Petri net

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A Petri net (also known as a place/transition net or P/T net) is one of several mathematical representations of discrete distributed systems. As a modeling language, it graphically depicts the structure of a distributed system as a directed bipartite graph with annotations. As such, a Petri net has place nodes, transition nodes, and directed arcs connecting places with transitions. Petri nets were invented in 1962 by Carl Adam Petri.

(a) Petri net trajectory example
(a) Petri net trajectory example

Contents

[edit] Basic Petri nets

A Petri net consists of places, transitions, and directed arcs. Arcs run between places and transitions—not between places and places or transitions and transitions. The places from which an arc runs to a transition are called the input places of the transition; the places to which arcs run from a transition are called the output places of the transition.

Places may contain any number of tokens. A distribution of tokens over the places of a net is called a marking. Transitions act on input tokens by a process known as firing. A transition is enabled if it can fire, i.e., there are tokens in every input place. When a transition fires, it consumes the tokens from its input places, performs some processing task, and places a specified number of tokens into each of its output places. It does this atomically, i.e., in one non-interruptible step.

Execution of Petri nets is nondeterministic. This means two things:

  1. multiple transitions can be enabled at the same time, any one of which can fire
  2. none are required to fire — they fire at will, between time 0 and infinity, or not at all (i.e. it is totally possible that nothing fires at all).

Since firing is nondeterministic, Petri nets are well suited for modeling the concurrent behavior of distributed systems.

[edit] A formal definition

A Petri net is a 5-tuple (S,T,F,M_0,W)\!, where (see Desel and Juhás[1])

  • S is a set of places.
  • T is a set of transitions.
  • S and T are disjoint, i.e. no object can be both a place and a transition
  • F is a set of arcs known as a flow relation. The set F is subject to the constraint that no arc may connect two places or two transitions, or more formally: F \subseteq (S \times T) \cup (T \times S).
  • M_0 : S \to \mathbb{N} is an initial marking, where for each place s \in S, there are n_s \in \mathbb{N} tokens.
  • W : F \to \mathbb{N^+} is a set of arc weights, which assigns to each arc f \in F some n \in \mathbb{N^+} denoting how many tokens are consumed from a place by a transition, or alternatively, how many tokens are produced by a transition and put into each place.

A variety of other formal definitions exist. Some definitions do not have arc weights, but they allow multiple arcs between the same place and transition, which is conceptually equal to one arc with a weight of more than one.

[edit] Basic mathematical properties

The state of a Petri net can be represented as an M vector, where the 1st value of the vector is the number of tokens in the 1st place of the net, the 2nd is the number of tokens in the 2nd place, and so on. Such a representation fully describes the state of a Petri net.

A state-transition list, \vec \sigma = \langle M_{i_0} t_{i_1} M_{i_1} \ldots t_{i_n} M_{i_n} \rangle, which can be shortened to simply \vec \sigma = \langle t_{i_1} \ldots t_{i_n} \rangle is called a firing sequence if each and every transition satisfies the firing criteria (i.e. there are enough tokens in the input for every transition). In this case, the state-transition list of \langle M_{i_0} M_{i_1} \ldots M_{i_n} \rangle is called a trajectory, and M_{i_n} is called reachable from M_{i_0} through the firing sequence of \vec \sigma. Mathematically written: M_{i_0} [ \vec \sigma > M_{i_n}. The set of all firing sequences that can be reached from a net N and an initial marking M0 are noted as L(N,M0).

The state-transition matrix W is | S | by | T | large, and represents the number of tokens taken by each transition from each place. Similarly, W + represents the number of tokens given by each transition to each place. The sum of the two, W = W +W can be used for calculating the above mentioned equation of M_{i_0} [ \vec \sigma > M_{i_n} which can now be simply written as M_0 - M_n = W^T \cdot \sigma, where σ is a vector of how many times each transition fired in the sequence. Note that just because the equation can be satisfied, does not mean that it can actually be carried out - for that there should be enough tokens for each transition to fire, i.e. the satisfiability of the equation is required but not sufficient to say that state Mn can be reached from state M0.

