Muons and Taus
Overview
Teaching: 10 min
Exercises: 0 minQuestions
How are muons and taus treated in CMS OpenData?
Objectives
Learn member functions for muon track-based quantities
Bookmark informational web pages for different objects
Learn member functions for identification and isolation of muons and taus
Muons and tau leptons are have many features that are similar to electrons and photons, but their own unique identification algorithms. In this episode we will be studying MuonAnalyzer.cc
and TauAnalyzer.cc
. We explored the muon kinematics member functions in Episode 1, which are identical for all objects.
CMS TWiki references:
- Muons: SWGuide Muon ID
- Tau leptons: Legacy Tau ID Run 1, Nutshell Recipe
Muon identification and isolation
Muons have a different member functions for accessing the associated track compared to electrons:
auto trk = itmuon->globalTrack();
if (trk.isNonnull()) {
muon_dxy.push_back(trk->dxy(pv));
muon_dz.push_back(trk->dz(pv));
muon_dxyErr.push_back(trk->d0Error());
muon_dzErr.push_back(trk->dzError());
}
The CMS Muon object group has created member functions for the identification algorithms that simply storing pass/fail decisions about the quality of each muon. As shown below, the algorithm depends on which vertex is being considered as the primary interaction vertex!
Hard processes produce large angles between the final state partons. The final object of interest will be separated from the other objects in the event or be “isolated”. For instance, an isolated muon might be produced in the decay of a W boson. In contrast, a non-isolated muon can come from a weak decay inside a jet.
Muon isolation is calculated from a combination of factors: energy from charged hadrons, energy from neutral hadrons, and energy from photons, all in a cone of radius dR < 0.3 or 0.4 around the muon. Many algorithms also feature a “correction factor” that subtracts average energy expected from pileup contributions to this cone – we’ll explore this in the hands-on exercise. Decisions are made by comparing this energy sum to the transverse momentum of the muon.
if (itmuon->isPFMuon() && itmuon->isPFIsolationValid()) {
auto iso04 = itmuon->pfIsolationR04();
muon_pfreliso04all.push_back((iso04.sumChargedHadronPt + iso04.sumNeutralHadronEt + iso04.sumPhotonEt)/itmuon->pt());
}
muon_tightid.push_back(muon::isTightMuon(*itmuon, *vertices->begin()));
Tau identification
The CMS Tau object group relies almost entirely on pre-computed algorithms to determine the quality of the tau reconstruction and the decay type. Since this object is not stable and has several decay modes, different combinations of identification and isolation algorithms are used across different analyses. The TWiki page provides a large table of available algorithms.
In contrast to the muon object, tau algorithm results are typically saved in the AOD files as their own PFTauDisciminator collections, rather than as part of the tau object class.
// Get the tau collection (the exact name is given in poet_cfg.py
Handle<reco::PFTauCollection> mytaus;
iEvent.getByLabel(tauInput, mytaus); // tauInput opens "hpsPFTauProducer"
// Get various tau discriminator collections
Handle<PFTauDiscriminator> tausLooseIso, tausVLooseIso, tausMediumIso, tausTightIso,
tausDecayMode, tausRawIso;
iEvent.getByLabel(InputTag("hpsPFTauDiscriminationByDecayModeFinding"),tausDecayMode);
iEvent.getByLabel(InputTag("hpsPFTauDiscriminationByRawCombinedIsolationDBSumPtCorr"),tausRawIso);
iEvent.getByLabel(InputTag("hpsPFTauDiscriminationByVLooseCombinedIsolationDBSumPtCorr"),tausVLooseIso);
//...etc...
The tau discriminator collections act as pairs, containing the index of the tau and the value of the discriminant for that tau. Note that the arrays are filled by calls to the individual discriminant objects, but referencing the vector index of the tau in the main tau collection.
for (reco::PFTauCollection::const_iterator itTau=mytaus->begin(); itTau!=mytaus->end(); ++itTau){
// store the tau decay mode
tau_decaymode.push_back(itTau->decayMode());
// Discriminators
const auto idx = itTau - mytaus->begin();
tau_iddecaymode.push_back(tausDecayMode->operator[](idx).second);
tau_idisoraw.push_back(tausRawIso->operator[](idx).second);
tau_idisovloose.push_back(tausVLooseIso->operator[](idx).second);
// ...etc...
