<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns="http://purl.org/rss/1.0/" xmlns:dc="http://purl.org/dc/elements/1.1/">
  <channel rdf:about="http://hdl.handle.net/2289/3587">
    <title>DSpace Collection:</title>
    <link>http://hdl.handle.net/2289/3587</link>
    <description />
    <items>
      <rdf:Seq>
        <rdf:li rdf:resource="http://hdl.handle.net/2289/3589" />
        <rdf:li rdf:resource="http://hdl.handle.net/2289/3588" />
      </rdf:Seq>
    </items>
    <dc:date>2026-04-08T12:12:08Z</dc:date>
  </channel>
  <item rdf:about="http://hdl.handle.net/2289/3589">
    <title>General relativistic rotation effects in pulsar radiation</title>
    <link>http://hdl.handle.net/2289/3589</link>
    <description>Title: General relativistic rotation effects in pulsar radiation
Authors: Samuel, J.
Description: Open Access</description>
    <dc:date>2008-01-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2289/3588">
    <title>Dynamics of vibrated grains</title>
    <link>http://hdl.handle.net/2289/3588</link>
    <description>Title: Dynamics of vibrated grains
Authors: Dhar, Abhishek; Sinha, Supurna
Abstract: We study number density distribution and the behavior of time correlation&#xD;
functions in the density of grains for a quasi-two dimensional system of vibrated grains. We study the system at various packing fractions, from low&#xD;
to high. At low densities we recover usual gas like behavior, reflected in a&#xD;
Poissonian statistics for the number density distribution. At higher densities&#xD;
we notice effects like formation of cages of the kind that are seen in glass&#xD;
transition. We study these effects with a perspective of understanding the&#xD;
similarities and differences between an atomic fluid and a “scaled up fluid”&#xD;
like a vibrated granular system.
Description: Open Access</description>
    <dc:date>2004-10-06T00:00:00Z</dc:date>
  </item>
</rdf:RDF>

