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Geometrical Measures of Non-Gaussianity Generated by Single Field Models of Inflation

  • Author / Creator
    Junaid, Muhammad
  • In this thesis we have compiled the study of geometrical non-Gaussianity generated by inflation along with necessary basics and background knowledge of inflationary universe. We effectively calculated the power spectrum and the bispectrum, as a measure of non-Gaussianity, using the approach laid by Maldacena. We developed a robust numerical technique to compute the bispectrum for different single field inflationary models that may even have some features in the inflationary potential. From the bispectrum, we evaluated the third order moments of scalar curvature perturbations in configuration space. We evaluate these moments analytically in the slow roll regime while we devised a numerical mechanism to calculated these moments even for non slow roll single field inflationary models with standard kinetic term that are minimally coupled to gravity. With help of these third order moments one can directly predict many non-Gaussian and geometrical measures of three dimensional distributions as well as two dimensional CMB maps in the configuration space. Thus, we have devised a framework to calculate geometrical measures, for example Minkowski functionals or skeleton statistic, generated by different single field models of inflation. Finally, we also calculated these configuration space moments for the two dimensional projection maps on the sky. We subtracted the monopole contribution of the two dimensional perturbation field from these moments so that we can estimate observable geometrical non-Gaussianity in CMB temperature maps generated by single field inflationary models.

  • Subjects / Keywords
  • Graduation date
    2015-11
  • Type of Item
    Thesis
  • Degree
    Doctor of Philosophy
  • DOI
    https://doi.org/10.7939/R30G8Q
  • License
    This thesis is made available by the University of Alberta Libraries with permission of the copyright owner solely for non-commercial purposes. This thesis, or any portion thereof, may not otherwise be copied or reproduced without the written consent of the copyright owner, except to the extent permitted by Canadian copyright law.
  • Language
    English
  • Institution
    University of Alberta
  • Degree level
    Doctoral
  • Department
    • Department of Physics
  • Supervisor / co-supervisor and their department(s)
    • Prof. Dmitri Pogosyan (Department of Physics) University of Alberta
  • Examining committee members and their departments
    • Richard Sydora (Department of Physics) University of Alberta
    • Alexander Penin (Department of Physics) University of Alberta
    • Valeri Frolov (Department of Physics) University of Alberta
    • Carlo Contaldi (Department of Physics) Imperial College London