Lesson 14 of 15

Cross Section Units and Luminosity

Cross Section Units and Luminosity

In particle physics experiments the interaction probability between two particles is quantified by the cross section σ\sigma — a measure of the effective area for a given process.

The Barn and its Submultiples

The natural unit for cross sections is the barn:

1 b=1028 m2=1024 cm21 \text{ b} = 10^{-28} \text{ m}^2 = 10^{-24} \text{ cm}^2

Modern collider physics works with much smaller cross sections:

UnitValue
1 mb (millibarn)10310^{-3} b
1 μb (microbarn)10610^{-6} b
1 nb (nanobarn)10910^{-9} b
1 pb (picobarn)101210^{-12} b
1 fb (femtobarn)101510^{-15} b

Conversion from Natural Units

In natural units (where =c=1\hbar = c = 1), cross sections are computed in GeV2^{-2}. The conversion to physical units uses:

1 GeV2=0.3894 mb=3.894×108 pb1 \text{ GeV}^{-2} = 0.3894 \text{ mb} = 3.894 \times 10^8 \text{ pb}

Luminosity and Event Rates

The instantaneous luminosity L\mathcal{L} [cm2^{-2}s1^{-1}] relates the event rate RR to the cross section:

R=LσR = \mathcal{L} \cdot \sigma

The integrated luminosity Lint\mathcal{L}_{\text{int}} [fb1^{-1}] gives the total number of events:

Nevents=LintσN_{\text{events}} = \mathcal{L}_{\text{int}} \cdot \sigma

At the LHC, Run 2 (2015–2018) delivered about 140 fb1^{-1} of integrated luminosity at 13 TeV. Key benchmark cross sections:

  • ppHpp \to H (Higgs production via gluon fusion): σ55\sigma \approx 55 pb at 13 TeV
  • ppZpp \to Z: σ60\sigma \approx 60 nb =60,000= 60{,}000 pb

Your Task

Implement:

  • GeV2_to_pb(sigma_GeV2) — convert cross section from GeV2^{-2} to pb
  • events_expected(sigma_pb, luminosity_fb_inv) — number of events (1 fb1^{-1} = 1000 pb1^{-1})
  • luminosity_from_rate(event_rate_per_s, sigma_cm2) — instantaneous luminosity in cm2^{-2}s1^{-1}

All constants must be defined inside each function body.

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