[PDF] Top 20 Massive Gravitational Waves from Black Hole Inspirals in Quantum Gravity
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Massive Gravitational Waves from Black Hole Inspirals in Quantum Gravity
... the massive waves in the context of astrophysical processes, it is also possible to envisage the production of these new quantum gravitational massive classical modes during first order ... See full document
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Fundamental Physics Through Gravitational Waves: From No Hair Theorem to Quantum Structures of Black Holes
... suffer from a superradiant instability, although this instability can quenched by tuning the compactness and other parameters describing the ECO [89, ...suffer from nonlinear instabilities. While the ... See full document
175
Effect of the Dilaton Field on Deflection Angle of Massive Photons by Black Holes in Einstein-Maxwell-Dilaton-Axion Theory
... of quantum gravity and obviously the attributes of black holes (BHs) in string theory would be most ...differs from general relativity (GR) due to the existence of scalar field which is known ... See full document
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A status report on the phenomenology of black holes in loop quantum gravity: Evaporation, tunneling to white holes, dark matter and gravitational waves
... is massive, the quantum state after the jump is – in the global perspective – completely different from the initial ...different from the ones of the initial ...the quantum numbers for ... See full document
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Event horizons, gravitational waves and astrophysical kicks in black-hole spacetimes
... gravitational waves, and therefore the existence of gravitational waves, will be an additional proof in favor of the validity of General Relativity in the strong gravity ...of ... See full document
252
Gravitational Collapse of a Massive Star and Black Hole Formation
... the black hole ...of black holes cannot decrease, that is, A 0 . For Schwarzschild black hole, the only way to reduce this area is to extract mass from black ... See full document
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Quantum-gravitational trans-Planckian energy of a time-dependent black hole
... constraints among the classical modes - which is thus of “order-1” effect, and thereby qualitatively change the classical part of the solution. As the higher- order terms (that are not explicitly shown in (13)) are added ... See full document
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Search for gravitational waves from primordial black hole binary coalescences in the galactic halo
... days from February 14 to April 14, ...light from the two arms recombining at the beam splitter is strongly depen- dent on the difference between the lengths of the two ... See full document
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Gravitational radiation in infinite derivative gravity and connections to effective quantum gravity
... [44] Aindri Conroy. Infinite Derivative Gravity: A Ghost and Singularity-free Theory. PhD thesis, Lancaster U., 2017. [45] James Edholm and Aindriu Conroy. Criteria for re- solving the cosmological singularity in ... See full document
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GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
... Both of these waveform models are calibrated to partially overlapping sets of numerical-relativity simulations of binary black hole coalescences, following from the initial break- throughs reported ... See full document
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Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
... inating from instrumental noise so as to efficiently detect the gravitational wave signals (measured using simulated injec- tions, as described in Section III ...drawn from the full data ... See full document
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P V Criticality of a Modified BTZ Black Hole in 2 + 1 Dimensional Intrinsic Time Quantum Gravity
... In [3] a formulation of intrinsic time quantum geometrodynamics (ITQG) is presented, which is applicable to 3 + 1 dimensional spacetime. We would like to study an analogous 2 + 1 formulation corresponding to two ... See full document
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Visualizing, Approximating, and Understanding Black-Hole Binaries
... quasicircular black-hole binary as passing through three different stages: inspiral, merger, and ringdown (see, ...comparable-mass black holes, the three stages correspond to the times one can use ... See full document
424
Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data
... for black hole ringdowns in data from the fifth LIGO science run is currently ...sources from which a detection could be ...to black holes with masses up to 2000 M or ... See full document
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GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
... support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry ... See full document
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Probing Quantum Gravity through Strong Gravitational Lensing
... used gravitational lensing to explore its distribution in cluster ...the quantum state of space-time in the ambient of the baryonic ...of quantum gravity is that under certain critical ... See full document
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Surrogate Models of Gravitational Waves from Numerical Relativity Simulations of Binary Black Hole Mergers
... GWs from BBH mergers and other systems in the near ...of gravity that agree with GR in the weak field limit and agree with experiments to date can produce di ff erent GW signals from BBHs and other ... See full document
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GW151226 : observation of gravitational waves from a 22-solar-mass binary black hole coalescence
... parameters from the post-Newtonian approximation [26 – 28] and from fits to numerical relativity simulations) to deviate from their nominal values, and check whether the resulting waveforms are ... See full document
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Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals
... star–black hole (NS-BH) binaries (rather than BH-BH ...away from the main sequence, the more massive star would expand until it fills its Roche lobe before transferring mass to its ...more ... See full document
19
Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
... The background generated by the cosmic population of MB- HBs is present across the whole observational window of PTAs (cf. Paper I). The Monte Carlo simulations reported in Paper I clearly show the presence of ... See full document
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