Re: (n,gamma) interaction

From: Vasilis Vlachoudis <Vasilis.Vlachoudis_at_cern.ch>
Date: Mon, 6 Jun 2011 13:55:22 +0200

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Hi Julian,

photonuclear interactions are not on by default. Please use the PHOTONUC
card to enable them and possibly the LAM-BIAS to enhance them.
Please find attached an input file that I used to test
The output of the MDSTCK is printed in the .log file

Cheers
Vasilis

On 01/06/11 11:03, Julian Rassolov wrote:
> Good afternoon , Vasilis.
> I have triedto use the subroutine that you sent me and have
> successfully compiled it , but unfortunately due to luck of my
> experience I want able to use this function properly ( actually I
> wasn't able to use it at all ) . If it is possible for you to send me
> some small example of usage of any function (and the way to collect
> its results) in the fluka - it would be great.
> Thank you in advance , Julian.
>
> On Wed, May 18, 2011 at 3:32 PM, Vasilis Vlachoudis
> <Vasilis.Vlachoudis_at_cern.ch <mailto:Vasilis.Vlachoudis_at_cern.ch>> wrote:
>
> Dear Julian,
>
> there is no direct solution to identify the reaction, however by
> inspecting the particles stack you can find out if a photon pushes
> neutrons (after a photonuclear reaction). The way I found was to
> use the routine MDSTCK,
> which is called just after an interaction and before pushing the
> secondaries in the main FLUKA stack (FLKSTK).
> Note the particle that made the interaction is removed from the
> stack, actually only the stack pointer NPFLKA is decreased, and
> all its information is found in the main stack with pointer NPFLKA+1
>
> Therefore you inspect the if the "last" particle (NPFLKA+1) in the
> stack to check if it was a photon ILOFLK(NPFLKA+1)=7
> and scan the secondary particles from (GENSTK) if any of the them
> KPART(#)=8 is a neutron
>
> SUBROUTINE MDSTCK ( IFLAG, NPSECN )
>
> INCLUDE '(DBLPRC)'
> INCLUDE '(DIMPAR)'
> INCLUDE '(IOUNIT)'
> *
> *----------------------------------------------------------------------*
> *
> *
> * Copyright (C) 1998-2007 by Alfredo Ferrari & Paola
> Sala *
> * All Rights Reserved.
> *
> *
> *
> *
> *
> * Created on 19 may 1998 by Alfredo Ferrari & Paola
> Sala *
> * Infn - Milan
> *
> *
> *
> * Last change on 18-jan-07 by Alfredo Ferrari
> *
> *
> *
> *
> *
> * Iflag = 1: standard Kaskad call
> *
> * = 2: Kaskad call after elastic (but hydrogen)
> *
> * = 3: Kasneu call
> *
> * = 4: Emfsco call
> *
> *
> *
> *----------------------------------------------------------------------*
> *
> INCLUDE '(EMFSTK)'
> INCLUDE '(FHEAVY)'
> INCLUDE '(FLKSTK)'
> INCLUDE '(GENSTK)'
> INCLUDE '(TRACKR)'
>
> LOGICAL LFIRST
>
> * Peak the last removed particle from the stack
> IF (ILOFLK(NPFLKA+1) .EQ. 7) THEN
> * Scan the secondary stack
> LFIRST = .TRUE.
> DO I=1,NP,1
> * Do we have a neutron there
> IF (KPART(I).EQ.8) THEN
> IF (LFIRST) THEN DO
> LFIRST = .FALSE.
> PRINT *,'Photonnuclear: E=',TKEFLK(NPFLKA+1)
> PRINT *,' Weight=',WTFLK(NPFLKA+1)
> PRINT *,' Pos=',XFLK(NPFLKA+1),
> & YFLK(NPFLKA+1),
> & ZFLK(NPFLKA+1)
> END IF
> PRINT *,' neutron E=',TKI(I), ' wgt=',WEI(I)
> END IF
> END DO
> END IF
> *
> RETURN
> *=== End of subroutine Mdstck
> =========================================*
> END
>
>
>
> Vasilis Vlachoudis
> Dep EN, CERN
> CH-1211 GENEVA 23
> SWITZERLAND
>
> Phone: +41-22 767 9851
> GSM: +41-76 487 4378
> Fax: +41-22 766 9644
>
>
> ________________________________________
> From: owner-fluka-discuss_at_mi.infn.it
> <mailto:owner-fluka-discuss_at_mi.infn.it>
> [owner-fluka-discuss_at_mi.infn.it
> <mailto:owner-fluka-discuss_at_mi.infn.it>] on behalf of Julian
> Rassolov [julian.rassolov_at_gmail.com
> <mailto:julian.rassolov_at_gmail.com>]
> Sent: 16 May 2011 19:50
> To: fluka-discuss_at_fluka.org <mailto:fluka-discuss_at_fluka.org>
> Subject: (n,gamma) interaction
>
> Good afternoon, everyone.
>
> I am facing some problem here, I need to track amount of the gamma-n
> reaction that took place in some material. How is it possible to
> define?
>
>
> Thank you in advance,
>
> Julian.
>
>
>

