A precise determination of the primordial spectrum of matter density fluctuations at super-
horizon scales is essential in understanding large scale structure in the universe. Attempts to …

We implement and investigate a method for measuring departures from scale-invariance,
both scale-dependent as well as scale-free, in the primordial power spectrum of density …

The acoustic peak in the cosmic microwave background power spectrum is sensitive to
causal processes and cosmological parameters in the early universe up to the time of last …

A model-independent determination of the primordial power spectrum of matter density
fluctuations could uniquely probe physics of the very early universe and provide powerful …

We constrain the shape of the primordial power spectrum using recent measurements of the
cosmic microwave background (CMB) from the Wilkinson Microwave Anisotropy Probe …

We present a Bayesian analysis of large-scale structure (LSS) and cosmic microwave
background data to constrain the form of the primordial power spectrum. We have extended …

Measuring the deviation from scale invariance of the primordial power spectrum is a critical
test of inflation. In this paper we reconstruct the shape of the primordial power spectrum of …

The shape of the primordial fluctuation spectrum is probed by cosmic microwave
background fluctuations which measure density fluctuations at z∼ 1000 on scales of …

Current cosmological observations are remarkably consistent with a concordance
cosmology including an epoch of inflation in the very early universe. There is a tantalizing …

Cosmological theories for the origin and evolution of structure in the Universe are highly
predictive of the form of the angular power spectrum of cosmic microwave background …