AIP Conference Proceedings 2009
DOI: 10.1063/1.3183425
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Preparation and optical characterization of PbS quantum dots

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“…To this end I have shown the behaviour of theoretical CMB B mode polarization power spectra for low and high scale inflection point models of inflation within 10 −29 ≤ r 0.002 ≤ 0.12, which is also consistent with the upper bound of tensorto-scalar ratio obtained from Planck data. Further my aim is to carry forward this work in a more broader sense where I will extract the contribution from gravitational lensing and non-Gaussian contribution from the primordial magnetic field from the generic sub-Planckian inflationary setup expected to be reported shortly [42].…”
Section: Power Spectra From Faraday Rotation Angle Cmb Bb Angular Powmentioning
confidence: 99%
“…To this end I have shown the behaviour of theoretical CMB B mode polarization power spectra for low and high scale inflection point models of inflation within 10 −29 ≤ r 0.002 ≤ 0.12, which is also consistent with the upper bound of tensorto-scalar ratio obtained from Planck data. Further my aim is to carry forward this work in a more broader sense where I will extract the contribution from gravitational lensing and non-Gaussian contribution from the primordial magnetic field from the generic sub-Planckian inflationary setup expected to be reported shortly [42].…”
Section: Power Spectra From Faraday Rotation Angle Cmb Bb Angular Powmentioning
confidence: 99%