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  <responseDate>2026-08-25T20:03:58Z</responseDate>
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        <identifier>oai:meral.edu.mm:recid/2969</identifier>
        <datestamp>2021-12-13T08:03:49Z</datestamp>
        <setSpec>1582963492007:1595850252716</setSpec>
        <setSpec>user-yuoe</setSpec>
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      <metadata>
        <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns="http://www.w3.org/2001/XMLSchema" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
          <dc:title>Naked Singularity and Black Hole in Self-Similar Spacetimes</dc:title>
          <dc:creator>Htwe Nwe Oo</dc:creator>
          <dc:description>Attempts are made to give a clear description of self-similar spacetimes,
which is proving to be very useful in astrophysics and general relativity. We
have attempted to study the nature of naked singularity and black hole,
which are also likely to take place in self-similar spacetimes. The metric for
collapsing dust cloud is utilized in this formalism. Mathematica was used to
compute the details of the formalism and to visualize the graphics.</dc:description>
          <dc:date>2008-01-10</dc:date>
          <dc:identifier>http://hdl.handle.net/20.500.12678/0000002969</dc:identifier>
          <dc:identifier>https://meral.edu.mm/records/2969</dc:identifier>
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