2 $a SpringerLink (Online service) $3 273601
773 0 $t Springer Nature eBook
830 0 $a Springer theses. $3 557607
856 4 0 $u https://doi.org/10.1007/978-981-19-1765-3
950 $a Physics and Astronomy (SpringerNature-11651)