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19932000
most citedLarge Scale Structure and Supersymmetric Inflation without Fine Tuning

648 citations · 959 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph2000

Millimetric Ground Based Observation of CMBR Anisotropy at $δ=+28^{\lowercase{o}}$

G. Romeo, S. Ali, B. Femenia +4

Results from the third campaign of a ground-based multi-band observation of the millimeter emission of the sky from Tenerife (Canary Islands) are presented. The instrument consists…

hep-ph1996

The Cold Plus Hot Dark Matter Model From Supersymmetric Inflation

Qaisar Shafi, Robert K. Schaefer

The cold plus hot dark matter (CHDM) model is arguably the best theory we currently have for a consistent description of the observed large scale structure formation. This is espec…

astro-ph1996

An Efficient Technique for making maps from Observations of the Cosmic Microwave Background Radiation

L. Piccirillo, G. Romeo, R. K. Schaefer +1

We describe a new technique for turning scans of the microwave sky into intensity maps. The technique is based on a Fourier series analysis and is inspired by the lock-in deconvolu…

hep-ph1996★ 120 cited

Supersymmetric Inflation With Constraints on Superheavy Neutrino Masses

G. Lazarides, R. K. Schaefer, Q. Shafi

We consider a supersymmetric model of inflation in which the primordial density fluctuations are nearly scale invariant (the spectral index n is approximately 0.98) with amplitude…

astro-ph1996★ 12 cited

Study of the Correlations Between the Highest Energy Cosmic Ray Showers and Gamma Ray Bursts

Todor Stanev, Robert Schaefer, Alan Watson

We examine the correlation between the arrival direction of ultra high energy cosmic ray showers and gamma ray bursts in the third BATSE catalog. We find no correlation between the…

astro-ph1995★ 3 cited

Gauge Invariant Density and Temperature Perturbations in the Quasi-Newtonian Formulation

Robert K. Schaefer, Andrew A. de Laix

We give an improved formalism for calculating the evolution of density fluctuations and temperature perturbations in flat universes. Our equations are general enough to treat the p…