BLACK HOLE SEARCH
Ping Pong in Dangerous Graphs: Optimal Black Hole Search with Pure Tokens
... A black hole is a node that destroys any incoming agent; no observable trace of such a destruction will be evident to the other ...the black hole is unknown to the agents. The Black ...
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Tight Bounds for Black Hole Search with Scattered Agents in Synchronous Rings
... so-called black hole in a synchronous anonymous ring network with mobile ...A black hole is a harmful stationary process residing in a node of the network and destroying destroys all mobile ...
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Ping Pong in Dangerous Graphs: Optimal Black Hole Search with Pebbles
... the black hole search problem in networks of arbitrary but known topology, the pebble model of agent interaction is compu- tationally as powerful as the whiteboard model; furthermore the complexity ...
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Hardness and Approximation Results for Black Hole Search in Arbitrary Networks
... Unité de recherche INRIA Sophia Antipolis 2004, route des Lucioles - BP 93 - 06902 Sophia Antipolis Cedex France Unité de recherche INRIA Futurs : Parc Club Orsay Université - ZAC des Vi[r] ...
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The basic physics of the binary black hole merger GW150914
... The paper is organized as follows: our presentation begins with the data output by the detectors. 2 Section 2 describes the properties of the signal read off the strain data, and how they determine the quantities ...
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Maxwell and Yang-Mills Equations on Curved Black Hole Space-Times
... theorem to T tµ , where T is the Maxwell energy momentum tensor, between two space-like hypersurfaces prescribed by t = constant leads to a conservation of energy that is at the level of a space integral of T tt . In ...
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Black-Hole Microstates in String Theory : Black is the Color but Smooth are the Geometries?
... in black-hole physics and in holographic renormalization group flows, singularities arise when one does not include the essential degrees of freedom needed to resolve ...resolve black-hole ...
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Our black hole
... Our universe is a black hole. The big bang, or the start of our universe is just the death of a heavy star. This means that our universe is surrounded by another one, and that all the black holes ...
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Nonlinear energy transfer to improve the acoustic black hole effect
... Nonlinear energy transfer to improve the acoustic black hole effect Haiqin Li ./,? , Viven Denis ` , Adrien Pelat , Franc¸ois Gautier and Cyril Touz´e ./ ./ IMSIA, ENSTA ParisTech-CNRS-EDF-CEA, ...
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Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run
... IMBHB search to data collected between July 2009 and October 2010 during the sixth LIGO science run (S6) and the second and third Virgo science run (VSR2 and ...same search algorithm and statistical ...
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AMUSE-VIRGO. II. DOWN-SIZING IN BLACK HOLE ACCRETION
... , a regime where the very existence of nuclear supermassive black holes (SMBHs) is debated. Out of 100 objects, 32 show a nuclear X-ray source, including 6 hybrid nuclei which also host a massive nuclear cluster ...
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ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914
... Abilene Christian University, Abilene, TX 79699, USA Received 2016 January 29; accepted 2016 February 3; published 2016 February 11 ABSTRACT The discovery of the gravitational-wave (GW) source GW150914 with the Advanced ...
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Cold, clumpy accretion onto an active supermassive black hole
... 35. Astropy Collaboration. Astropy: A community Python package for astron- omy. Astron. Astrophys. 558, A33 (2013). Acknowledgements This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00988.S. ALMA is a ...
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Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during their First and Second Observing Runs
... a search for eccentric BBH mergers with the coherent WaveBurst (cWB) algorithm that does not rely on binary system ...high-mass black holes. The search has been carried out over data from Advanced ...
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The basic physics of the binary black hole merger GW150914
... two black holes. The black holes were each of approximately 35 M , still orbited each other as close as ∼350 km apart and subsequently merged to form a single black ...these black holes were ...
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Sparse control of Hegselmann-Krause models: Black hole and declustering
... of black holes (where complete collapse to consensus is not avoidable), safety zones (where the control can keep the system far from clustering), basins of attraction (attractive zones around the clustering set) ...
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Binary Black Hole Mergers in the First Advanced LIGO Observing Run
... APPENDIX A: SEARCH DESCRIPTION In this appendix, we give further details of the two analyses, PyCBC and GstLAL, used in the search. Both analyses separately correlate the data from each detector with ...
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Binary Black Hole Mergers in the First Advanced LIGO Observing Run
... coalescence search detects both GW150914 and GW151226 with a significance of greater than ...heaviest black hole in GW150914 with a mass of ...lightest black hole of ...coalescing ...
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Accretion-ejection instability and QPO in black hole binaries I. Observations
... the black-body contri- bution exceeds half of the total (extrapolated to 50 keV), although we find that in general the radius values for the rejected points are more consistent than in GRO ...
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Immersed acoustic black hole as a travelling wave absorber: understanding artificial cochlear mechanics
... As the longitudinal mechanical coupling seems to be very low, the mammalian basilar membrane is often represented in literature with local mechanical impedance [11, 8]. Plate [10] or membrane [12] models are classically ...
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