Numerical models of stellar interiors

E272772

Numerical models of stellar interiors is a seminal astrophysics work by Martin Schwarzschild that developed theoretical and computational methods for understanding the internal structure and evolution of stars.

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Predicate Object
instanceOf astrophysics monograph
scientific book
academicDiscipline computational astrophysics
theoretical astrophysics
appliesTo evolving stellar models
giant stars
main-sequence stars
author Martin Schwarzschild
contribution early use of computers in stellar structure calculations
linking internal stellar structure to observable properties
systematic framework for constructing stellar models
countryOfPublication United States of America
surface form: United States
describes boundary conditions for stellar models
convective energy transport
energy generation in stars
energy transport in stellar interiors
equations of state for stellar matter
equations of stellar structure
hydrostatic equilibrium in stars
nuclear energy generation rates in stars
numerical integration of stellar structure equations
radiative energy transport
stellar opacity
field astrophysics
stellar astrophysics
genre scientific non-fiction
hasImpactOn computational modeling of stars
interpretation of Hertzsprung–Russell diagrams
standard stellar evolution codes
theoretical understanding of stellar lifetimes
influencedBy Martin Schwarzschild’s earlier work on stellar structure
language English
mainSubject stellar evolution
stellar interiors
stellar structure
notableFor developing numerical methods for modeling stellar interiors
developing theoretical methods for modeling stellar interiors
influencing modern stellar evolution theory
timePeriodDescribed 20th-century stellar astrophysics
usedIn graduate education in astrophysics
research on stellar evolution

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Martin Schwarzschild notableWork Numerical models of stellar interiors