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A. A. Shah

Researcher at Marshall Space Flight Center

Publications -  16
Citations -  12506

A. A. Shah is an academic researcher from Marshall Space Flight Center. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 15, co-authored 16 publications receiving 11227 citations. Previous affiliations of A. A. Shah include Rutherford Appleton Laboratory.

Papers
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The CMS experiment at the CERN LHC

S. Chatrchyan, +3175 more
TL;DR: The Compact Muon Solenoid (CMS) detector at the Large Hadron Collider (LHC) at CERN as mentioned in this paper was designed to study proton-proton (and lead-lead) collisions at a centre-of-mass energy of 14 TeV (5.5 TeV nucleon-nucleon) and at luminosities up to 10(34)cm(-2)s(-1)
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GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

B. P. Abbott, +1065 more
TL;DR: The magnitude of modifications to the gravitational-wave dispersion relation is constrain, the graviton mass is bound to m_{g}≤7.7×10^{-23} eV/c^{2} and null tests of general relativity are performed, finding that GW170104 is consistent with general relativity.
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CMS physics technical design report, volume II: Physics performance

G. L. Bayatian, +2063 more
- 01 Jun 2007 - 
TL;DR: In this article, the authors present a detailed analysis of the performance of the Large Hadron Collider (CMS) at 14 TeV and compare it with the state-of-the-art analytical tools.
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A gravitational-wave standard siren measurement of the Hubble constant

B. P. Abbott, +1322 more
- 02 Nov 2017 - 
TL;DR: A measurement of the Hubble constant is reported that combines the distance to the source inferred purely from the gravitational-wave signal with the recession velocity inferred from measurements of the redshift using the electromagnetic data.
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GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

B. P. Abbott, +1101 more
TL;DR: In this paper, the authors show that the signal waveform is consistent with the predictions of general relativity and verify that the signals from the merger of two stellar-mass black holes in the LIGO detectors are consistent with these predictions.