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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Numerical models of stellar interiors canonical 1

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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 ⓘ
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 ⓘ