Gravitational-wave Sources
PROPERTIES OF BINARY NEUTRON STARS AS GRAVITATIONAL WAVE SOURCES
... PROPERTIES OF BINARY NEUTRON STARS AS GRAVITATIONAL WAVE SOURCES.. Tauris (2018), Phys..[r] ...
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Modeling Gravitational-wave Sources for Pulsar Timing Arrays
... the gravitational wave sources that pulsar timing arrays can detect? Prior to LIGO’s detection of gravitational waves from a pair of merging black holes, the best evidence for the existence of ...
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Electromagnetic follow-up of gravitational wave sources and the case of GW150914
... from gravitational wave (GW) sources is a powerful tool to gain a complete understanding of the astrophysical event, as well as to support GW data ...GW sources detectable by the advanced LIGO ...
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Linking Optical and Infrared Observations with Gravitational Wave Sources Through Variability
... and gravitational signal strenghts suggests that we pay attention to being able to measure (in multiple filters) the transient OIR flux from bright ...fainter sources, smaller telescopes have been relegated ...
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Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
... main gravitational wave (GW) sources for pulsar timing arrays (PTAs); however, it is still unclear if the observed GW signal will be produced by a few single MBHBs, or if it will have the properties ...
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Relativistic Jets from Compact Binary Mergers as Electromagnetic Counterparts to Gravitational Wave Sources
... common, X-ray, optical, and radio transients, i.e. on-axis orphan afterglows (Dermer et al., 2000; Huang et al., 2002; Nakar & Piran, 2003; Rhoads, 2003; Cenko et al., 2013, 2015), would be more frequent than short GRBs. ...
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Null stream analysis of Pulsar Timing Array data: localisation of resolvable gravitational wave sources
... metric perturbation at the pulsar at the time of pulse emission and at the Earth at the time of pulse detection, respectively. Only the Earth term adds up coherently in the analysis of multiple pulsars in the array. ...
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LOW-Γ JETS from COMPACT STELLAR MERGERS: CANDIDATE ELECTROMAGNETIC COUNTERPARTS to GRAVITATIONAL WAVE SOURCES
... & Berger 2012; Nakar & Piran 2011; Gao et al. 2013; Kisaka, Ioka & Takami 2015). In this paper, we discuss the possibility that a significant fraction of compact stellar mergers result in the production of low−Γ jets (Γ ...
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LOW-Γ JETS from COMPACT STELLAR MERGERS: CANDIDATE ELECTROMAGNETIC COUNTERPARTS to GRAVITATIONAL WAVE SOURCES
... Rhoads 2003; Cenko et al. 2013, 2015 ), would be more frequent than short GRBs. Such low-frequency transients would accompany a good fraction of GW events and they allow for the accurate determination of the sky ...
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GRAVITATIONAL WAVE PHYSICS
... of gravitational waves As we have mentioned earlier, when the gravitational field is strong there are a number on nonlinear effects that influence the generation and propagation of gravi- tational ...of ...
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Topics in Gravitational Wave Physics
... detect gravitational waves, several fronts of theoretical research are presently being pursued, including second-generation detector design, data analysis, and numerical-relativity simulations of ...ground-based ...
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A dynamical gravitational wave source in a dense cluster
... Making use of a new N-body model to describe the evolution of a moderate-size globular cluster we in- vestigate the characteristics of the population of black holes within such a cluster. This model reaches core-collapse ...
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Model selection for gravitational-wave transient sources
... The aLIGO and AdVirgo detectors are designed to detect GWs of various astro- physical origin [70]. The non-Gaussian, non-stationary nature of advanced detector noise produces glitches, which affect the sensitivity of ...
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Characterization of low-significance gravitational-wave compact binary sources
... noise fluctuations can seriously impact the measurement of the chirp mass, since this is obtained by “following” the phase evolution of the waveform signal through thousands of cycles [101]. We get a (rough) ...
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The Three Ss of Gravitational Wave Astronomy: Sources, Signals, Searches
... Detection of EMRIs with LISA is difficult (in discussions of data analysis, we will generally use the term EMRIs to refer to both EMRIs and IMRIs since most of the discussion applies to both types of inspirals, except ...
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Squeezed light sources for current and future interferometric gravitational-wave detectors
... We have demonstrated an ultra-stable glass-based squeezed light source, the first experiment of this kind to operate under vacuum. The squeezer cavity is constructed quasi-monolithically, with optics and nonlinear ...
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Gravitational-Wave Science with the Laser Interferometer Gravitational-Wave Observatory
... the gravitational-wave science workflow after calibrating the data is searching the data for gravitational-wave ...of gravitational waves or set new upper limits on the rate of ...
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Gravitational Wave Universe
... disentangle seed formation models at the high-mass end of the seed spectrum probe the population of inspiralling MBHs in low-redshift dwarf galaxies pin down the physics of MBHB dynamics[r] ...
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Gravitational wave group
... Test mass of LCGT is connected to a cooling system by a heat link that possibly introduces mechanical noise. A suspension point interferometer (SPI) is introduced to maintain hig[r] ...
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Sound Wave as a Particular Case of the Gravitational Wave
... of gravitational field of the ...of gravitational filed became possible due to the fact that in the equation of the state of the atmosphere, considered to be an ideal gas, entropy s is taken into ...
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