63,560 research outputs found
Tight Bounds for Black Hole Search with Scattered Agents in Synchronous Rings
We study the problem of locating a particularly dangerous node, the so-called
black hole in a synchronous anonymous ring network with mobile agents. A black
hole is a harmful stationary process residing in a node of the network and
destroying destroys all mobile agents visiting that node without leaving any
trace. We consider the more challenging scenario when the agents are identical
and initially scattered within the network. Moreover, we solve the problem with
agents that have constant-sized memory and carry a constant number of identical
tokens, which can be placed at nodes of the network. In contrast, the only
known solutions for the case of scattered agents searching for a black hole,
use stronger models where the agents have non-constant memory, can write
messages in whiteboards located at nodes or are allowed to mark both the edges
and nodes of the network with tokens. This paper solves the problem for ring
networks containing a single black hole. We are interested in the minimum
resources (number of agents and tokens) necessary for locating all links
incident to the black hole. We present deterministic algorithms for ring
topologies and provide matching lower and upper bounds for the number of agents
and the number of tokens required for deterministic solutions to the black hole
search problem, in oriented or unoriented rings, using movable or unmovable
tokens
Data Analysis Challenges for the Einstein Telescope
The Einstein Telescope is a proposed third generation gravitational wave
detector that will operate in the region of 1 Hz to a few kHz. As well as the
inspiral of compact binaries composed of neutron stars or black holes, the
lower frequency cut-off of the detector will open the window to a number of new
sources. These will include the end stage of inspirals, plus merger and
ringdown of intermediate mass black holes, where the masses of the component
bodies are on the order of a few hundred solar masses. There is also the
possibility of observing intermediate mass ratio inspirals, where a stellar
mass compact object inspirals into a black hole which is a few hundred to a few
thousand times more massive. In this article, we investigate some of the data
analysis challenges for the Einstein Telescope such as the effects of increased
source number, the need for more accurate waveform models and the some of the
computational issues that a data analysis strategy might face.Comment: 18 pages, Invited review for Einstein Telescope special edition of
GR
Black Hole Search with Finite Automata Scattered in a Synchronous Torus
We consider the problem of locating a black hole in synchronous anonymous
networks using finite state agents. A black hole is a harmful node in the
network that destroys any agent visiting that node without leaving any trace.
The objective is to locate the black hole without destroying too many agents.
This is difficult to achieve when the agents are initially scattered in the
network and are unaware of the location of each other. Previous studies for
black hole search used more powerful models where the agents had non-constant
memory, were labelled with distinct identifiers and could either write messages
on the nodes of the network or mark the edges of the network. In contrast, we
solve the problem using a small team of finite-state agents each carrying a
constant number of identical tokens that could be placed on the nodes of the
network. Thus, all resources used in our algorithms are independent of the
network size. We restrict our attention to oriented torus networks and first
show that no finite team of finite state agents can solve the problem in such
networks, when the tokens are not movable. In case the agents are equipped with
movable tokens, we determine lower bounds on the number of agents and tokens
required for solving the problem in torus networks of arbitrary size. Further,
we present a deterministic solution to the black hole search problem for
oriented torus networks, using the minimum number of agents and tokens
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