gravitational-wave emission
Upper limits on gravitational wave emission from 78 radio pulsars
... and gravitational wave ...the gravitational wave ...electromagnetic emission source wan- ders with respect to the mass quadrupole, could result from a weak exchange of angular momentum ...
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Beating the spin-down limit on gravitational wave emission from the crab pulsar
... on gravitational wave emission from the Crab pulsar using data from the first 9 months of the fifth science run of the Laser Interferometer Gravitational-wave Observatory ...the ...
7
The binary progenitors of short and long GRBs and their gravitational-wave emission
... cal accretion process onto the NS: if the accretion is sufficiently high the NS reaches the critical mass and collapses forming a BH, otherwise a massive NS is formed. Therefore long GRBs can lead either to NS-BH or to ...
10
Upper limits on gravitational wave emission from 78 radio pulsars
... the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO 600 gravitational wave ...the gravitational strain ...
20
Limits on Gravitational Wave Emission from Selected Pulsars Using LIGO Data
... generic source with a 1% false alarm rate and 10% false dis- missal rate, as given by Eq. (2.2) in [2] for single detector analyses and for a joint detector analysis. All the curves use typical S2 sensitivities and ...
6
Limits on gravitational-wave emission from selected pulsars using LIGO data
... expected gravitational- wave signal, which is twice the observed radio rotation ...Any gravitational signal in the data would show a residual time evolution reflecting the antenna pattern of the ...
6
Beating the spin-down limit on gravitational wave emission from the Vela pulsar
... In this paper we present the results of the analysis of Virgo VSR2 run data for the search of continuous GW signals from the Vela pulsar. The data have been analyzed using three largely independent methods and assuming ...
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Strong-field gravitational-wave emission in Schwarzschild and Kerr geometries: some general considerations
... energy emission occurs, ∆ E = ⌘m(m/M), where m and M are the particle and BH mass, with ⌘ ranging from ...the gravitational-wave energy and angular momentum flux at infinity, following the ...
5
Searches for gravitational waves from known pulsars at two harmonics in 2015–2017 LIGO data
... for gravitational waves from 222 pulsars with rotation frequencies 10 ...highest-sensitivity gravitational-wave data so far ...target emission from both the l = m = 2 mass quadrupole ...
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Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015 2017 LIGO Data
... for gravitational waves from 221 pulsars with rotation frequencies & 10 ...highest-sensitivity gravitational-wave data so far ...target emission from both the l = m = 2 mass quadrupole ...
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Stochastic Gravity and Ontological Quantum Mechanics
... continuous gravitational wave emission is very small in comparison to the normal energy exchange caused by thermal noise that a nucleus suffers in normal ...stochastic gravitational ...
6
Highly excited strings I: Generating function
... for gravitational wave emission from strings with cusps where the associated burst of radiation is highly anisotropic, and this ultimately provides one of the strongest signals in cosmic string ...
82
Data analysis infrastructure for gravitational wave astronomy
... a gravitational wave observatory’s location, orienta tion and sensitivity is ...to gravitational wave sources directly above or below the plane of the two (perpendicular) arms, there is ...
163
Quantum limited measurements in gravitational wave detectors
... travelling wave cavities is that the increased number of necessary optical elements increases the intra-cavity round trip loss. However, significant developments in the engineering of double resonant type designs ...
226
Improving the Performance and Sensitivity of Gravitational Wave Detectors
... the gravitational wave observatory Advanced LIGO, this system will study the behavior of metals in the elastic regime, far from the yield stress that would introduce plastic ...
139
Length Sensing and Control of a Prototype Advanced Interferometric Gravitational Wave Detector
... out. These measurements revealed the difficulty of accurately predicting these noise couplings, and will inform the choices of interferometer topology, readout technique, and most importantly, control scheme for future ...
235
Experiments with a laser interferometric gravitational wave antenna
... 136 A Test Mass Testing 139 B Principle of the Optical Phase Detection 144 C Burst and Coalescing Binary Sources 149 C.1 Short Bursts of Gravitational Radiation 149 C.2 Coalescing Compat[r] ...
185
Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory
... the gravitational-wave spectrum, based on the measurements of the CMB spectrum and pulsar ...stochastic gravitational- wave background is limited to the LIGO frequency ...
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Mitigating Noise in Interferometric Gravitational Wave Detectors
... in gravitational-wave detection [122] and scanning probe microscopy, optomechanical devices can also be used to probe the quantum behavior of mechanical ...interferometric gravitational wave ...
235
Topics in Gravitational Physics: Tidal Coupling in Gravitational Wave Searches and Mach’s Principle
... will be at frequencies close to the floor of the LISA noise curve (∼ 3 mHz). LISA will detect the bursts of radiation emitted near periapse throughout the inspiral, but these bursts will not be individually resolvable ...
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