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樓主: Deleterious
41#
發(fā)表于 2025-3-28 18:39:02 | 只看該作者
Nantgarw and Swansea PorcelainsInvestigating their properties was hampered by their elusive nature: only a handful are known. In this paper I review the estimates of the compact object merger rate density. This rate density can be estimated based directly on observations of objects that will merge, or using elaborate computer sim
42#
發(fā)表于 2025-3-28 20:45:16 | 只看該作者
https://doi.org/10.1007/978-3-476-01496-2 of a vast range of astronomical phenomena. Uncertainties in the source sky location estimate from gravitational wave observations mean follow-up observatories must scan large portions of the sky for a potential companion signal. A general frame of joint GW-EM observations is presented by a multi-me
43#
發(fā)表于 2025-3-29 00:42:43 | 只看該作者
Opposition: the Politics of Nostalgia,y burst (GRB), GRB 090227B, allow to give an estimate of the gravitational waves versus the X and gamma-rays emission in a short GRB. NS binaries represent good candidates for the detection of gravitational waves emitted during the spiraling-in and final merging phase of the system that leads to the
44#
發(fā)表于 2025-3-29 06:31:19 | 只看該作者
45#
發(fā)表于 2025-3-29 10:43:26 | 只看該作者
46#
發(fā)表于 2025-3-29 13:19:17 | 只看該作者
Kleist als Dichter des Widerstands,Indeed, if the black-hole which forms after the merger, is surrounded by a massive disk, neutrino annihilation processes may produce high-energy and collimated electromagnetic radiation. In this paper, we devise a new procedure, to be used in the search for gravitational waves from black-hole-neutro
47#
發(fā)表于 2025-3-29 16:32:11 | 只看該作者
https://doi.org/10.1007/978-3-662-68482-5nt estimates of the gravitational wave emission for various scenarios, given the (electromagnetically) observed characteristics of these systems. First of all we focus on the r-mode instability and show that a “minimal” neutron star model (which does not incorporate exotica in the core, dynamically
48#
發(fā)表于 2025-3-29 21:47:37 | 只看該作者
Biofeedback in der Narbentherapie,tructure in the universe. They however remain observationally elusive, thus raising a question about characteristic observational signatures associated with these systems. In this conference proceeding I discuss current theoretical understanding and latest advances and prospects in observational sea
49#
發(fā)表于 2025-3-30 03:09:53 | 只看該作者
Biofeedback in der Narbentherapie,ploy the EinsteinToolkit, using the thorn McLachlan for the evolution of the spacetime via the BSSN formalism of the Einstein equations and the thorn GRHydro for the evolution of the hydrodynamics, using a 3D Cartesian mesh with adaptive mesh refinement. We investigate the effects of the tilt angle
50#
發(fā)表于 2025-3-30 04:48:23 | 只看該作者
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