TABLE OF CONTENTS
- 1. /VecMesWinkel
- 1.1. VecMesWinkel/vecmesa
- 1.2. VecMesWinkel/dsigdt
- 1.3. VecMesWinkel/vecdelta
/VecMesWinkel [ Modules ]
NAME
module VecMesWinkel
PURPOSE
Incorporates the functions used for angular distributions of finalstates in gamma N -> V N and gamma N -> V Delta
VecMesWinkel/vecmesa [ Subroutines ]
[ Top ] [ VecMesWinkel ] [ Subroutines ]
NAME
subroutine vecmesa(sqrts,idM,massM,massIn2,cost,iParam,successflag)
PURPOSE
determines scattering angle for gamma N --> V N
INPUTS
- real :: sqrts -- sqrt(s)
- integer :: idM -- ID of vector meson
- real :: massM -- mass of outgoing vector meson
- real :: massIn2 -- mass squared of incoming gamma (negative: Q^2!)
- integer :: iParam -- select the distribution (see below)
OUTPUT
- real :: cost -- cos(theta) of scattering angle
- logical, OPTIONAL :: successflag -- false, if problems with in-medium masses
NOTES
- massIn2 may be negative: Q^2 !
- The slope parameter B and the total cross section should be consistent!
The parameter 'iParam' selects the used distribution:
- =0: 'old' parametrisation for gammaN->VN (cf. Effenberger PhD): Slope paremeter B according ABBHHM collab, PR 175, 1669 (1968)
- =1: Pythia parametrisation: Slope parameter B=2*b_p+2*b_V+4*s**eps-4.2
- =2: 'Donnachie, Landshoff' Select t according dsig/dt as given by VecMesWinkel/dsigdt, not by a given slope parameter
- =3: as 1, but for rho and W<~6GeV slope parameter adjusted according CLAS experimental data [Morrow et al, EPJ A39, 5 (2009)]
- =4: old Muehlich routines
- =5: as 1, but modified for low W (used in rho0 Toy Init)
- =6: W and Q2 dependent slope as fitted to VMD distribution of PYTHIA. Only valid for W<3.3GeV. (used in rho0 Toy Init)
The default value for iParam is 3 (until Jan 2010 the default was 2)
VecMesWinkel/dsigdt [ Functions ]
[ Top ] [ VecMesWinkel ] [ Functions ]
NAME
real function dsigdt(sqrts,t,iv)
PURPOSE
Calculate the cross section dsigma/dt for gamma N -> V N according a parametrization of scattering amplitude from Donnachie and Landshoff
INPUTS
- real :: sqrts -- sqrt(s)
- real :: t -- Mandelstam-t ( <0!)
- integer :: iv -- ID of vector meson
OUTPUT
function value: dsig/dt in mub/GeV^2
NOTES
Reference:
- A. Donnachie and P. V. Landshoff, ``Exclusive vector photoproduction: Confirmation of Regge theory,'' Phys. Lett. B 478, 146 (2000).
The parametrization is for photoproduction.
Range of validity: sqrt(s)=6.9...200 GeV.
Maybe one should upgrade to the newest work of the authors:
- A.~Donnachie and P.~V.~Landshoff, ``Successful description of exclusive vector meson electroproduction,'' arXiv:0803.0686 [hep-ph].
VecMesWinkel/vecdelta [ Subroutines ]
[ Top ] [ VecMesWinkel ] [ Subroutines ]
NAME
subroutine vecdelta(sqrts,idM,massD,massM,massIn2,cost,successflag)
PURPOSE
determines scattering angle for gamma N --> V Delta
INPUTS
- real :: sqrts -- sqrt(s)
- integer :: idM -- ID of vector meson
- real :: massD -- mass of outgoing baryon (Delta)
- real :: massM -- mass of outgoing vector meson
- real :: massIn2 -- mass squared of incoming gamma (negative: Q^2!)
OUTPUT
- real :: cost -- cos(theta) of scattering angle
- logical, OPTIONAL :: successflag -- false, if problems with in-medium masses
NOTES
- massIn2 may be negative: Q^2 !