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    Hi everyone,<br>
    <br>
    just a short reminder that we'll have a journal club tomorrow at
    3:30 in the MOB theory room.<br>
    <br>
    See you there
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      <br>
      -------- Weitergeleitete Nachricht --------
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            <th valign="BASELINE" align="RIGHT" nowrap="nowrap">Betreff:
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            <td>[Isac-journal-club] Journal/Snack Club Wed 20th Sept
              3:30 MOB Theory Room</td>
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            <th valign="BASELINE" align="RIGHT" nowrap="nowrap">Datum: </th>
            <td>Thu, 7 Sep 2017 13:54:20 -0700</td>
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            <th valign="BASELINE" align="RIGHT" nowrap="nowrap">Von: </th>
            <td>Nir Nevo Dinur <a class="moz-txt-link-rfc2396E" href="mailto:nnevodinur@triumf.ca"><nnevodinur@triumf.ca></a></td>
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            <th valign="BASELINE" align="RIGHT" nowrap="nowrap">An: </th>
            <td><a class="moz-txt-link-abbreviated" href="mailto:isac-journal-club@trmail.triumf.ca">isac-journal-club@trmail.triumf.ca</a></td>
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      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif">Hi all,<br>
          <br>
          Nir Nevo Dinur will be presenting the attached THEORETICAL (be
          warned) paper</font></div>
      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif"><a moz-do-not-send="true"
href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.119.082501">https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.119.082501</a><br>
          <br>
          Don't worry, I'm not going to go into the details of the
          method (it's not in the paper...).<br>
          But one should probably also read Sec. 1 of the Supp. Mat.
          (also attached) to understand what is their starting point.<br>
          The main results which we'll discuss are Eqs. (1)-(3) and Fig.
          1<br>
          <br>
          For perspective and for the discussion, compare this work with
          Ref. [18] (and also [15,23]).<br>
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          <br>
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      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif">Questions:</font></div>
      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif"><br>
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      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif">1. What is so interesting/challenging in the 11Be
          spectrum?</font></div>
      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif">2. What are the important physics aspects included
          in the current method?<br>
          3. Do they get the physics right?<br>
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      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif">4. </font><font size="+1" face="Helvetica, Arial,
          sans-serif"><font size="+1" face="Helvetica, Arial,
            sans-serif">How, according to the authors, is the parity
            inversion in the 11Be nucleus similar to the Lamb shift in
            the hydrogen atomic spectrum?<br>
          </font></font><font size="+1" face="Helvetica, Arial,
          sans-serif"><font size="+1" face="Helvetica, Arial,
            sans-serif">5. </font>How would you assess this method and
          these results compared to those of Ref. [18]? What are the
          advantages and disadvantages, and possible uses of this
          method, in reference to current ab-initio calculations?
          (should we all quit?)<br>
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      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif"><br>
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      <div class="gmail_default"><font size="+1" face="Helvetica, Arial,
          sans-serif">See you all there.</font></div>
      <p> </p>
      <pre class="moz-signature" cols="72">-- 
Dr. Nir Nevo Dinur
Postdoctoral Fellow
Theory Group
Physical Sciences Div.
TRIUMF
4004 Wesbrook Mall,
Vancouver, BC V6T 2A3, Canada
+1-604-222-1047x6445</pre>
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