From: me@marychin.org
Date: Sat Jul 28 2007 - 19:12:20 CEST
Hi.
Following my query on 24th July that I couldn't find any secondaries produced by 10 MeV deuterons in nitrogen-14, I can't find any in neon-20 either.
Is this due to the following explanation:
"In 1992, transport of light ions (deuterons, tritons, 3He, a) was introduced, without nuclear interactions."
which I found on page 363/405 of CERN-2005-10.pdf?
Many thanks,
mary
Forwarded message follows:
> Hi.
> I started 30 MeV deuterons in N14. Deuteron threshold was 10 keV. Input file given below. I found the stars generated per beam particle to be 100% deuterons. Number of secondaries per call to usdraw was at most one, and when it happens the secondary is a deuteron. Shouldn't I expect some neutrons and gammas?
> Many thanks,
> mary
>
> *...+....1....+....2....+....3....+....4....+....5....+....6....+....7....+....8
> TITLE
> Deuterons in a sea of N14
> GLOBAL -1.0
> BEAM -3E-02 1.E4 DEUTERON
> BEAMPOS 0.0 0.0 0.0
> PART-THR -0.00001 -6.0 9.0 0.0 0.0 1.0
> EMFCUT -1.0E-5 1.0E-5 0.0 1.0 @LASTMAT PROD-CUT
> EMFCUT -1.0E-5 1.0E-5 0.0 R1 @LASTREG
> PHYSICS 3.0 EVAPORATion
> GEOBEGIN COMBNAME
> 0 0 A simple sea
> SPH B1 0.0 0.0 0.0 +500000.0
> SPH B2 0.0 0.0 0.0 +500001.0
> END
> R1 5 +B1
> R2 5 -B1 +B2
> END
> GEOEND
> MATERIAL 7.0 14.003074 1. 26.0 14. MYMAT
> LOW-MAT 26.0 NITROGEN
> ASSIGNMAT MYMAT R1
> ASSIGNMAT BLCKHOLE R2
> RADDECAY 2. 0. 1.
> RESNUCLEi 3.
> USERDUMP 100 7.0 1.0 dump
> RANDOMIZE 1.0
> START 2e7
> STOP
>
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