Author:

Engelhardt, Wolfgang

Category:

Communications

Sub-Category:

Gravity

Language:

English

Date Published:

July 1, 2016

File:

/Communications-Gravity/Download/6576

Downloads:

351

Keywords:

N/A

Abstract:

on Feb. 11, 2016 the LIGO-team published the paper PRL 116, 061102 (2016): Observation of Gravitational Waves from a Binary Black Hole Merger. The experimental proof for the existence of a gravitational wave was announced: Mirrors of 40 kg had been displaced by 10-18 m during fractions of a second as measured with a Michelson-interferometer with 4 km arm length resulting in a strain of 10-21. Scaling up these data by a factor of 1013 a relative accuracy must have been achieved by a hair’s breadth (10 microns) in relation to the distance to the next fixed star (4 light-years). This is by a factor of 1 Million better than the relative Mössbauer accuracy of 10-15 obtained so far. Indeed, Rudolf Mössbauer was awarded the Nobel Prize for physics in 1961 for this achievement

Help keep GS Journal progressing to become the most valuable scientific research website on the net!

View Profile