(b) Petri net Example
(b) Petri net Example

W^{+}=\begin{bmatrix} * & t1 & t2 \\ p1 & 0  & 1 \\ p2 & 1 & 0 \\ p3 & 1& 0 \\ p4 & 0 & 1 \end{bmatrix}

 W^{-}=\begin{bmatrix} * & t1 & t2 \\ p1 & 1  & 0 \\ p2 & 0 & 1 \\ p3 & 0 & 1 \\ p4 & 0 & 0 \end{bmatrix}

W=\begin{bmatrix} * & t1 & t2 \\ p1 & -1  & 1 \\ p2 & 1 & -1 \\ p3 & 1 & -1 \\ p4 & 0 & 1 \end{bmatrix}

M_{0}=\begin{bmatrix} 1 & 0 & 2 & 1 \end{bmatrix}

[edit] Reachability

All states that can be reached from a net N with an initial marking M0 are denoted as R(N,M0). The reachability problem is then the following: is it true that M_{w} \in  R(N,M_{0}) where Mw is, for example, an erroneous state.

The reachability of a petri net's states can be represented with a reachability graph, a directed graph whose points represent states (i.e. M) and arcs represent transitions between two such states. The graph is constructed through breadth-first search as follows: the starting state (M0) is taken, and all possible transitions are explored from this state, then the transitions from these states, and so on. As the reachability graph may be infinitely large, breadth-first search is preferred because depth-first search would not find all possible states even if given infinite time.

While reachability seems to a be a good tool to find erroneous states, for practical problems the constructed graph usually has far too many states to calculate. To alleviate this problem, linear temporal logic is usually used in conjunction with the tableau method to prove that such states cannot be reached. LTL uses the semi-decision technique to find if indeed a state can be reached, by finding a set of necessary conditions for the state to be reached then proving that those conditions cannot be satisfied.

Reachability is known to be decidable, in at least exponential time. All known general algorithms so far, however, employ non-primitive recursive space [2].

[edit] Liveness

Petri nets can be described as having different levels of liveness L0L4. While the levels of liveness are defined on transitions within the Petri net, the Petri net itself is considered Lk live if and only if every transition within it is Lk live.

A Petri net (N,M0)'s transition t is

  • L0 live, or dead, if and only if it can not be fired, i.e. it is not in any firing sequence \vec \sigma where \vec \sigma  \in L(N,M_0)
  • L1 live if and only if it can possibly be fired, i.e. it is in a firing sequence \vec \sigma where \vec \sigma \in L(N,M_0)
  • L2 live if and only if for any k positive whole number, t can be fired at least k times in a firing sequence \vec \sigma where \vec \sigma \in L(N,M_0)
  • L3 live if and only if there exists a firing sequence \vec \sigma \in L(N,M_0) where t is fired infinitely
  • L4 live or simply live if and only if in any reachable state M (i.e. \forall M \in R(N,M_0)), t is L1 live

Note that these are increasingly stringent requirements such that if a transition is L3 live for example, it is automatically L1 and L2 live as well. As an example, (b) Example Petri net is live with the given initial state, but with a different (e.g. totally empty) initial state, all of its transitions are dead.

In computer programming and other applications, the property of liveness of a Petri net is used to model that the system can never lock up.

[edit] Boundedness

Reachability graph of (a) Petri net Example if the net is 2-bounded. In this case, it can only have a maximum of 9 (or 32) states.
Reachability graph of (a) Petri net Example if the net is 2-bounded. In this case, it can only have a maximum of 9 (or 32) states.

A Petri net is inherently k-bounded if in no reachable state can at any place contain more than k tokens. A Petri net is safe if it is 1-bounded. Naturally, the initial M0 marking is also restricted by the boundedness. Note that a Petri net is inherently bounded if and only if all its reachability graphs (i.e reachability graphs with all possible starting states) all have a finite number of states.

Formally, K : S \to \mathbb{N^+} is a set of capacity restrictions, which assigns to each place s \in S some positive number n \in \mathbb{N^+} denoting the maximum number of tokens that can occupy that place. A net in which each of its places has some capacity k, is known as an 'inherently k-bounded' Petri net.

Boundedness is decidable by looking at covering, by constructing the Karp-Miller Tree. In computer programming and other applications, the property of boundedness of a Petri net is used to model limits on available system resources such as CPUs and I/O buses.

