CDROM/APJS/INPRESS Neutrino Energy Loss in Stellar Interiors. VII (Itoh+ 1995) ================================================================================ Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes Naoki Itoh, Hiroshi Hayashi, Akinori Nishikawa, & Yasuharu Kohyama <1996, ApJS, in press> =1996ApJS...IP....NI ================================================================================ Abstract: The results of the calculations of the neutrino energy loss rates due to pair, photo-, plasma, bremsstrahlung, and recombination processes are summarized in the form of tables and analytic fitting formulae. Care has been taken for the convenience of the users of these results. We have tried to make the present paper as self-contained as possible. The present paper is intended to serve as useful physical input data for stellar evolution computations. Keywords: dense matter -- elementary particles -- radiation mechanisms: miscellaneous -- stars: interiors Description: This paper, which is still in press as of this writing, has been published on the AAS CD-ROM Series with the special permission of the ApJ Editorial Office. The contents of the directories listed below are adequately described by the author-supplied documentation, and the manuscript for the paper accepted by the Astrophysical Journal Supplement Series. The following is directly from the file 'content.doc' supplied by the authors. " Directories and Files " /itoh -+-- /text -+--/tex | +--/graphics | +-- /tables -+-- /pair1 | +-- /pair2 | +-- /photo | +-- /plasma | | +-- /version1 +-- /brems analytic fitting | +-- /pair analytic fitting | +-- /photo analytic fitting | +-- /plasma analytic fitting | +-- /recomb analytic fitting | +-- /version2 +-- /brems analytic fitting | +-- /pair quadratic interpolation | | (grid of log T = 0.2) | +-- /photo quadratic interpolation | +-- /plasma quadratic interpolation | +-- /recomb analytic fitting | +-- /version3 +-- /brems analytic fitting +-- /pair quadratic interpolation | (grid of log T = 0.05) +-- /photo quadratic interpolation +-- /plasma quadratic interpolation +-- /recomb analytic fitting /text; 'NEUTRINO ENERGY LOSS IN STELLAR INTERIORS. VII. PAIR, PHOTO-, PLASMA, BREMSSTRAHLUNG, AND RECOMBINATION PROCESSES ' Itoh, N., Hayashi, H., Nishikwa, A., & Kohyama, Y. textfile; compile with LaTeX graphics; EPS files /tables; numerical data pair.dat1; The grid of log T = 0.05 Q_{pair}^{+} & Q_{pair}^{-} in equation (2.1) pair.dat2; The grid of log T = 0.2 Q_{pair}^{+} & Q_{pair}^{-} in equation (2.1) photo.dat; Q_{photo}^{+} & Q_{photo}^{-} in equation (3.1) plasma.dat; Q_{T} & Q_{L} in equation (4.2) /version1; Fortran programs for the analytic fitting formulae usage compile with Fortran77. edit a; mass number of the ion z; charge number of the ion tinit; initial value of Log( temperature ) tfin; final value of Log( temperature ) tstep; step value of Log( tempetarure ) nt; number of steps of Log( tempetarure ) < integer > rinit; initial value of Log( rho/mu_e ) rfin; final value of Log( rho/mu_e ) rstep; step value of Log( rho/mu_e ) rt; number of steps of Log( rho/mu_e ) < integer > n; (number of neutrino flavors considered) - 1 < integer > zeta; zeta value in equation (6.7) nu; chemical potential in equation (6.8) execute and you will get an output file <'process'.dat> /version2,3; Fortran programs for the analytic fitting formulae and the quadratic interpolations. usage compile with Fortran77. edit recomb/ same as version1 brems/ same as version1 photo/ quadratic interpolations T-initial; initial value of Log( temperature ) T-final ; final value of Log( temperature ) The range of log T is from 7 to 11. The grid of log T is 0.1. Step ; step value of Log( rho/mu_e ) Input the value of step which is less than 0.1. e.g. 0.05, 0.01, ... plasma/ T-initial; initial value of Log( temperature ) T-final ; final value of Log( temperature ) The range of log T is from 7 to 11. The grid of log T is 0.2. Step ; step value of Log( rho/mu_e ) Input the value of step which is less than 0.2. e.g. 0.1, 0.05, 0.01, ... pair/(version2) T-initial; initial value of Log( temperature ) T-final ; final value of Log( temperature ) The range of log T is from 7 to 12. The grid of log T is 0.2. Step ; step value of Log( rho/mu_e ) Input the value of step which is less than 0.1. e.g. 0.05, 0.01, ... pair/(version3) T-initial; initial value of Log( temperature ) T-final ; final value of Log( temperature ) The range of log T is from 7 to 12. The grid of log T is 0.05. Step ; step value of Log( rho/mu_e ) Input the value of step which is less than 0.1. e.g. 0.05, 0.01, ... ================================================================================ (End) Lee Brotzman [ADS] 08-Nov-95