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<event>
<ID>1743</ID>
<category>CAST Meetings</category>
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<announcer>
 <user>
  <title></title>
  <name first="Alan" middle="" last="Barr"></name>
  <organization>University of Oxford (GB)</organization>
  <email>alan.barr@cern.ch</email>
  <userid>19868</userid>
 </user>
</announcer>
<supportEmail caption="Support">zioutas@physics.upatras.gr</supportEmail>
<title>2nd Joint ILIAS-CAST-CERN axion Training Workshop 2006</title>
<description></description>
<participants></participants>
<closed>False</closed>
<location>
 <name>University of Patras</name>
 <address>University of Patras 
Rio, 26500 Patras 
Greece</address>
 <room>Conference Center</room>
</location>
<startDate>2006-05-18T09:00:00</startDate>
<endDate>2006-05-19T20:00:00</endDate>
<creationDate>2006-04-08T22:20:51</creationDate>
<modificationDate>2011-09-13T20:02:40</modificationDate>
<timezone>Europe/Zurich</timezone>
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 <ID>6</ID>
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 <title>Exotic Axion Cosmologies</title>
 <primaryAuthors>
  <user>
   <title></title>
   <name first="Kathryn" middle="" last="Zurek"></name>
   <organization>University of Washington Association</organization>
   <email>zurkat@u.washington.edu</email>
  </user>
 </primaryAuthors>
 <location>
  <name>University of Patras</name>
  <address>University of Patras 
Rio, 26500 Patras 
Greece</address>
  <room>Conference Center</room>
 </location>
 <startDate>2006-05-18T14:50:00</startDate>
 <endDate>2006-05-18T15:30:00</endDate>
 <duration>00:40</duration>
 <abstract>Kathryn Zurek 
University of Washington Association
zurkat@u.washington.edu</abstract>
 <material>
  <ID>0</ID>
  <title>Abstract</title>
  <description>We consider non-standard axion cosmologies in theories which exhibit a phase 
transition below the QCD scale.  In these theories, the cosmological upper bound on 
the axion decay constant is evaded.  There also result from this theory heavy (eV 
mass or higher) axion-like pseudoscalars which may be detectable.  We discuss 
implication for current axion detection experiments.</description>
  <type></type>
 </material>
</contribution>
<material>
 <ID>1</ID>
 <title>Abstract</title>
 <description>Due to their outstanding property to be storable and hence observable for long 
periods of time (several hundreds of seconds) in suitable material or magnetic 
traps, ultra-cold neutrons (UCN) with energies around 100 neV are an unique tool to 
study fundamental properties of the free neutron.
A brief introduction to the Institute Laue-Langevin (ILL) in Grenoble, France, 
which is a world leader in academic research with neutrons will be given. The scope 
of fundamental physics studies with neutrons is outlined. The main instruments 
provided for such studies are described and some past and current flagship 
experiments with ultra-cold neutrons (UCN) in this field (lifetime and quantum 
states) are highlighted. The properties and the production of UCN are described in 
detail.

For particles to have electric dipole moments, the forces concerned in their 
structure must be asymmetric with regard to space-parity (P) and time reversal (T). 
P violation is a well-known intrinsic feature of the weak interaction which is 
responsible for the beta-decay of the free neutron. T violation turns out to be 
necessary to explain the survival of matter at the expense of antimatter after the 
Big Bang. By searching for an EDM of the free neutron hypothetical new channels of 
T-violation can be investigated.
In this talk two EDM projects will be presented in detail, an experiment at room 
temperature that has recently been completed and a cryogenic experiment that is 
currently being constructed. The experiments are based on a precision measurement 
of the Larmor precession frequency of polarised ultracold neutrons stored in a cell 
in a magnetic field. An EDM would reveal itself by a response of the Larmor 
precession frequency of the neutron to an electric field applied over the storage 
volume.
The room temperature experiment has been carefully analysed. An upper limit on the 
absolute value of the neutron EDM of |dn| &lt; 3.0x10-26 e∙cm (90% CL) has been found 
(paper submitted to PRL, preprint hep-ex/0602020).
The two experiments at the ILL will be compared to competing EDM projects worldwide.</description>
 <type></type>
</material>
<material>
 <ID>0</ID>
 <title>Abstract</title>
 <description>In addition to the very well-known photon coupling, the coupling of axions to 
nucleons provides several interesting and experimentally accessible production 
channels.  Such axions can be classified as “high-energy” with respect to the much 
lower energy relic and Primakoff axions, with typical kinetic energies in the tens 
of MeV region.  For a helioscope experiment that relies on the axion-photon 
conversion, the high kinetic energy of these nuclear axions improves the coherence 
condition along the magnetic field length, thereby improving the conversion 
probability compared to that of Primakoff axions for a given axion mass.  During 
the 2004 Phase 1 run, the CAST calorimeter conducted the first helioscope search 
for high-energy axions.  I will introduce the production mechanisms of high-energy 
axions that are of interest in general and go through the modified axion-photon 
conversion probability and expected signal. I will then describe the CAST 
calorimeter and the results obtained.</description>
 <type></type>
</material>
<material>
 <ID>paper</ID>
 <title>Paper</title>
 <description></description>
 <type></type>
</material>
<material>
 <ID>poster</ID>
 <title>Poster</title>
 <description></description>
 <type></type>
</material>
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  <todayReference>2013-06-19</todayReference>
  <tomorrowReference>2013-06-20</tomorrowReference>
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