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Hi all,<br>
<br>
Reminder for tomorrow's EO meeting, last before the summer. Lutz is
the coordinator of supernova neutrino detection with IceCube, he is
spending his sabbatical in Uppsala and we are stealing him down for
a talk for the day.<br>
<br>
best,<br>
chad<br>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">Subject:
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<td>[Okc-wp4] Last EO meeting before summer on Thursday June
8th (13:00, KTH meeting room 5th floor)</td>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">Date: </th>
<td>Fri, 2 Jun 2017 09:13:32 +0000</td>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">From: </th>
<td>Francesco Taddia <a class="moz-txt-link-rfc2396E" href="mailto:francesco.taddia@astro.su.se"><francesco.taddia@astro.su.se></a></td>
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<th align="RIGHT" nowrap="nowrap" valign="BASELINE">To: </th>
<td><a class="moz-txt-link-abbreviated" href="mailto:Okc-wp4@fysik.su.se">Okc-wp4@fysik.su.se</a> <a class="moz-txt-link-rfc2396E" href="mailto:Okc-wp4@fysik.su.se"><Okc-wp4@fysik.su.se></a></td>
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Hi all,
<div class=""><br class="">
</div>
<div class="">next week we will have our last EO meeting before
summer.</div>
<div class=""><span style="background-color: rgb(255, 255, 255);"
class="">Lutz Köpke from University of Mainz will give a talk
titled: </span><span style="background-color: rgb(255, 255,
255);" class="">"The next galactic supernova with the IceCube
observatory</span>”<br style="background-color: rgb(255, 255,
255);" class="">
<br class="">
Here the abstract:</div>
<div class=""><br style="background-color: rgb(255, 255, 255);"
class="">
<span style="background-color: rgb(255, 255, 255);" class="">Core
collapse supernovae are expected to occur in our galaxy about
twice per century. As the inner region of the star cannot be
studied with electromagnetic probes, neutrinos provide unique
insights into the internal mechanisms in place during the core
collapse. With about 500.000 recorded O(10 MeV) neutrino
interactions for a supernova at the galactic center, IceCube
offers unrivaled statistical precision and will remain
competitive even when future neutrino detectors are realized.
The basic detection principle and simulations that address
selected particle and astrophysical aspects will be discussed.
As the signal is observed on top of a large dark rate
background, IceCube cannot resolve individual neutrino
interactions at these low energies to determine energy,
direction and the neutrino type. Investigations that help to
remedy this situation and joint measurements of various
neutrino and gravitational wave experiments will be
mentioned. </span></div>
<div class=""><br class="">
</div>
<div class="">cheers</div>
<div class=""><br class="">
</div>
<div class="">/Francesco<br style="background-color: rgb(255, 255,
255);" class="">
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<div style="orphans: 2; widows: 2;" class=""><font
class="Apple-style-span" face="Noteworthy">-------------------------------------------</font></div>
<div style="orphans: 2; widows: 2;" class=""><font
class="Apple-style-span" face="Noteworthy">Francesco
Taddia</font></div>
<div style="orphans: 2; widows: 2;" class=""><font
class="Apple-style-span" face="Noteworthy">Postdoctoral
Researcher</font></div>
<div style="orphans: 2; widows: 2;" class=""><font
class="Apple-style-span" face="Noteworthy">Department
of Astronomy</font></div>
<div style="orphans: 2; widows: 2;" class=""><font
class="Apple-style-span" face="Noteworthy">Stockholm
University, Sweden</font></div>
<div style="orphans: 2; widows: 2;" class=""><font
class="Apple-style-span" face="Noteworthy"><a
href="mailto:ftadd@astro.su.se" class=""
moz-do-not-send="true">ftadd@astro.su.se</a></font></div>
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