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<p style="margin-top:0;margin-bottom:0">Thanks Takashi,</p>
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<p style="margin-top:0;margin-bottom:0">We'll start looking at these right away.</p>
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<p style="margin-top:0;margin-bottom:0">Norman</p>
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<div id="divRplyFwdMsg" dir="ltr"><font color="#000000" face="Calibri, sans-serif" style="font-size:11pt"><b>From:</b> Hps-analysis <hps-analysis-bounces@jlab.org> on behalf of Maruyama, Takashi <tvm@slac.stanford.edu><br>
<b>Sent:</b> Wednesday, May 1, 2019 11:54 AM<br>
<b>To:</b> hps-analysis@jlab.org<br>
<b>Subject:</b> [Hps-analysis] phi0 samples</font>
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<div class="PlainText">I tried generating phi0 using Fluka (See my presentation at the November Collaboration meeting). There are many problems in dealing with phi0 production in Fluka; how to scale for Tungsten, how to model phi0 production etc. Photo-production
seems to be more reliable than electro-production. I have generated some phi0 events and phi0-Kshort decays.
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stdhep files can be found under /nfs/slac/g/hps_data2/mc_production/phi0/ .<br>
phi0_all.stdhep: all K+/K- events<br>
phi0_select.stdhep: |Mass(K+K-) - 1.020| < 0.005 GeV<br>
kshort_all.stdhep: K+ or K- from phi0_all is replaced by Kshort, and K0->pi+/pi- (only pi+/pi- are saved)<br>
kshort_select.stdhep: K+ or K- from phi0_select is replaced by Kshort, and K0->pi+/pi- (only pi+/pi- are saved)<br>
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Takashi<br>
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