Examining the end of inflation with primordial black hole mass distribution and gravitational waves
A Ashoorioon, A Rostami, JT Firouzjaee - Physical Review D, 2021 - APS
We explicitly construct a double-field inflationary model, which satisfies the latest Planck
constraints at the cosmic microwave background (CMB) scales and produces the whole dark …
constraints at the cosmic microwave background (CMB) scales and produces the whole dark …
Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future -mode polarization measurements
Current and future B-mode polarization data are the most powerful observables to constrain
gravitational waves from the early Universe. We set conservative constraints on tensor …
gravitational waves from the early Universe. We set conservative constraints on tensor …
Note on single-field inflation and the swampland criteria
S Das - Physical Review D, 2019 - APS
The recently proposed swampland criteria aim to evade any (meta-) stable de Sitter
constructions within string landscapes, making it difficult to accommodate accelerating …
constructions within string landscapes, making it difficult to accommodate accelerating …
Single field inflation in the light of Pulsar Timing Array Data: quintessential interpretation of blue tilted tensor spectrum through Non-Bunch Davies initial condition
S Choudhury - The European Physical Journal C, 2024 - Springer
In this work, we present a quintessential interpretation of having a blue-tilted tensor power
spectrum for canonical single-field slow-roll inflation to explain the recently observed Pulsar …
spectrum for canonical single-field slow-roll inflation to explain the recently observed Pulsar …
[HTML][HTML] Rescuing single field inflation from the swampland
A Ashoorioon - Physics Letters B, 2019 - Elsevier
The difficulty of building metastable vacua in string theory, has led some to conjecture that in
the string theory landscape, potentials satisfy|∇ V/V|≥ c∼ O (1). This condition, which is …
the string theory landscape, potentials satisfy|∇ V/V|≥ c∼ O (1). This condition, which is …
Blue tensor spectrum from particle production during inflation
S Mukohyama, R Namba, M Peloso… - Journal of Cosmology …, 2014 - iopscience.iop.org
We discuss a mechanism of particle production during inflation that can result in a blue
gravitational wave (GW) spectrum, compatible with the BICEP2 result and with the r< 0.11 …
gravitational wave (GW) spectrum, compatible with the BICEP2 result and with the r< 0.11 …
Trans-Planckian censorship, inflation, and excited initial states for perturbations
S Brahma - Physical Review D, 2020 - APS
The recently proposed trans-Planckian censorship conjecture (TCC) seems to require that
the energy scale of inflation is significantly lower than the Planck scale (H inf< 10-20 M Pl) …
the energy scale of inflation is significantly lower than the Planck scale (H inf< 10-20 M Pl) …
Avoiding the string swampland in single-field inflation: Excited initial states
S Brahma, MW Hossain - Journal of High Energy Physics, 2019 - Springer
A bstract One class of single-field inflationary models compatible with the recently-
conjectured Swampland criteria would be those in which a Hubble slow-roll arameter ϵ H is …
conjectured Swampland criteria would be those in which a Hubble slow-roll arameter ϵ H is …
Imprints of primordial gravitational waves with non-Bunch-Davies initial states on CMB bispectra
S Akama, HWH Tahara - Physical Review D, 2023 - APS
It has been shown that both scalar and tensor modes with non-Bunch-Davies initial states
can enhance the amplitudes of the primordial bispectra compared to those with the Bunch …
can enhance the amplitudes of the primordial bispectra compared to those with the Bunch …
Beating the Lyth bound by parametric resonance during inflation
We propose a novel mechanism for enhancing primordial gravitational waves without
significantly affecting the curvature perturbations produced during inflation. This is achieved …
significantly affecting the curvature perturbations produced during inflation. This is achieved …