The GWs from the S-stars revolving around the SMBH at Sgr A*

Abstract

A preliminary estimation of gravitational waves (GWs) from the extreme-mass-ratio-inspirals (EMRIs) system in the Galactic Centre (GC) is given for the 37 observed S-stars revolving around the supermassive black hole (SMBH) at Sagittarius (Sgr) A*. Within this century, the total strain of the gravitational waveform calculated from the post-Newtonian (PN) method with eccentricity is well below the current planned sensitivity of pulsar-timing-array (PTA). New technology might be required in order to extract GW signal from this EMRIs system for future PTA detections.

arXiv commentv1, 16 pages, 3 figures, 1 table, two columns; v2, reference added, numerical calculation improved, submitted to Phys.Rev.D

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