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    Hi Julian,<br>
    <br>
    photonuclear interactions are not on by default. Please use the
    PHOTONUC card to enable them and possibly the LAM-BIAS to enhance
    them.<br>
    Please find attached an input file that I used to test<br>
    The output of the MDSTCK is printed in the .log file<br>
    <br>
    Cheers<br>
    Vasilis<br>
    <br>
    On 01/06/11 11:03, Julian Rassolov wrote:
    <blockquote
      cite="mid:BANLkTi=PsqOHtS7FuhD6ERhADv7Uu_9GMg_at_mail.gmail.com"
      type="cite">
      <meta http-equiv="Content-Type" content="text/html;
        charset=ISO-8859-1">
      <div dir="ltr">
        <div>Good afternoon&nbsp; , Vasilis.</div>
        <div>&nbsp;</div>
        <div>I have triedto use the subroutine that you sent me and have
          successfully compiled it , but unfortunately due to luck of my
          experience I want able to use this function properly (
          actually I wasn't able to use it at all ) . If it is possible
          for you to send me some small example of usage of any function
          (and the way to collect its results) in the fluka - it would
          be great.</div>
        <div>&nbsp;</div>
        <div>Thank you in advance , Julian.<br>
          <br>
        </div>
        <div class="gmail_quote">On Wed, May 18, 2011 at 3:32 PM,
          Vasilis Vlachoudis <span dir="ltr">&lt;<a
              moz-do-not-send="true"
              href="mailto:Vasilis.Vlachoudis_at_cern.ch">Vasilis.Vlachoudis_at_cern.ch</a>&gt;</span>
          wrote:<br>
          <blockquote class="gmail_quote" style="padding-left: 1ex;
            margin: 0px 0px 0px 0.8ex; border-left: 1px solid rgb(204,
            204, 204);">Dear Julian,<br>
            <br>
            there is no direct solution to identify the reaction,
            however by inspecting the particles stack you can find out
            if a photon pushes neutrons (after a photonuclear reaction).
            The way I found was to use the routine MDSTCK,<br>
            which is called just after an interaction and before pushing
            the secondaries in the main FLUKA stack (FLKSTK).<br>
            Note the particle that made the interaction is removed from
            the stack, actually only the stack pointer NPFLKA is
            decreased, and all its information is found in the main
            stack with pointer NPFLKA+1<br>
            <br>
            Therefore you inspect the if the "last" particle (NPFLKA+1)
            in the stack to check if it was a photon ILOFLK(NPFLKA+1)=7<br>
            and scan the secondary particles from (GENSTK) if any of the
            them KPART(#)=8 is a neutron<br>
            <br>
            &nbsp; &nbsp; &nbsp;SUBROUTINE MDSTCK ( IFLAG, NPSECN )<br>
            <br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(DBLPRC)'<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(DIMPAR)'<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(IOUNIT)'<br>
            *<br>
*----------------------------------------------------------------------*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; Copyright (C) 1998-2007 &nbsp; &nbsp; &nbsp;by
&nbsp; &nbsp;Alfredo Ferrari
            &amp; Paola Sala &nbsp;*<br>
            * &nbsp; &nbsp; All Rights Reserved. &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; *<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; Created on &nbsp; &nbsp;19 may 1998 &nbsp;
&nbsp;by &nbsp; &nbsp;Alfredo Ferrari
            &amp; Paola Sala &nbsp;*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; Infn -
            Milan &nbsp; &nbsp; &nbsp; *<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; Last change on 18-jan-07 &nbsp; &nbsp; by
&nbsp; &nbsp;Alfredo Ferrari &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; *<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp;Iflag = 1: standard Kaskad call
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; *<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;= 2: Kaskad
call after elastic (but hydrogen)
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; *<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;= 3: Kasneu
