Quickstart

Your analysis starts by defining an amplitude model that describes the reaction process you want to study. Such a model is generally very complex and requires a fair amount of effort by the analyst (you). This also gives a lot of room for mistakes.

The ‘expert system’ is responsible to give you advice on the form of an amplitude model based on the problem set you define (initial state, final state, allowed interactions, intermediate states, etc.). Internally, the system propagates the quantum numbers through the reaction graph while satisfying the specified conservation rules. How to control this procedure is explained in more detail below.

Afterwards, the amplitude model of the expert system can be exported into ComPWA or Tensorwaves. The model can for instance be used to generate a data set (toy Monte Carlo) for this reaction and to optimize its parameters to resemble an actual data set as good as possible.

1.1. Define the problem set

We first define the boundary conditions of our physics problem, such as initial state, final state, formalism type, etc. and pass all of that information to the StateTransitionManager. This is the main user interface class of the expertsystem.

By default, the StateTransitionManager loads all particles from the PDG. The expertsystem would take a long time to check the quantum numbers of all these particles, so in this quickstart, we use a smaller subset of relatively common particles.

[1]:
from expertsystem.reaction import InteractionTypes, StateTransitionManager
[2]:
stm = StateTransitionManager(
    initial_state=["J/psi(1S)"],
    final_state=["gamma", "pi0", "pi0"],
    allowed_intermediate_particles=[
        "f(0)(980)",
        "f(0)(1500)",
        "f(2)(1270)",
        "f(2)(1950)",
        "omega(782)",
        "D*(2007)0",
        "rho(770)0",
        "phi(1020)",
        "a(0)(980)0",
    ],
    formalism_type="helicity",
)

Hint

How does the StateTransitionManager know what a "J/psi(1S)" is? Upon construction, the StateTransitionManager loads default definitions from the PDG. See Particle database for how to add custom particle definitions.

1.2. Prepare topologies

Create all topology graphs using the isobar model (tree of two-body decays) and initialize the graphs with the initial and final state. Remember that each interaction node defines its own set of conservation laws.

The StateTransitionManager (STM) defines three interaction types:

Interaction

Strength

strong

\(60\)

electromagnetic (EM)

\(1\)

weak

\(10^{-4}\)

By default, all three are used in the preparation stage. The function prepare_graphs() of the STM generates graphs with all possible combinations of interaction nodes. An overall interaction strength is assigned to each graph and they are grouped according to this strength.

[3]:
graph_interaction_settings_groups = stm.prepare_graphs()

1.3. Find solutions

If you are happy with the default settings generated by the StateTransitionManager, just start with solving directly!

This step takes about 30 sec on an Intel(R) Core(TM) i7-6820HQ CPU of 2.70GHz running, multi-threaded.

[4]:
result = stm.find_solutions(graph_interaction_settings_groups)

The find_solutions method returns a Result object from which you can extract the solutions and any violated_rules in case solutions were found. Now, you can use Result.get_intermediate_particles to print the names of the intermediate states that the StateTransitionManager found:

[5]:
print("found", len(result.solutions), "solutions!")
result.get_intermediate_particles().names
found 108 solutions!
[5]:
{'a(0)(980)0',
 'f(0)(1500)',
 'f(0)(980)',
 'f(2)(1270)',
 'f(2)(1950)',
 'omega(782)',
 'phi(1020)',
 'rho(770)0'}

Now we have a lot of solutions that are actually heavily suppressed (they involve two weak decays).

In general, you can modify the dictionary returned by prepare_graphs() directly, but the STM also comes with functionality to globally choose the allowed interaction types.

So, go ahead and disable the EM and weak interaction:

[6]:
stm.set_allowed_interaction_types([InteractionTypes.Strong])
graph_interaction_settings_groups = stm.prepare_graphs()
result = stm.find_solutions(graph_interaction_settings_groups)

print("found", len(result.solutions), "solutions!")
result.get_intermediate_particles().names
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
WARNING:root:The specified list of interaction types [<InteractionTypes.Strong: 1>] does not intersect with the valid list of interaction types [<InteractionTypes.EM: 2>].
Using valid list instead.
found 60 solutions!
[6]:
{'f(0)(1500)', 'f(0)(980)', 'f(2)(1270)', 'f(2)(1950)', 'rho(770)0'}

Huh, what happened here? Actually, since a \(\gamma\) particle appears in one of the interaction nodes, the expert system knows that this node must involve EM interactions! Because the node can be an effective interaction, the weak interaction cannot be excluded, as it contains only a subset of conservation laws.

