output
19952026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2009Show all

27 papers · 1 filter

math.DS2009★ 21 cited

The Ingram Conjecture

M. Barge, H. Bruin, S. Štimac

We prove the Ingram Conjecture, i.e., we show that the inverse limit spaces of every two tent maps with different slopes in the interval [1, 2] are non-homeomorphic. Based on the s…

astro-ph.CO2009★ 376 cited

An Upper Limit on the Stochastic Gravitational-Wave Background of Cosmological Origin

The LIGO Scientific Collaboration, the Virgo Collaboration

A stochastic background of gravitational waves is expected to arise from a superposition of a large number of unresolved gravitational-wave sources of astrophysical and cosmologica…

cond-mat.str-el2009★ 2 cited

Anisotropic In-Plane Strain and Transport in Epitaxial Nd(0.2)Sr(0.8)MnO(3) Thin Films

K. P. Neupane, J. J. Neumeier, J. L. Cohn

The structure, morphology, and electrical properties of epitaxial a-axis oriented thin films of Nd(0.2)Sr(0.8)MnO(3) are reported for thicknesses 10 nm <= t <= 150 nm. Films were g…

gr-qc2009★ 8 cited

Alternative derivation of the response of interferometric gravitational wave detectors

Neil J. Cornish

It has recently been pointed out by Finn that the long-standing derivation of the response of an interferometric gravitational wave detector contains several errors. Here I point o…

astro-ph.HE2009★ 272 cited

Indications of Proton-Dominated Cosmic Ray Composition above 1.6 EeV

R. U. Abbasi, T. Abu-Zayyad, M. Al-Seady +57

We report studies of ultra-high energy cosmic ray composition via analysis of depth of airshower maximum (Xmax), for airshower events collected by the High Resolution Fly's Eye (Hi…

astro-ph.SR2009★ 39 cited

Reconstructing the Local Twist of Coronal Magnetic Fields and the Three-Dimensional Shape of the Field Lines from Coronal Loops in EUV and X-Ray Images

A. Malanushenko, D. W. Longcope, D. E. McKenzie

Non-linear force-free fields are the most general case of force-free fields, but the hardest to model as well. There are numerous methods of computing such fields by extrapolating…