call &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;= 4: Emfsco
call &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
            * &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;*<br>
*----------------------------------------------------------------------*<br>
            *<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(EMFSTK)'<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(FHEAVY)'<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(FLKSTK)'<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(GENSTK)'<br>
            &nbsp; &nbsp; &nbsp;INCLUDE '(TRACKR)'<br>
            <br>
            &nbsp; &nbsp; &nbsp;LOGICAL LFIRST<br>
            <br>
            * Peak the last removed particle from the stack<br>
            &nbsp; &nbsp; &nbsp;IF (ILOFLK(NPFLKA+1) .EQ. 7) THEN<br>
            * Scan the secondary stack<br>
            &nbsp; &nbsp; &nbsp; &nbsp; LFIRST = .TRUE.<br>
            &nbsp; &nbsp; &nbsp; &nbsp; DO I=1,NP,1<br>
            * Do we have a neutron there<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;IF (KPART(I).EQ.8)
THEN<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;IF
(LFIRST) THEN DO<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp;LFIRST = .FALSE.<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp;PRINT *,'Photonnuclear:
            E=',TKEFLK(NPFLKA+1)<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp;PRINT *,' Weight=',WTFLK(NPFLKA+1)<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp;PRINT *,' &nbsp; &nbsp;Pos=',XFLK(NPFLKA+1),<br>
            &nbsp; &nbsp; &amp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; YFLK(NPFLKA+1),<br>
            &nbsp; &nbsp; &amp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; ZFLK(NPFLKA+1)<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;END IF<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;PRINT
*,' &nbsp; neutron E=',TKI(I), '
            wgt=',WEI(I)<br>
            &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;END IF<br>
            &nbsp; &nbsp; &nbsp; &nbsp; END DO<br>
            &nbsp; &nbsp; &nbsp;END IF<br>
            *<br>
            &nbsp; &nbsp; &nbsp;RETURN<br>
            *=== End of subroutine Mdstck
            =========================================*<br>
            &nbsp; &nbsp; &nbsp;END<br>
            <br>
            <br>
            <br>
            Vasilis Vlachoudis<br>
            Dep EN, CERN<br>
            CH-1211 GENEVA 23<br>
            SWITZERLAND<br>
            <br>
            Phone: &nbsp;+41-22 767 9851<br>
            GSM: &nbsp; &nbsp;+41-76 487 4378<br>
            Fax: &nbsp; &nbsp;+41-22 766 9644<br>
            <br>
            <br>
            ________________________________________<br>
            From: <a moz-do-not-send="true"
              href="mailto:owner-fluka-discuss_at_mi.infn.it">owner-fluka-discuss_at_mi.infn.it</a>
            [<a moz-do-not-send="true"
              href="mailto:owner-fluka-discuss_at_mi.infn.it">owner-fluka-discuss_at_mi.infn.it</a>]
            on behalf of Julian Rassolov [<a moz-do-not-send="true"
              href="mailto:julian.rassolov_at_gmail.com">julian.rassolov_at_gmail.com</a>]<br>
            Sent: 16 May 2011 19:50<br>
            To: <a moz-do-not-send="true"
              href="mailto:fluka-discuss_at_fluka.org">fluka-discuss_at_fluka.org</a><br>
            Subject: (n,gamma) interaction<br>
            <div>
              <div class="h5"><br>
                Good afternoon, everyone.<br>
                <br>
                I am facing some problem here, I need to track amount of
                the gamma-n<br>
                reaction that took place in some material. How is it
                possible to define?<br>
                <br>
                <br>
                Thank you in advance,<br>
                <br>
                &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; Julian.<br>
                <br>
                <br>
              </div>
            </div>
          </blockquote>
        </div>
        <br>
      </div>
    </blockquote>
    <br>
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