}
Generator-level particles
In simulation, we can access generated particles from the event generation process.
You can configure poet_cfg.py
to store information about generated particles with any Particle Data Group ID numbers and generator status codes.
By default, we will store information for final state electrons, muons, and photons, and taus with an intermediate status:
process.mygenparticle= cms.EDAnalyzer('GenParticleAnalyzer',
#---- Collect particles with specific "pdgid:status"
#---- Check PDG ID in the PDG.
#---- if 0:0, collect them all
input_particle = cms.vstring("1:11","1:13","1:22","2:15")
)
The particles’ properties are stored in GenParticleAnalyzer.cc
. The input collection is not configurable because it is constant across all CMS simulation
samples: “genParticles”.
Handle<reco::GenParticleCollection> gens;
iEvent.getByLabel("genParticles", gens);
We then process the configurable input_particle
string that was provided from the configuration file. The constructor opens this parameter into a vector of strings called particle
:
GenParticleAnalyzer::GenParticleAnalyzer(const edm::ParameterSet& iConfig):
particle(iConfig.getParameter<std::vector<std::string> >("input_particle"))
{
//now do what ever initialization is needed
...code...
}
In the analyze
function we can parse the desired particle/status pairs and check each generated particle against these conditions before storing its kinematic properties, status, and PDG ID into tree branches:
unsigned int i;
string s1,s2;
std::vector<int> status_parsed;
std::vector<int> pdgId_parsed;
std::string delimiter = ":";
for(i=0;i<particle.size();i++)
{
//get status and pgdId from configuration
s1=particle[i].substr(0,particle[i].find(delimiter));
s2=particle[i].substr(particle[i].find(delimiter)+1,particle[i].size());
//parse string to int
status_parsed.push_back(stoi(s1));
pdgId_parsed.push_back(stoi(s2));
}
if(gens.isValid())
{
numGenPart=gens->size();
for (reco::GenParticleCollection::const_iterator itGenPart=gens->begin(); itGenPart!=gens->end(); ++itGenPart)
{
//loop trough all particles selected in configuration
for(i=0;i<particle.size();i++)
{
if((status_parsed[i]==itGenPart->status() && pdgId_parsed[i]==itGenPart->pdgId())||(status_parsed[i]==0 && pdgId_parsed[i]==0))
{
GenPart_pt.push_back(itGenPart->pt());
GenPart_eta.push_back(itGenPart->eta());
GenPart_mass.push_back(itGenPart->mass());
GenPart_pdgId.push_back(itGenPart->pdgId());
GenPart_phi.push_back(itGenPart->phi());
GenPart_status.push_back(itGenPart->status());
GenPart_px.push_back(itGenPart->px());
GenPart_py.push_back(itGenPart->py());
GenPart_pz.push_back(itGenPart->pz());
}
}
}
}
Matching between generated and reconstructed particles is typically done based on spatial relationships. For example, the generated muon (ID = 13) “matched” to a certain reconstructed muon would be the generated muon that has the smallest angular separation from the reconstructed muon. Angular separation is defined as:
An example analysis code that opens a POET file and performs generated particle matching for several types of reconstructed objects is called MatchingAnalysis.cc. This provides an example of looping over reconstructed objects (say, muons) and finding the generated particle of the same type that minimizes “dR”. A CMSSW built-in function helps calculate dR between the reconstructed object and each generated particle:
float minDeltaR = 999.0;
float r;
Int_t j_matched;
tevent->AddFriend(tgenparticles);
tevent->GetEntry(event);
for (Int_t j=0; j<numGenPart;++j)
{
r = deltaR(GenPart_eta->at(j),GenPart_phi->at(j),object_eta,object_phi);
if (r < minDeltaR && abs(GenPart_pdgId->at(j)) == object_pdgId)
{
minDeltaR = r;
j_matched=j;
}
}
Key Points
Track access may differ, but track-related member functions are common across objects.
Physics objects in CMS are reconstructed from detector signals and are never 100% certain!
Muons and taus typically use pre-configured identification and isolation variable member functions.
Member functions for these algorithms are documented on public TWiki pages.