[PDF] Top 20 Gravitomagnetism and Angular Momenta of Black-Holes
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Gravitomagnetism and Angular Momenta of Black-Holes
... dependence of the gravitation and electric interactions, as characterized by Newton’s law of gravitation, and Coulomb’s law for electric charges, we would have on a par the equal contributions ... See full document
5
Evolution of binary black holes in self gravitating discs: Dissecting the torques
... understanding of the interplay between BHBs and their dense (stellar and gaseous) environment is required to predict ro- bust signatures that may allow their ...stages of BHB evolution: (i) ... See full document
13
A study of optical and radio properties of radio-loud AGN
... galaxies and double-double radio galaxies (DDRGs) have a common origin ...Merritt and Ekers, 2002; Liu et al., 2003; Liu, 2004). The symmetry of DDRG strongly suggests the interruption of the ... See full document
124
Massive black hole binary mergers within subparsec scale gas discs
... in black hole merg- ers, the results presented here suggest that geometrically thin gas discs could in principle drive mergers on a short enough time-scale for relatively low-mass black holes at low ... See full document
10
Structural aspects of asymptotically safe black holes
... typical momenta are of the order ...effect of scale-dependent coupling constants either at the level of the classical solutions, classical equations of motion, or the Lagrangian density ... See full document
25
Constant curvature black holes in Einstein AdS gravity: Conserved quantities
... BTZ black hole possesses constant curva- ture, and therefore it is locally indistinguishable from global AdS ...structure of the spacetime is modified [2]. In particular, mass and ... See full document
11
A Cardy-like formula for rotating black holes with planar horizon
... spite of the fact that the Cardy-like formula ...anisotropic black hole solutions are not known in the ...1, and hence the usual trick of performing a Lorentz boost to the static solution may ... See full document
26
Energy and Angular Momentum of Dilaton Black Holes
... Astrophysical black holes appear in a wide variety of ...result of stellar evolution (X-ray binaries, supernovas, collapsars, etc.), and also some of intermediate mass or ... See full document
7
On the Prevalence of Supermassive Black Holes over Cosmic Time
... Some of the prediction variance is likely due to the broad redshift range of the LBG selection (Δ z ≈ ...use of Lyman-alpha emitters ( LAEs ) to complement LBGs ...( and sometimes ... See full document
10
Sub dominant modes of the gravitational radiation from compact binary coalescences: construction of hybrid waveforms and impact on gravitational wave searches
... computation of the waveform describing the GW emission during the whole coalescence requires taking into account further effects like the energy loss via GW, the flux of energy through the event horizons ... See full document
173
A note on the Cardy formula and black holes in 3D (massive) bigravity
... strengths of both Newton’s ...derivatives of the metric ...family of theories include the recently much studied case of massive gravity ... See full document
7
Geometrization of integrable systems with application to holography.
... Furthermore, and noteworthy, the dynamics of this class of integrable systems can be equiv- alently understood in terms of Riemannian ...set of boundary conditions, so that in the ... See full document
128
The origin of the atomic and molecular gas contents of early type galaxies II Misaligned gas accretion
... driver of the variation in this percentage is the adopted dynamical friction ...mergers and consequently a lower merger rate at z = 0, leading to the 11 per cent figure referred to ...models of Lagos ... See full document
18
Following up the First Detection of Gravitational Waves with Numerical Relativity Simulations
... set of equations that carry information about the spatial structure for a given initial ...space and time is made and the whole set of coordinates is treated the same way, a formalism to ... See full document
94
New observational constraints on the growth of the First Supermassive Black Holes
... redshift of such heavy obscurations is certainly possible ...energies of ∼ 30 keV, at the peak of the AGN X-ray emission, even for heavily obscured ...models and expectations, will still ... See full document
9
Weighhing the black holes in z 2 submillimeter emitting galaxies hosting active galactic nuclei
... 2004) and Stevens et ...evolution of SMGs ...the black hole have started to remove gas and dust from the nucleus and the host galaxy (as suggested by most models; ...consequence ... See full document
14
4D higher spin black holes with nonlinear scalar fluctuations
... class of Frobenius-Chern-Simons theories [108], that in their turn can be embedded into a broader class of models based on homotopy associative ...structure of the base manifold, it arises naturally ... See full document
74
Holes of paper
... a continuació presentem un conjunt d’autors molt representatius en la búsqueda d’un llen- guatge visual gràfic lligat als continguts dels seus llibres.. el conjunt de l’obra de cada au[r] ... See full document
56
Exact black hole solution for scale dependent gravitational couplings and the corresponding coupling flow
... qualitative and quantitative agreement between the actual ERG result and the black hole induced results, one is tempted to believe that the solution (4, 5, and 6) is actually a selfconsistent ... See full document
15
Evidence of Supermassive Black Holes in Narrow Emission Line Galaxies
... 1987), and different classifi- cation criteria (Kewley et ...fraction of these NELGs were found to have spectra consistent with that of an AGN, al- though they do not show lines as broad as the Sy1 ... See full document
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