Multi-dimensional processes in stellar physics : Evry Schatzman School 2018 /
Multi-dimensional processes in stellar physics : Evry Schatzman School 2018 /
Michel Rieutord, Isabelle Baraffe and Yveline Lebreton, Eds.
- 1 online resource
- EDP sciences proceedings .
- EDP sciences proceedings. .
Includes bibliographical references.
Multi-Dimensional Processes In Stellar Physics -- List of Participants -- Table of contents -- Preface -- Double-diffusive processes in stellar astrophysics -- 1 Introduction -- 2 Linear instability of double-diffusive systems -- 3 Mixing by fingering convection -- 4 Oscillatory double-diffusive convection and layered convection -- 5 What next? -- References -- Thermo-compositional adiabatic and diabatic convection -- 1 Introduction -- 2 Linear stability analysis of adiabatic and diabatic convection -- 3 Non-linear regime and temperature-gradient reduction -- References Fully compressible time implicit hydrodynamics simulations for stellar interiors -- 1 The MUSIC code -- 2 An example of application: convective penetration -- References -- Thermal Convection in Stars and in Their Atmosphere -- 1 Introduction -- 2 Convection in astrophysics and the basic physics of convection -- 3 Modelling of convection -- 4 Challenges and pitfalls in numerical modelling -- 5 Applications: overshooting -- 6 Summary -- References -- Turbulence in stably stratified radiative zone -- 1 Introduction -- 2 Stability of parallel shear flows in radiative atmosphere 3 Turbulent transport -- 4 Conclusion -- References -- An extremely short course on stellar rotation and magnetism -- Preface -- Lecture 1: An introduction to stellar rotation and magnetism -- Lecture 2: Descriptive MHD, and some limiting cases in fluid mechanics -- Lecture 3: an introduction to dynamo theory -- Closing remarks: simulations, open issues, and a biased summary -- References -- Stellar magnetism: bridging dynamos and winds -- 1 Introduction -- 2 A brief summary of what is a star -- 3 Mean-field model of stellar dynamo and nonlinear aspects 4 Stellar wind: extensions of the Parker model -- 5 Coupling dynamo and stellar wind on dynamical and secular timescales: a perspective -- 6 Conclusion -- References -- 7 Solutions of the exercises -- Multi-dimensional asteroseismology -- 1 Introduction -- 2 Impact of rotation on stellar structure and evolution -- 3 Calculating pulsations -- 4 The effects of rotation on pulsations -- 5 Asteroseismology -- 6 Conclusion -- References -- Multi-dimensional physics of core-collapse supernovae -- 1 Introduction -- 2 Hydrodynamic instabilities -- 3 Magnetic field origin and impact -- 4 Conclusion
When one has to deal with fluid flows, magnetic fields or heat transfer in stars, one faces the partial differential equations that govern these processes. These phenomena are naturally multi-dimensional and their study requires new and sophisticated models. This volume gathers the lecture notes which summarize the essence of the lectures and conferences given by world experts in the field of multi-dimensional modelling of stars, during the 2018 Evry Schatzman School held in Roscoff, France. It gives the present status of our understanding of several processes that occur in stars, like thermal convection, double-diffusive convection, dynamo effect or baroclinic flows. Every subject is discussed under the light of the most recent results of nowadays research and is made accessible to all newcomers, either students or researchers who wish to join the field.
9782759824373 (electronic bk.) 2759824373 (electronic bk.)
Differential equations, Partial--Congresses.
Équations aux dérivées partielles--Congrès.
Differential equations, Partial.
Electronic books.
Conference papers and proceedings.
QA374
515.353
Includes bibliographical references.
Multi-Dimensional Processes In Stellar Physics -- List of Participants -- Table of contents -- Preface -- Double-diffusive processes in stellar astrophysics -- 1 Introduction -- 2 Linear instability of double-diffusive systems -- 3 Mixing by fingering convection -- 4 Oscillatory double-diffusive convection and layered convection -- 5 What next? -- References -- Thermo-compositional adiabatic and diabatic convection -- 1 Introduction -- 2 Linear stability analysis of adiabatic and diabatic convection -- 3 Non-linear regime and temperature-gradient reduction -- References Fully compressible time implicit hydrodynamics simulations for stellar interiors -- 1 The MUSIC code -- 2 An example of application: convective penetration -- References -- Thermal Convection in Stars and in Their Atmosphere -- 1 Introduction -- 2 Convection in astrophysics and the basic physics of convection -- 3 Modelling of convection -- 4 Challenges and pitfalls in numerical modelling -- 5 Applications: overshooting -- 6 Summary -- References -- Turbulence in stably stratified radiative zone -- 1 Introduction -- 2 Stability of parallel shear flows in radiative atmosphere 3 Turbulent transport -- 4 Conclusion -- References -- An extremely short course on stellar rotation and magnetism -- Preface -- Lecture 1: An introduction to stellar rotation and magnetism -- Lecture 2: Descriptive MHD, and some limiting cases in fluid mechanics -- Lecture 3: an introduction to dynamo theory -- Closing remarks: simulations, open issues, and a biased summary -- References -- Stellar magnetism: bridging dynamos and winds -- 1 Introduction -- 2 A brief summary of what is a star -- 3 Mean-field model of stellar dynamo and nonlinear aspects 4 Stellar wind: extensions of the Parker model -- 5 Coupling dynamo and stellar wind on dynamical and secular timescales: a perspective -- 6 Conclusion -- References -- 7 Solutions of the exercises -- Multi-dimensional asteroseismology -- 1 Introduction -- 2 Impact of rotation on stellar structure and evolution -- 3 Calculating pulsations -- 4 The effects of rotation on pulsations -- 5 Asteroseismology -- 6 Conclusion -- References -- Multi-dimensional physics of core-collapse supernovae -- 1 Introduction -- 2 Hydrodynamic instabilities -- 3 Magnetic field origin and impact -- 4 Conclusion
When one has to deal with fluid flows, magnetic fields or heat transfer in stars, one faces the partial differential equations that govern these processes. These phenomena are naturally multi-dimensional and their study requires new and sophisticated models. This volume gathers the lecture notes which summarize the essence of the lectures and conferences given by world experts in the field of multi-dimensional modelling of stars, during the 2018 Evry Schatzman School held in Roscoff, France. It gives the present status of our understanding of several processes that occur in stars, like thermal convection, double-diffusive convection, dynamo effect or baroclinic flows. Every subject is discussed under the light of the most recent results of nowadays research and is made accessible to all newcomers, either students or researchers who wish to join the field.
9782759824373 (electronic bk.) 2759824373 (electronic bk.)
Differential equations, Partial--Congresses.
Équations aux dérivées partielles--Congrès.
Differential equations, Partial.
Electronic books.
Conference papers and proceedings.
QA374
515.353