The Glass Transition

Mattsson, Johan

doi:10.1002/9781119220510.ch13

Search citation statements

Order By: Relevance

Paper Sections

Select...

Mean-flow Equations1

Citation Types

Supporting

Mentioning

Contrasting

Year Published

2017

Publication Types

Select...

Other1

Relationship

Self Cite0

Independent1

Authors

Journals

Cited by 1 publication

(1 citation statement)

References 93 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Using Favré (1962) averaging the equation of motion (EOM) for a spherical wind will receive an additional "wave pressure" term (see Mattsson 2016 and references therein for further details),…”

Section: Mean-flow Equationsmentioning

confidence: 99%

Improved implementation of dust-driven winds and dust formation in models of AGB evolution: Effects of pulsation and gas-pressure forcing

Mattsson,

Ventura

2017

Preprint

View full text Add to dashboard Cite

Mass loss is a crucial component in stellar evolution models, since it largely determines the rate of evolution at the later stages of a star's life. The dust-driven outflows from AGB stars are particularly important in this regard. Including AGB dust formation in a stellar evolution model does also require a model of these outflows. Since AGB stars exhibit large-amplitude pulsation, a model based on time-dependent radiation hydrodynamics (RHD) is needed in order to capture all the important physical aspects of dust formation. However, this cannot be afforded in a stellar evolution model. Here, a mean-flow model is presented, which include corrections to the steady-state model currently being used in AGB evolution models with dust formation.

show abstract

Section: Mean-flow Equationsmentioning

confidence: 99%