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Hi Beni, All,
<div><br>
</div>
<div>Thanks for the information about the crystals. I like the idea to replace some of the scintillators directly in the “production” microscope for the experiment if we’re convinced it will produce usable signals so that we don’t create a loss of acceptance
in some region of the tagger. We would learn more about the radiation hardness there than we would in the PS area.</div>
<div><br>
</div>
<div>A test setup in the PS area would have the advantage that it could be more flexible to evaluate different couplings procedures or other scintillator options which are more speculative, with easier access to adjust the geometry or setup without moving the
full microscope. If we have any spare material from the original scintillator from Saint-Gobain, we could also have a control sample to compare with (before radiation). </div>
<div><br>
</div>
<div>Maybe we want to do both of these tests in 2026?</div>
<div><br>
</div>
<div>-Justin<br id="lineBreakAtBeginningOfMessage">
<div><br>
<blockquote type="cite">
<div>On Oct 10, 2025, at 10:15 AM, zihlmann via Halld-tagger <halld-tagger@jlab.org> wrote:</div>
<br class="Apple-interchange-newline">
<div>
<div><font size="4" face="monospace">Hi All,<br>
<br>
regarding scintillator alternatives (proposed by Malte, Arshak, ...) I am investigating several paths to obtain LYSO crystals <br>
with 2mm by 2mm cross section and a length of 20mm or thereabouts. I think the length is not that important but the cross section <br>
is to fit the current geometry. I contacted two companies in the US and waiting responses. There is a company in China where one <br>
could buy online such crystals right away with a cost of 39$ per piece (excluding taxes and tarifs). So my hope is that we could <br>
get our hands on some such crystals on a rather short time scale.<br>
<br>
My basic idea is to equip the last "bundle" (most downstream), 3 columns with 5 scintillators each, with such crystals<br>
(the coupling has not yet been evaluated) till February and run with that in the next run period. If that is possible we would learn<br>
likely quite a lot about the usefulness of such crystals and hopefully a path forward to "upgrade" the full microscope.<br>
<br>
cheers,<br>
Beni <br>
</font><br>
<div class="moz-cite-prefix">On 10/10/25 08:36, Justin Stevens via Halld-tagger wrote:<br>
</div>
<blockquote type="cite" cite="mid:0840C242-5EDD-4244-8875-74F803C24016@jlab.org">
<div>Hi Richard, All,</div>
<div><br>
</div>
<div>Thanks for the summary of yesterday’s discussion and sorry I had to leave a bit early for the DNP practice talks. While we continue to investigate the exact reason for the loss of light yield, I suggest we begin planning a test that can be performed in
2026 to evaluate the options for potential replacement of the scintillating fibers before GlueX-III. </div>
<div><br>
</div>
<div>One possibility would be a small test setup on one of the PS arms with candidates for the 2x2 mm scintillators that can be tested with real signals from <span style="caret-color: rgb(0, 0, 0);">energy-tagged electrons. We would need </span>an equivalent
readout to the existing TAGM bundles, but most of the electronics infrastructure: f250 and f1TDC boards, crates, LV, etc. should already be available in that area for the PS/ST/TPOL readout. So, I believe we would need the TAGM preamp boards with SiPMs and
light guide fibers to couple to the candidate scintillators we want to evaluate. Do we have spares of those items that could be used for such a test starting in early 2026?</div>
<div><br>
</div>
<div>There is also the potentially more important question of what are the options for replacement scintillators with the appropriate shape that may be more radiation resistant and how can we test that radiation hardness? I understood from Malte that there
may be some LYSO crystals with an appropriate profile and Eljen <a href="https://eljentechnology.com/products/fibers" moz-do-not-send="true" class="moz-txt-link-freetext">https://eljentechnology.com/products/fibers</a> may have some appropriate fibers, but
we should consider procuring these and other options soon if we aim to test them next year.</div>
<div><br>
</div>
<div>More thoughts, suggestions, corrections are welcome. I just think we need to keep brainstorming on this to keep up the momentum towards finding a solution for GlueX-III.</div>
<div><br>
</div>
<div>-Justin</div>
<div><br>
<blockquote type="cite">
<div>On Oct 9, 2025, at 2:20 PM, Richard T. Jones via Halld-tagger <a class="moz-txt-link-rfc2396E" href="mailto:halld-tagger@jlab.org">
<halld-tagger@jlab.org></a> wrote:</div>
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<div>
<div dir="ltr">Hello all,
<div><br>
</div>
<div>We had a special meeting this morning at 10:00 devoted to a review of everything we know regarding the degrading response of the tagger microscope over the last few run periods. A new logbook entry has been added containing a historical record of the photon
yield and other calibration constants for the TAGM which presents clear evidence of significant loss of scintillation photon yields over the past 5 years, with most of the loss occurring in the rows that saw the greatest flux of electrons.</div>
<div>
<ul>
<li><a href="https://logbooks.jlab.org/entry/4459304" class="gmail-logtitle" style="color:rgb(143,106,175);font-family:"Trebuchet MS","Helvetica Neue",Arial,Helvetica,sans-serif;font-size:14px;background-color:rgb(245,245,245)" moz-do-not-send="true">gain and
photon yield history of the tagger microscope</a></li></ul>
<div>Ideas to further investigate the exact reasons for the decrease, as well as ideas for recovering and sustaining good performance during Phase 3 running are still in process, with follow-up to happen in the next Photon Beam working group mtg next week.</div>
</div>
<div><br>
</div>
<div>-Richard Jones</div>
</div>
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