<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:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>ÁLVAREZ, ENRIQUE</dc:creator>
  <dc:creator>ORTÍN, TOMÁS</dc:creator>
  <dc:date>2011</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">&lt;jats:p&gt; The asymptotic form of the density of states for a p-brane is computed (using the semi-classical approximation for the expression of the mass formula), and a value is found which only resembles the exponential growth of black holes in the formal limit p → ∞. Some physical consequences for the thermodynamics of these objects are also presented. &lt;/jats:p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://sonar.ch/global/documents/256718</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1142/s0217732392002251</dc:relation>
  <dc:relation>info:eu-repo/semantics/altIdentifier/issn/0217-7323</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:source>Modern Physics Letters A. - World Scientific Pub Co Pte Lt. - 1992, vol. 07, no. 31, p. 2889-2893</dc:source>
  <dc:subject xmlns:ns1="xml" ns1:lang="en">Nuclear and High Energy Physics</dc:subject>
  <dc:subject xmlns:ns2="xml" ns2:lang="en">Astronomy and Astrophysics</dc:subject>
  <dc:title xmlns:ns3="xml" ns3:lang="en">ASYMPTOTIC DENSITY OF STATES OF p-BRANES</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>