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G

G. Mueller

Researcher at RWTH Aachen University

Publications -  69
Citations -  5195

G. Mueller is an academic researcher from RWTH Aachen University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 36, co-authored 69 publications receiving 4496 citations.

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The Pierre Auger Cosmic Ray Observatory

A. Aab, +643 more
TL;DR: The Pierre Auger Observatory as mentioned in this paper, the world's largest cosmic ray observatory, has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km$^2$ sr yr.

Working Group Report: New Light Weakly Coupled Particles

TL;DR: A review of the physics motivation for dark sectors and the exciting opportunities for experimental exploration is provided in this article, where axions, which solve the strong CP problem and are an excellent dark matter candidate, and their generalization to axion-like particles.
Journal ArticleDOI

The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914

B. P. Abbott, +961 more
TL;DR: In this paper, the authors report on the constraints these observations place on the rate of binary black hole coalescences, and estimate a 90% credible range of merger rates between $2$--$53 \, \mathrm{Gpc}^{-3} \mathm{yr}^{ −1}$ (comoving frame).
Journal Article

Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

B. P. Abbott, +1101 more
TL;DR: The sensitivity of the LIGO network to transient gravitational-wave signals is estimated, and the capability of the network to determine the sky location of the source is studied, to facilitate planning for multi-messenger astronomy with gravitational waves.
Journal ArticleDOI

Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications

A. Aab, +484 more
- 31 Dec 2014 - 
TL;DR: In this article, the authors examined the implications of the distributions of the depths of atmospheric shower maximum (X-max) using a hybrid technique, for composition and hadronic interaction models, and found that their data are not well described by a mix of protons and iron nuclei over most of the energy range.