Example place-transformation. The grey place that was originally inherently 2-bounded has been transformed into two places: a grey original, and a counter place
Example place-transformation. The grey place that was originally inherently 2-bounded has been transformed into two places: a grey original, and a counter place

Boundedness of a certain place in an inherently bounded net can be mimicked in a non-inherently bounded net by doing a place-transformation, where a new place (called counter-place) is created, and all transitions that put x tokens to the original place take x tokens from the counter-place, and all transitions that take away x tokens from the original place put x tokens to the counter-place. The number of tokens in M0 must now satisfy the equation place+counter-place=boundedness. Thus, doing a place-transformation for all places in a bounded net, and restricting the starting state M0 to conform to the above noted equality, a bounded net can easily be transformed to a non-bounded net. Therefore any analysis that is used on inherently non-bounded nets can be used on bounded nets (but not the other way around).

[edit] Extensions

There are many extensions to Petri nets. Some of them are completely backwards-compatible (e.g. coloured Petri nets) with the original Petri net, some add properties that cannot be modelled in the original Petri net (e.g. timed Petri nets). If they can be modelled in the original Petri net, they are not real extensions, instead, they are convenient ways of showing the same thing, and can be transformed with mathematical formulas back to the original Petri net, without losing any meaning. Extensions that cannot be transformed are sometimes very powerful, but usually lack the full range of mathematical tools available to analyse normal Petri nets.

The term high-level Petri net is used for many Petri net formalisms that extend the basic P/T net formalism. This includes coloured Petri nets, hierarchical Petri nets, and all other extensions sketched in this section.

A short list of possible extensions:

  • In a standard Petri net, tokens are indistinguishable. In a Coloured Petri net, every token has a value. In popular tools for coloured Petri nets such as CPN Tools, the values of tokens are typed, and can be tested and manipulated with a functional programming language. A subsidiary of coloured Petri nets are the well-formed Petri nets, where the arc and guard expressions are restricted to make it easier to analyse the net.
  • Another popular extension of Petri nets is hierarchy: Hierarchy in the form of different views supporting levels of refinement and abstraction were studied by Fehling. Another form of hierarchy is found in so-called object Petri nets or object systems where a Petri net can contain Petri nets as its tokens inducing a hierarchy of nested Petri nets that communicate by synchronisation of transitions on different levels. See [3] for an informal introduction to object Petri nets.
  • A Vector Addition System with States (VASS) can be seen as a generalisation of a Petri net. Consider a finite state automaton where each transition is labelled by a transition from the Petri net. The Petri net is then synchronised with the finite state automaton, i.e., a transition in the automaton is taken at the same time as the corresponding transition in the Petri net. It is only possible to take a transition in the automaton if the corresponding transition in the Petri net is enabled, and it is only possible to fire a transition in the Petri net if there is a transition from the current state in the automaton labelled by it. (The definition of VASS is usually formulated slightly differently.)
  • Prioritised Petri nets add priorities to transitions, whereby a transition cannot fire, if a higher-priority transition is enabled (i.e. can fire). Thus, transitions are in priority groups, and e.g. priority group 3 can only fire if all transitions are disabled in groups 1 and 2. Within a priority group, firing is still non-deterministic.
  • The non-deterministic property has been a very valuable one, as it lets the user abstract a large number of properties (depending on what the net is used for). In certain cases, however, the need arises to also model the timing, not only the structure of a model. For these cases, timed Petri nets have evolved, where there are transitions that are timed, and possibly transitions which are not timed (if there are, transitions that are not timed have a higher priority than timed ones). A subsidiary of timed Petri nets are the stochastic Petri nets that add nondeterministic time through adjustable randomness of the transitions. The exponential random distribution is usually used to 'time' these nets. In this case, the nets' reachability graph can be used as a Markov chain.

There are many more extensions to Petri nets, however, it is important to keep in mind, that as the complexity of the net increases in terms of extended properties, the harder it is to use standard tools to evaluate certain properties of the net. For this reason, it is a good idea to use the most simple net type possible for a given modelling task.

