ar X iv : 1 50 3 . 00 35 4 v 1 [ gr - q c ] 1 M ar 2 01 5 Search for an emission line of a gravitational wave background

ar X iv : 0 70 4 . 33 68 v 2 [ gr - q c ] 2 6 A pr 2 00 7 Search for gravitational waves from binary inspirals in S 3 and S 4 LIGO data

ar X iv : 1 51 1 . 04 39 8 v 2 [ gr - q c ] 1 8 Fe b 20 16 All - sky search for long - duration gravitational wave transients with initial LIGO

Gravitatational Waves in G4v∗

Gravitational coupling of the propagation four-vectors of matter wave functions is formulated in flat space-time. Coupling at the momentum level rather than at the “force-law” level greatly simplifies many calculations. This locally Lorentz-invariant approach (G4v) treats electromagnetic and gravitational coupling on an equal footing. Classical mechanics emerges from the incoherent aggregation ...

ar X iv : 0 80 6 . 01 41 v 2 [ gr - q c ] 5 J an 2 00 9 Quantum induced ω = − 1 crossing of the quintessence and phantom models

Considering the single scalar field models of dark energy, i.e. the quintessence and phantom models, it is shown that the quantum effects can cause the system crosses the ω = −1 line. This phenomenon does not occur in classical level. The quantum effects are described via the account of conformal anomaly.

ar X iv : a st ro - p h / 01 03 43 8 v 1 2 7 M ar 2 00 1 X - rays and accretion discs as probes of the strong gravity of black holes

The observations and interpretation of broad iron lines in the X-ray spectra of Seyfert 1 galaxies are reviewed. The line profiles observed from MCG–6-30-15 and NGC 3516 show extended red wings to the line explained by large gravitational red-shifts. The results are consistent with the emission expected from an X-ray irradiated flat accretion disc orbiting very close to a black hole. Results fr...