activity
20072013
most citedGravitational Wave Constraints on DBI Inflation

70 citations · 244 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2013★ 5 cited

Isocurvature Perturbations and Reheating in Multi-Field Inflation

Ian Huston, Adam J. Christopherson

Inflationary models involving more than one scalar field naturally produce isocurvature perturbations. However, while these are fairly well studied, less is known about their evolu…

astro-ph.CO2013★ 1 cited

Quantifying the behaviour of curvature perturbations near Horizon Crossing

Ellie Nalson, Adam J. Christopherson, Ian Huston +1

How much does the curvature perturbation change after it leaves the horizon, and when should one evaluate the power spectrum? To answer these questions we study single field inflat…

astro-ph.CO2012

The Evolution of Non-adiabatic Pressure Perturbations during Multi-field Inflation

Ian Huston, Adam J. Christopherson

Non-adiabatic pressure perturbations naturally occur in models of inflation consisting of more than one scalar field. The amount of non-adiabatic pressure present at the end of inf…

astro-ph.CO2012★ 25 cited

Large trispectrum in two-field slow-roll inflation

Joseph Elliston, Laila Alabidi, Ian Huston +2

We calculate the conditions required to produce a large local trispectrum during two-field slow-roll inflation. This is done by extending and simplifying the 'heatmap' approach dev…

astro-ph.CO2011★ 15 cited

Quantifying the behaviour of curvature perturbations during inflation

Ellie Nalson, Adam J. Christopherson, Ian Huston +1

How much does the curvature perturbation change after it leaves the horizon, and when should one evaluate the power spectrum? To answer these questions we study single field inflat…

astro-ph.CO2011★ 43 cited

Calculating Non-adiabatic Pressure Perturbations during Multi-field Inflation

Ian Huston, Adam J. Christopherson

Isocurvature perturbations naturally occur in models of inflation consisting of more than one scalar field. In this paper we calculate the spectrum of isocurvature perturbations ge…