output
20022013
most citedFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

5.7k citations

Showing 2004Show all

73 papers · 1 filter

quant-ph200459 cited

Characterization of the non-classical nature of conditionally prepared single photons

Alfred B. U'Ren, Christine Silberhorn, Jonathan L. Ball +2

A reliable single photon source is a prerequisite for linear optical quantum computation and for secure quantum key distribution. A criterion yielding a conclusive test of the sing…

astro-ph20041 cited

Weak lensing measurements of dark matter halos of galaxies from COMBO-17

M. Kleinheinrich, P. Schneider, H. -W. Rix +8

We present a measurement of mass estimates for dark matter halos around galaxies from the COMBO-17 survey using weak gravitational lensing. COMBO-17 is particularly useful for this…

quant-ph2004

Encoding a qubit into multilevel subspaces

Matthew Grace, Constantin Brif, Herschel Rabitz +3

We present a formalism for encoding the logical basis of a qubit into subspaces of multiple physical levels. The need for this multilevel encoding arises naturally in situations wh…

cond-mat.mes-hall20045 cited

Zener quantum dot spin filter in a carbon nanotube

D. Gunlycke, J. H. Jefferson, S. W. D. Bailey +3

We predict and analyze a novel spin filter in semiconducting carbon nanotubes. By using local electrostatic gates, the conduction and valence bands can be modulated to form a doubl…

cond-mat.supr-con200437 cited

Universal scaling relations in molecular superconductors

F. L. Pratt, S. J. Blundell

Scaling relations between the superconducting transition temperature , the superfluid stiffness and the normal state conductivity are identi…

astro-ph200420 cited

The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: I. A Spatially Compact Lyman-alpha Emitting Galaxy at Redshift 5.721

Eduard Westra, D. Heath Jones, Chris E. Lidman +6

We report the spectroscopic confirmation of a compact \lya emitting galaxy at . A FORS2 spectrum of the source shows a strong asymmetric line with a flux of 5$\times10^{-1…