5 * Revision 1.1.1.2 1996/10/30 08:28:52 cernlib
8 * Revision 1.1.1.1 1996/04/12 15:29:24 plothow
12 #include "pdf/pilot.h"
13 SUBROUTINE MRSDSHD(X,SCALE,MODE,UPV,DNV,USEA,DSEA,STR,CHM,BOT,GL)
14 C***************************************************************C
17 C MRS *** DIS SCHEME ** VERSIONS: S0',D0',D-' (FEB 1993) C
18 C NEW SET MRS(H) ADDED (DECEMBER 1993) C
20 C MODE 1 IS THE MRS(S0'-DIS) SET C
21 C MODE 2 IS THE MRS(D0'-DIS) SET C
22 C MODE 3 IS THE MRS(D-'-DIS) SET C
23 C MODE 4 IS THE MRS(H-DIS) SET C
24 C ALL SETS ARE FITTED TO THE RECENT NMC C
25 C AND CCFR STRUCTURE FUNCTION DATA, C
26 C AND HAVE (D0',D-',H) UBAR < DBAR IN THE SEA. C
27 C BOTH THESE NEW SETS HAVE C
28 C LAMBDA(MSbar,NF=4) = 230 MeV C
30 C THE REFERENCE IS: A.D. Martin, R.G. Roberts and C
31 C W.J. Stirling, RAL preprint RAL-93-077 (1993) C
34 C >>>>>>>> CROSS CHECK <<<<<<<< C
36 C THE FIRST NUMBER IN THE "1" GRID IS 0.01733 C
37 C THE FIRST NUMBER IN THE "2" GRID IS 0.00930 C
38 C THE FIRST NUMBER IN THE "3" GRID IS 0.00783 C
39 C THE FIRST NUMBER IN THE "4" GRID IS 0.01508 C
43 C (NOTE THAT X TIMES THE PARTON DISTRIBUTION FUNCTION C
44 C IS RETURNED I.E. G(X) = GLU/X ETC. IF IN DOUBT, CHECK THE C
45 C MOMENTUM SUM RULE! NOTE ALSO THAT SCALE=Q IN GEV) C
49 C (THE RANGE OF APPLICABILITY IS CURRENTLY: C
50 C 10**-5 < X < 1 AND 5 < Q**2 < 1.31 * 10**6 C
51 C HIGHER Q**2 VALUES CAN BE SUPPLIED ON REQUEST C
52 C - PROBLEMS, COMMENTS ETC TO WJS@UK.AC.DUR.HEP C
55 C***************************************************************C
56 #include "pdf/impdp.inc"
57 IF(MODE.EQ.1) CALL SFDISS0(X,SCALE,UPV,DNV,USEA,DSEA,STR,CHM,BOT,
59 IF(MODE.EQ.2) CALL SFDISD0(X,SCALE,UPV,DNV,USEA,DSEA,STR,CHM,BOT,
61 IF(MODE.EQ.3) CALL SFDISDM(X,SCALE,UPV,DNV,USEA,DSEA,STR,CHM,BOT,
63 IF(MODE.EQ.4)CALL SFDISH(X,SCALE,UPV,DNV,USEA,DSEA,STR,CHM,BOT,GL)