<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>Ellis, John</dc:creator>
  <dc:creator>García, Marcos A. G.</dc:creator>
  <dc:creator>Nagata, Natsumi</dc:creator>
  <dc:creator>Nanopoulos, Dimitri V.</dc:creator>
  <dc:creator>Olive, Keith A.</dc:creator>
  <dc:creator>Verner, Sarunas</dc:creator>
  <dc:date>2020</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">&lt;jats:p&gt; After reviewing the motivations for cosmological inflation formulated in the formalism of supersymmetry, we argue that the appropriate framework is that of no-scale supergravity. We then show how to construct within this framework inflationary models whose predictions for the tilt in the spectrum of scalar perturbations, [Formula: see text], and the ratio, [Formula: see text], of tensor and scalar perturbations coincide with those of the [Formula: see text] model of inflation proposed by Starobinsky. A more detailed study of no-scale supergravity reveals a structure that is closely related to that of [Formula: see text] modifications of the minimal Einstein–Hilbert action for general relativity, opening avenues for constructing no-scale de Sitter and anti-de Sitter models by combining pairs of Minkowski models, as well as generalizations of the original no-scale Starobinsky models of inflation. We then discuss the phenomenology of no-scale models of inflation, including inflaton decay and reheating, and then the construction of explicit scenarios based on SU(5), SO(10) and string-motivated flipped SU(5)×U(1) GUT models. The latter provides a possible model of almost everything below the Planck scale, including neutrino masses and oscillations, the cosmological baryon asymmetry and cold dark matter, as well as [Formula: see text] and [Formula: see text]. &lt;/jats:p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://sonar.ch/global/documents/86998</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1142/s0218271820300116</dc:relation>
  <dc:relation>info:eu-repo/semantics/altIdentifier/issn/0218-2718</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:source>International Journal of Modern Physics D. - World Scientific Pub Co Pte Lt. - 2020, p. 2030011</dc:source>
  <dc:subject xmlns:ns1="xml" ns1:lang="en">Space and Planetary Science</dc:subject>
  <dc:subject xmlns:ns2="xml" ns2:lang="en">Mathematical Physics</dc:subject>
  <dc:subject xmlns:ns3="xml" ns3:lang="en">Astronomy and Astrophysics</dc:subject>
  <dc:title xmlns:ns4="xml" ns4:lang="en">Building models of inflation in no-scale supergravity</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>
