Difference between revisions of "User:Tohline/AxisymmetricConfigurations/HSCF"
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=Hachisu Self-Consistent-Field Technique= | =Hachisu Self-Consistent-Field Technique= | ||
<table border="0" cellpadding="10" align="left"><tr><th>[[Image:Hai.gif|90px| | <table border="0" cellpadding="10" align="left"><tr><th>[[Image:Hai.gif|90px|center|Izumi Hachisu]]<br />I. Hachisu</th></tr></table> In 1986, Izumi Hachisu published two papers in '''The Astrophysical Journal Supplement Series''' ([http://adsabs.harvard.edu/abs/1986ApJS...61..479H vol. 61, pp. 479-507], and [http://adsabs.harvard.edu/abs/1986ApJS...62..461H vol. 62, pp. 461-499]) describing ''"A Versatile Method for Obtaining Structures of Rapidly Rotating Stars."'' (Henceforth, we will refer to this method as the Hachisu Self-Consistent-Field, or HSCF, technique.) We have found the HSCF technique to be an extremely powerful tool for constructing equilibrium configurations of self-gravitating fluid systems under a wide variety of different circumstances. This chapter has been built upon [http://www.phys.lsu.edu/astro/H_Book.current/Applications/Structure/HSCF_Code/HSCF.outline.html an (''ca.'' 1999) outline of the HSCF technique] that appeared in our [http://www.phys.lsu.edu/astro/H_Book.current/H_Book.html original version of this HyperText Book] (H_Book). The photo of Professor Izumi Hachisu shown here, on the left, dates from the mid-1980s — about the time he developed this remarkably useful numerical technique; a more recent photo can be found on the [http://gpes.c.u-tokyo.ac.jp/faculty-staff/materials-systems-and-dynamics/izumi-hachisu.html web page associated with Professor Hachisu's current faculty appointment at the University of Tokyo, Komaba]. | ||
Revision as of 20:29, 22 March 2018
Hachisu Self-Consistent-Field Technique
 I. Hachisu |
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In 1986, Izumi Hachisu published two papers in The Astrophysical Journal Supplement Series (vol. 61, pp. 479-507, and vol. 62, pp. 461-499) describing "A Versatile Method for Obtaining Structures of Rapidly Rotating Stars." (Henceforth, we will refer to this method as the Hachisu Self-Consistent-Field, or HSCF, technique.) We have found the HSCF technique to be an extremely powerful tool for constructing equilibrium configurations of self-gravitating fluid systems under a wide variety of different circumstances. This chapter has been built upon an (ca. 1999) outline of the HSCF technique that appeared in our original version of this HyperText Book (H_Book). The photo of Professor Izumi Hachisu shown here, on the left, dates from the mid-1980s — about the time he developed this remarkably useful numerical technique; a more recent photo can be found on the web page associated with Professor Hachisu's current faculty appointment at the University of Tokyo, Komaba.
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