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13th International Conference on Membrane Computing - MTA Sztaki

13th International Conference on Membrane Computing - MTA Sztaki

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M. Stannett<br />

The questi<strong>on</strong> arises, whether accelerating speed-up of this kind is physically<br />

feasible. Calude and Păun’s c<strong>on</strong>structi<strong>on</strong> was based <strong>on</strong> the observati<strong>on</strong><br />

that smaller is faster, but this analogy has obvious physical limitati<strong>on</strong>s (in any<br />

event, it is not the volume of reagents that matters, but their c<strong>on</strong>centrati<strong>on</strong>).<br />

N<strong>on</strong>etheless, a careful analysis of accelerating systems shows that certain cosmological<br />

implementati<strong>on</strong>s may indeed be possible. Our system clearly c<strong>on</strong>tains<br />

two agents: an observer A and a computing device B whose output is observed<br />

by A. Write t for the spacetime trajectory followed by B, and p for the point<br />

in spacetime at which A makes its observati<strong>on</strong>. For the system to be implementable,<br />

we require two things: t should be infinitely l<strong>on</strong>g from B’s point of<br />

view (to allow all instances of R(n) to be executed in the case they all return<br />

false); and it must be possible for a signal to be sent from any point <strong>on</strong> t to p. We<br />

call p a Malament-Hogarth (MH) event (Fig. 1). Perhaps surprisingly, sensible<br />

spacetimes c<strong>on</strong>taining MH-events (MH-spacetimes) can be defined, and their use<br />

[EN02] provides perhaps the most hopeful approach to dem<strong>on</strong>strating the feasibility<br />

of physical hypercomputati<strong>on</strong> since they are known to be associated with<br />

slowly rotating massive black holes of the kind c<strong>on</strong>sidered to have been observed<br />

experimentally at the centre of our own galaxy [G + 09]. It should n<strong>on</strong>etheless<br />

be noted that the suitability of such black holes for computati<strong>on</strong>al purposes is<br />

the subject of <strong>on</strong>going debate; it is as yet an open questi<strong>on</strong> whether other, less<br />

c<strong>on</strong>troversial, examples of physically relevant MH-spacetimes can be identified.<br />

A says "yes" if a note<br />

arrived, "no" if not<br />

A receives<br />

the note<br />

here, if <strong>on</strong>e<br />

was sent<br />

p<br />

If the program<br />

halts, B sends a<br />

note saying so<br />

B has infinite<br />

proper time available<br />

A sends the program<br />

to B, who runs it<br />

Does the following<br />

program ever halt?<br />

Fig. 1. Using Malament-Hogarth spacetime to solve the halting problem<br />

More complicated spacetime c<strong>on</strong>figurati<strong>on</strong>s (involving chains of MH-events)<br />

can be exploited to solve problems at all levels of the arithmetic hierarchy<br />

[Hog04], and this naturally raises the questi<strong>on</strong> whether accelerating P systems<br />

64

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