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      -------- Forwarded Message --------
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            <th valign="BASELINE" nowrap="nowrap" align="RIGHT">Subject:
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            <td>Fwd: GGI Tea Breaks - Keith Olive - Wed. November 17th -
              5:00PM CET</td>
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            <th valign="BASELINE" nowrap="nowrap" align="RIGHT">Date: </th>
            <td>Mon, 15 Nov 2021 11:14:26 +0100</td>
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            <th valign="BASELINE" nowrap="nowrap" align="RIGHT">From: </th>
            <td>Agustin Sabio Vera <a class="moz-txt-link-rfc2396E" href="mailto:a.sabio.vera@gmail.com"><a.sabio.vera@gmail.com></a></td>
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            <th valign="BASELINE" nowrap="nowrap" align="RIGHT">Reply-To:
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            <td>Agustin Sabio Vera <a class="moz-txt-link-rfc2396E" href="mailto:a.sabio.vera@gmail.com"><a.sabio.vera@gmail.com></a></td>
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            <th valign="BASELINE" nowrap="nowrap" align="RIGHT">To: </th>
            <td>Dept. & IFT @ UAM
              <a class="moz-txt-link-rfc2396E" href="mailto:joint-list-dept-ift-l@uam.es"><joint-list-dept-ift-l@uam.es></a></td>
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          <div dir="ltr" class="gmail_attr">---------- Forwarded message
            ---------<br>
            De: <strong class="gmail_sendername" dir="auto">GGI
              Secretariat</strong> <span dir="auto"><<a
                href="mailto:segreteriaggi@fi.infn.it"
                moz-do-not-send="true" class="moz-txt-link-freetext">segreteriaggi@fi.infn.it</a>></span><br>
            Date: lun, 15 nov 2021 a las 11:12<br>
            Subject: GGI Tea Breaks - Keith Olive - Wed. November 17th -
            5:00PM CET<br>
            To: <<a href="mailto:ggi.participants@lists.fi.infn.it"
              moz-do-not-send="true" class="moz-txt-link-freetext">ggi.participants@lists.fi.infn.it</a>>,
            <<a href="mailto:ggi.students@lists.fi.infn.it"
              moz-do-not-send="true" class="moz-txt-link-freetext">ggi.students@lists.fi.infn.it</a>><br>
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            <p>Dear all,<br>
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                                                          <p>we are
                                                          happy to
                                                          announce a new
                                                          Theory
                                                          Colloquium on
                                                          the theory of
                                                          fundamental
                                                          interactions
                                                          within the <b>GGI
                                                          Tea Breaks’</b> series.  <br>
                                                          It will take
                                                          place via Zoom
                                                          at: <a
                                                          href="https://infn-it.zoom.us/j/83324611205"
target="_blank" moz-do-not-send="true" class="moz-txt-link-freetext">https://infn-it.zoom.us/j/83324611205</a></p>
                                                          <p>on</p>
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                                                          <p><b>Wednesday
                                                          November 17th
                                                          </b>at<b> <u>5</u><u>:00
                                                          PM</u> </b>(CET)
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                                                          <p> and will
                                                          be given by </p>
                                                          <p><span
                                                          style="text-align:center;background-color:rgb(255,255,255)"><b>Keith
                                                          Olive
                                                          (University of
                                                          Minnesota)</b><span></span><span></span><b><br>
                                                          </b></span></p>
                                                          <p>He will
                                                          talk about <font><span
style="text-align:center;background-color:rgb(255,255,255)"><span><b> “Big
                                                          Bang
                                                          Nucleosynthesis
                                                          - Post Planck"</b></span></span></font></p>
                                                          <p
style="box-sizing:inherit;font-style:normal;font-variant-ligatures:normal;font-variant-caps:normal;font-weight:400;letter-spacing:normal;text-indent:0px;text-transform:none;white-space:normal;word-spacing:0px;text-align:justify"><strong
style="box-sizing:inherit">Abstract</strong></p>
                                                          Big bang
                                                          nucleosynthesis
                                                          provides a
                                                          window to the
                                                          physics of the
                                                          universe just
                                                          seconds after
                                                          the big bang.
                                                          Its
                                                          predictions of
                                                          the light
                                                          element
                                                          abundances of
                                                          D, 4He, and
                                                          7Li can be
                                                          compared with
                                                          observational
determinations. Over the last several years, significant progress has
                                                          been made in
                                                          the
                                                          determinations
                                                          of deuterium
                                                          and helium
                                                          abundances and
                                                          most
                                                          importantly
                                                          results from
                                                          Planck
                                                          measurements
                                                          of the
                                                          microwave
                                                          background
                                                          have provided
                                                          precise values
                                                          for the baryon
                                                          density of the
                                                          universe, a
                                                          key input used
                                                          in abundance
                                                          predictions.
                                                          Planck data is
                                                          combined with
                                                          BBN to test
                                                          the
                                                          consistency of
                                                          the Standard
                                                          Model. Recent
                                                          nuclear cross
                                                          section data
                                                          and its effect
                                                          on BBN
                                                          precision is
                                                          also
                                                          discussed.
                                                          These
                                                          predictions
                                                          are sensitive
                                                          to the
                                                          conditions
                                                          when the
                                                          temperature of
                                                          the universe
                                                          was ≈ MeV or ≈
                                                          10^10 K. Using
                                                          inputs from
                                                          the standard
                                                          model of
                                                          cosmology and
                                                          particle
                                                          physics yields
                                                          excellent
                                                          agreement
                                                          between theory
                                                          and
                                                          experiment.
                                                          Thus
                                                          deviations
                                                          from the
                                                          standard model
                                                          such as the
                                                          number of
                                                          particle
                                                          degrees of
                                                          freedom (often
                                                          parametrized
                                                          as the number
                                                          of neutrino
                                                          flavors) can
                                                          be tested.<br>
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                                                          <p
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                                                          space for
                                                          questions and
                                                          discussion
                                                          will be
                                                          allocated at
                                                          the end of the
                                                          TH Colloquium.
                                                           We have also
                                                          created an
                                                          online Q&A
                                                          space for each
                                                          seminar. You
                                                          can submit
                                                          your question
                                                          by filling
                                                          the <a
href="https://docs.google.com/forms/d/e/1FAIpQLSfskqHeUko1e_GxLng6fDquV4JANEZQARIa2m9YF_voyxs6JQ/viewform"
target="_blank" moz-do-not-send="true">form</a>. The answers will be
                                                          published soon
                                                          after.</p>
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                                                          <div>For more
                                                          info see  <a
                                                          href="https://www.ggi.infn.it/seminars"
target="_blank" moz-do-not-send="true" class="moz-txt-link-freetext">https://www.ggi.infn.it/seminars</a></div>
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                                                          <div>Please
                                                          forward this
                                                          announcement
                                                          to anyone who
                                                          might be
                                                          interested.</div>
                                                          <div>We wait
                                                          for your
                                                          participation,</div>
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                                                          </div>
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                                                          <p> The
                                                          Organising
                                                          Committee of
                                                          the GGI Tea
                                                          Breaks</p>
                                                          <p><br>
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