Since only the strong interaction was supposed to be used, this results in a warning and the STM automatically corrects the mistake.

Once the EM interaction is included, this warning disappears. Be aware, however, that the EM interaction is now available globally. Hence, there now might be solutions in which both nodes are electromagnetic.

[7]:
stm.set_allowed_interaction_types([InteractionTypes.Strong, InteractionTypes.EM])
graph_interaction_settings_groups = stm.prepare_graphs()
result = stm.find_solutions(graph_interaction_settings_groups)

print("found", len(result.solutions), "solutions!")
result.get_intermediate_particles().names
found 90 solutions!
[7]:
{'a(0)(980)0',
 'f(0)(1500)',
 'f(0)(980)',
 'f(2)(1270)',
 'f(2)(1950)',
 'omega(782)',
 'phi(1020)',
 'rho(770)0'}

Great! Now we selected only the strongest contributions. Be aware, though, that there are more effects that can suppress certain decays, like small branching ratios. In this example, the initial state \(J/\Psi\) can decay into \(\pi^0 + \rho^0\) or \(\pi^0 + \omega\).

decay

branching ratio

\[\omega \rightarrow \gamma+\pi^0\]

0.0828

\[\rho^0 \rightarrow \gamma+\pi^0\]

0.0006

Unfortunately, the \(\rho^0\) mainly decays into \(\pi+\pi\), not \(\gamma+\pi^0\) and is therefore suppressed. This information is currently not known to the expert system, but it is possible to hand the expert system a list of allowed intermediate states.

[8]:
# particles are found by name comparison,
# i.e. f2 will find all f2's and f all f's independent of their spin
stm.allowed_intermediate_particles = ["f(0)", "f(2)"]

result = stm.find_solutions(graph_interaction_settings_groups)

print("found", len(result.solutions), "solutions!")
result.get_intermediate_particles().names
found 90 solutions!
[8]:
{'a(0)(980)0',
 'f(0)(1500)',
 'f(0)(980)',
 'f(2)(1270)',
 'f(2)(1950)',
 'omega(782)',
 'phi(1020)',
 'rho(770)0'}

Now we have selected all amplitudes that involve f states. The warnings appear only to notify the user that the list of solutions is not exhaustive: for certain edges in the graph, no suitable particle was found (since only f states were allowed).

1.4. Generate an amplitude model

Now that we are satisfied with the intermediate resonances, we are all set convert the solutions that the STM found to an amplitude model! This can be done with generate_amplitude_model. Depending on the formalism type that you chose when constructing the STM, generate_amplitude_model will use for instance HelicityAmplitudeGenerator if you chose to work with formalism type "helicity".

The result is an AmplitudeModel from which you can extract all information about Particle instances, FitParameters, Kinematics etc.

[9]:
from expertsystem.amplitude import generate_amplitude_model

amplitude_model = generate_amplitude_model(result)
amplitude_model.particles.names
[9]:
{'J/psi(1S)',
 'a(0)(980)0',
 'f(0)(1500)',
 'f(0)(980)',
 'f(2)(1270)',
 'f(2)(1950)',
 'gamma',
 'omega(782)',
 'phi(1020)',
 'pi0',
 'rho(770)0'}

Note

In this example, we used the helicity formalism. If you want to work with the canonical formalism, you have to construct the StateTransitionManager with argument formalism_type="canonical-helicity" instead of formalism_type="helicity".

Finally, you can use the expertsystem.io to write the AmplitudeModel to a file (either XML or YAML):

[10]:
from expertsystem import io

io.write(amplitude_model, filename="model.xml")
io.write(amplitude_model, filename="model.yml")

This allows you to cache file AmplitudeModel to disk and then load it back using load_amplitude_model:

[11]:
imported_model_xml = io.load_amplitude_model(filename="model.xml")
imported_model_yml = io.load_amplitude_model(filename="model.yml")

assert imported_model_xml == amplitude_model
assert imported_model_yml == amplitude_model

Have a look through the sections of the resulting XML or YAML recipe file to see what you recognize from the problem set defined above. There may also be some things you want to change in there manually, so make sure you store this recipe file carefully (e.g. track it with Git) as to avoid overwriting it your changes after rerunning the expert system.

Now you can use this recipe file as an amplitude model in a PWA framework!