<?xml version="1.0" encoding="UTF-8"?>
<xml>
<records>
<record>
  <contributors>
    <authors>
      <author>ATLAS, Collaboration</author>
    </authors>
  </contributors>
  <titles>
    <title>Event display of a 4-muon candidate in the ATLAS detector</title>
    <secondary-title>Event display of a H -&gt; 4mu candidate event</secondary-title>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <keywords>
    <keyword>Higgs Candidates</keyword>
    <keyword>Proton Collisions</keyword>
    <keyword>Event Displays</keyword>
    <keyword>Physics</keyword>
    <keyword>ATLAS</keyword>
    <keyword>Muons</keyword>
  </keywords>
  <dates>
    <year>2012</year>
    <pub-dates>
      <date>2012</date>
    </pub-dates>
  </dates>
  <abstract>Event display of a 4mu candidate. EventNumber: 71902630 RunNumber: 204769 m_4l=125.1 GeV. m_12=86.3 GeV, m_34=31.6 GeV. mu_1: pt=36.1 GeV, eta=1.29, phi=1.33. mu_2: pt=47.5 GeV, eta=0.69, phi=-1.65. mu_3: pt=26.4 GeV, eta=0.47, phi=-2.51. mu_4: pt=71.7 GeV, eta=1.85, phi=1.65.</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Simulation astrophysic particle tools</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>part of http://www.ihep.ac.cn/~chep01/
&lt;br /&gt;
&lt;br /&gt;</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Planetary physics </title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>the Institute of Planetary Research carries out and supports research programs on the internal structure, formation and evolution of the planets, their moons, and asteroids and comets. Techniques employed include remote sensing and in-situ investigations using instruments carried on spacecraft, astronomical observations from the ground, theoretical modeling, and laboratory experiments. </abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Europlanet@DLR</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>planet resaerches by eu programs</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>astroparticle physics</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Presently the fields of astrophysics, cosmology, astroparticle and cosmic physics are going through 
&lt;br /&gt;a golden age characterized by fruitful interactions between laboratory experiments, direct 
&lt;br /&gt;observations of the Universe and simulations, which encourage continual and deep revisions of 
&lt;br /&gt;theories.</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Astroparticle: high energy gamma-rays, cosmic-rays and neutrino astrophysics</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Astroparticle: high energy gamma-rays, cosmic-rays and neutrino astrophysics</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Helmholtz Alliance for Astroparticle Physics</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Helmholtz Alliance for Astroparticle Physics</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Planetary Evolution and Life</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Planetary Evolution and Life</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>astroparticlephysics</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>https://indico.cern.ch/getFile.py/access?resId=0&amp;materialId=slides&amp;confId=34690+1-2</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>hadron colliders Lec.4</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>hadron colliders Lec.4
&lt;br /&gt;http://indico.cern.ch/getFile.py/access?resId=0&amp;materialId=slides&amp;confId=34710</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>exhibition “Universe of Particles”</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>dates and questions</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>cyclotron</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Seventy-five years after one of the world’s first working cyclotrons was handed to the London Science Museum,.....</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Smart Grid Interoperability  Standards</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>NIST used the following definitions for the key terms below: -p21</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>Ernest Lawrence</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>cyclotron as a first inquiry</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>smasher and colliders</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>smasher and colliders</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>accelerator science</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Here are a few areas where accelerator science has helped:
&lt;br /&gt;
&lt;br /&gt;Production of specific radio-isotopes. These can be used in medicine for PET (Positron emission tomography) scans.
&lt;br /&gt;Crystallography. Accelerators can be used to determine the spatial and chemical structure of molecules and even watch in real time changes to them.
&lt;br /&gt;Non-destructive imaging. This is useful when something fragile is being studied, eg. artworks and archaeology.
&lt;br /&gt;As a source of targeted radiation. For instance in hadron therapy as a method of treating cancer. Hadron therapy is far less destructive to surrounding tissue than radio therapy.</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>appeal3</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>https://indico.cern.ch/conferenceOtherViews.py?view=standard&amp;confId=190525
&lt;br /&gt;
&lt;br /&gt;appeal 3
&lt;br /&gt; 2012</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>enlight</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>ht</abstract>
</record>


</records>
</xml>