[edit] Main Petri net types

Petri net types graphically
Petri net types graphically

There are six main types of petri net:

  1. State Machine (SM) - here, every transition has one incoming arc, and one outgoing arc. This means, that there can not be concurrency, but there can be conflict (i.e. Where should the token from the place go? To one transition or the other?). Mathematically: \forall t\in T: |t\bullet|=|\bullet t|=1
  2. Marked Graph (MG) - here, every place has one incoming arc, and one outgoing arc. This means, that there can not be conflict, but there can be concurrency. Mathematically: \forall s\in S: |s\bullet|=|\bullet s|=1
  3. Free choice (FC) - here, an arc is either the only arc going from the place, or it is the only arc going to a transition. I.e. there can be both concurrency and conflict, but not at the same time. Mathematically: \forall s\in S: (|s\bullet|\leq 1) \vee (\bullet (s\bullet)=\{s\})
  4. Extended free choice (EFC) - a Petri net that can be transformed into an FC.
  5. Asymmetric choice (AC) - concurrency and conflict (in sum, confusion), but not asymmetrically. Mathematically: \forall s_1,s_2\in S: (s_1\bullet \cap s_2\bullet\neq 0) \to [(s_1\bullet\subseteq s_2\bullet) \vee (s_2\bullet\subseteq s_1\bullet)]
  6. Multiple Asymmetric choice (MAC) - multiple concurrency and conflict (in sum, multiple confusion). Mathematically: for a set |P|=k, \forall t\in T exist a subset  \bullet t, and  \bullet T contains all subset and is the Power Set 2k without the empty subset
  7. Petri Net (PN) - confusion is allowed (i.e. everything is allowed)

[edit] Other models of concurrency

Other ways of modelling concurrent computation have been proposed, including process algebra, the actor model, and the theory of traces[2]. Different models provide tradeoffs of concepts such as compositionality, modularity, and locality.

An approach to relating some of these models of concurrency is proposed in the chapter by Winskel and Nielsen[3].

[edit] Application areas

[edit] Programming tools

[edit] See also

[edit] References

  • Cardoso, Janette; Heloisa Camargo. Fuzziness in Petri Nets. Physica-Verlag. ISBN 3-7908-1158-0. 
  • Jensen, Kurt. Coloured Petri Nets. Springer Verlag. ISBN 3-540-62867-3. 
  • Котов, Вадим (1984). Сети Петри (Petri Nets, in Russian). Наука, Москва. 
  • Pataricza, András (2004). Formális moódszerek az informatikában (Formal methods in informatics). TYPOTEX Kiadó. ISBN 963-9548-08-1. 
  • Peterson, James L. (1977). "Petri Nets". ACM Computing Surveys 9 (3): 223–252. doi:10.1145/356698.356702. 
  • Peterson, James Lyle. Petri Net Theory and the Modeling of Systems. Prentice Hall. ISBN 0-13-661983-5. 
  • Petri, Carl A. (1962). "Kommunikation mit Automaten". Ph. D. Thesis. . University of Bonn
  • Reisig, Wolfgang. A Primer in Petri Net Design. Springer-Verlag. ISBN 3-540-52044-9. 
  • Riemann, Robert-Christoph. Modelling of Concurrent Systems: Structural and Semantical Methods in the High Level Petri Net Calculus. Herbert Utz Verlag. ISBN 3-89675-629-X. 
  • Störrle, Harald. Models of Software Architecture - Design and Analysis with UML and Petri-Nets. Books on Demand. ISBN 3-8311-1330-0.  With courtesy of the author, freely available online.
  • Zhou, Mengchu; Frank Dicesare. Petri Net Synthesis for Discrete Event Control of Manufacturing Systems. Kluwer Academic Publishers. ISBN 0-7923-9289-2. 
  • Zhou, Mengchu; Kurapati Venkatesh. Modeling, Simulation, & Control of Flexible Manufacturing Systems: A Petri Net Approach. World Scientific Publishing. ISBN 981-02-3029-X. 

[edit] Footnotes

  1. ^ Desel, Jörg and Juhás, Gabriel "What Is a Petri Net? Informal Answers for the Informed Reader", Hartmut Ehrig et al. (Eds.): Unifying Petri Nets, LNCS 2128, pp. 1-25, 2001. [1]
  2. ^ Antoni Mazurkiewicz, "Introduction to Trace Theory", in The Book of Traces V. Diekert, G. Rozenberg, eds. World Scientific, Singapore (1995) pp 3-67.
  3. ^ G. Winskel, M. Nielsen. "Models for Concurrency". Handbook of Logic and the Foundations of Computer Science, vol. 4, pages 1-148, OUP.

[edit] External links