Input description
Card 1: TITLE (A60)
KTRL(1) - controls how many columns of output you get.
If 1, you get energy straggling and multiple scattering (only).
If 2, you get multiple scattering and energy-loss difference (only).
If 3, you get energy straggling and energy-loss diffrence (only).
Note: if you get warning messages that
a hidden target contribution was bigger than those output, you should try
KTRL(1) = 0 or else another new value to check you are not mislead by the
numbers currently output.
If 1, use formulae from Marion & Young.
If 2, use formulae from Review of Particle
Properties (1994).
If 1 use second kinematic soln. Th(c.m.) is output as 180 - th(c.m.)
If 2, first kinematic soln. with th(c.m.) output as 180 - th(c.m.)
If 3, second kinematic soln., th(c.m.)
output as is.
If > 1, gives debug output to stderr.
The higher the value of KTRL(4), the more output generated.
If > 1, also read and calculate contribution
from a given target non-uniformity.
If 1, read mass excesses in keV from input file following Card 7.
If 2, read mass excesses from mass table.
In cases 1 and 2, the baseline nuclear masses are read first (from Card 7). These baseline masses in AMU should include any nuclear excitation energy.
This addition of excitation energy
in AMU also has to be done for KTRL(6)=2: then Card 7 should be the integer
mass + any excitation energy in MeV/AMU). For KTRL(6)=1, any excitation
energy can be more easily added in keV to the mass excess on Card 7a.
If 1, this is done assuming "worst case" distribution of 2 * beta * Egamma.
If 2, there is an empirical reduction by 60%.
See Bohlen et al., Z. Phys. A285 (1978) 379, for proper treatment.
"MYLAR", "KAPTO", "SCINT", "POLYP", "METHA", etc.
If KTRL(6) = 1, they should be input as integers, and the following additional Card 7a will be read.
If KTRL(6) = 2, the masses should be entered as integers, and the mass excesses will be read from a mass table.



