Ja n 20 06 2 - D Stellar Evolution Code Including Arbitrary Magnetic Fields . I . Mathematical Techniques and Test Cases

نویسندگان

  • L. H. Li
  • P. Ventura
  • S. Basu
  • S. Sofia
  • P. Demarque
چکیده

A high-precision two-dimensional stellar evolution code has been developed for studying solar variability due to structural changes produced by varying internal magnetic fields of arbitrary configurations. Specifically, we are interested in modeling the effects of a dynamo-type field on the detailed internal structure and on the global parameters of the Sun. The high precision is required both to model very small solar changes (of order of 10 −4) and short time scales (or order of one year). It is accomplished by using the mass coordinate to replace the radial coordinate, by using fixed and adjustable time steps, a realistic stellar atmosphere, elements diffusion, and by adjusting the grid points. We have also built into the code the potential to subsequently include rotation and turbulence. The current code has been tested for several cases, including its ability to reproduce the 1-D results.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Evolution Code Including Arbitrary Magnetic Fields . I . Mathematical Techniques and Test Cases

A high-precision two-dimensional stellar evolution code has been developed for studying solar variability due to structural changes produced by varying internal magnetic fields of arbitrary configurations. Specifically, we are interested in modeling the effects of a dynamo-type field on the detailed internal structure and on the global parameters of the Sun. The high precision is required both ...

متن کامل

ar X iv : g r - qc / 0 70 11 09 v 1 1 9 Ja n 20 07 WhiskyMHD : a new numerical code for general relativistic magnetohydrodynamics

The accurate modelling of astrophysical scenarios involving compact objects and magnetic fields, such as the collapse of rotating magnetized stars to black holes or the phenomenology of γ-ray bursts, requires the solution of the Einstein equations together with those of general-relativistic magnetohydrodynamics. We present a new numerical code developed to solve the full set of general-relativi...

متن کامل

Ja n 20 01 Spectra of 2 D H - donors in magnetic field and their Zeeman splitting

The pseudoperturbative shifted l expansion technique PSLET [20-25] is employed to study the spectra of 2D H-donors in magnetic field. The Zeeman effect is investigated and results are found to be excellent compared to those in ref[14].

متن کامل

ar X iv : m at h - ph / 0 20 10 06 v 2 1 5 Ja n 20 02 Quasi - classical versus non - classical spectral asymptotics for magnetic Schrödinger operators with decreasing electric potentials

We consider the Schrödinger operator H on L 2 (R 2) or L 2 (R 3) with constant magnetic field, and electric potential V which typically decays at infinity exponentially fast or has a compact support. We investigate the asymptotic behaviour of the discrete spectrum of H near the boundary points of its essential spectrum. If the decay of V is Gaussian or faster, this behaviour is non-classical in...

متن کامل

ar X iv : a st ro - p h / 06 01 53 0 v 1 2 4 Ja n 20 06 A Braking Index for the Young Pulsar at the Center of the Supernova Remnant Kes 75

We present the first phase-coherent measurement of a braking index for the young, energetic and high magnetic field pulsar, PSR J1846−0258, located at the center of the supernova remnant Kes 75. We present two consistent timing solutions from a phase-coherent timing analysis over 2 yr and a partially phasecoherent timing analysis of 6 yr of widely spaced data obtained with the Rossi X-ray Timin...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2006