* * $Id$ * * $Log$ * Revision 1.1.1.2 1996/10/30 08:30:53 cernlib * Version 7.04 * * Revision 1.1.1.1 1996/04/12 15:29:48 plothow * Version 7.01 * * #include "pdf/pilot.h" SUBROUTINE SMRSPI(X,SCALE,MODE,UPV,DNV,SEA,STR,CHM,BOT,GLU) C***************************************************************C C C C PION DISTRIBUTION FUNCTIONS EXTRACTED FROM DRELL-YAN AND C C PROMPT PHOTON PION BEAM DATA, USING (NUCLEAR TARGET C C CORRECTED) HMRS(B) DISTRIBUTIONS FOR THE NUCLEON. C C MAIN UNCERTAINTY IS IN SEA, HENCE FOLLOWING THREE SETS... C C MODE=2 IS THE "BEST FIT" SET. C C C C MODE 1 CORRESPONDS TO A 10% MOMENTUM SEA (0.11213) C C MODE 2 CORRESPONDS TO A 15% MOMENTUM SEA (0.16119) C C MODE 3 CORRESPONDS TO A 20% MOMENTUM SEA (0.23785) C C C C (NUMBER IN BRACKETS IS LAST ENTRY IN FIRST ROW OF GRID) C C C C -*- C C C C REFERENCE: A.D. MARTIN. R.G. ROBERTS. W.J. STIRLING C C AND P.J. SUTTON, PREPRINT RAL-91-058 (1991). C C -*- C C C C FOR THESE SETS.... C C * LAMBDA(MSBAR,NF=4) = 190 MEV C C * UV=DV, STR=USEA=DSEA, BTM=0 C C C C NOTE THAT X TIMES THE PARTON DISTRIBUTION FUNCTION C C IS RETURNED I.E. G(X) = GLU/X ETC, AND THAT "SEA" C C IS THE QUARK SEA / 6 I.E. UBAR(X)=DBAR(X) C C = SEA/X FOR A PION. IF IN DOUBT, CHECK THE C C MOMENTUM SUM RULE! NOTE ALSO THAT SCALE=Q IN GEV C C C C -*- C C C C THE RANGE OF APPLICABILITY IS CURRENTLY: C C 10**-5 < X < 1 AND 5 < Q**2 < 1.31 * 10**6 C C HIGHER Q**2 VALUES CAN BE SUPPLIED ON REQUEST C C - PROBLEMS, COMMENTS ETC TO WJS@UK.AC.DUR.HEP C C C C C C***************************************************************C #include "pdf/impdp.inc" IF(MODE.EQ.1) CALL SMRSP31(X,SCALE,UPV,DNV,SEA,STR,CHM,BOT,GLU) IF(MODE.EQ.2) CALL SMRSP32(X,SCALE,UPV,DNV,SEA,STR,CHM,BOT,GLU) IF(MODE.EQ.3) CALL SMRSP33(X,SCALE,UPV,DNV,SEA,STR,CHM,BOT,GLU) RETURN END