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Brandon McKinzieOctober 2014
Analysis of the Upsilon Meson:
Polarization Systematic Uncertainty at CMS
1 / 10
Compact Muon Solenoid (CMS)
Upsilon Event at CMS
Brandon McKinzieOctober 2014
Unknown:
Degree of Upsilon Polarization
Physics Motivation
Early universe was in Quark-Gluon
Plasma (QGP) state.
Upsilon meson is a temperature
probe and indicator of
deconfinement in the QGP.
Need to understand Upsilon.
Time Evolution of Universe
Upsilon Event in CMS
2 / 10
Brandon McKinzieOctober 2014
The Upsilon Meson
● What is it?
– More Specifically:
b
b
* Masses of different energy states:
→ Υ(1S) : 9.46 GeV/c2
→ Υ(2S) : 10.02 GeV/c2
→ Υ(3S) : 10.36 GeV/c2
* Discovered in 1977
* First observation of the bottom quark
3 / 10
Brandon McKinzieOctober 2014
Upsilon Polarization
Using this definition,
simulate millions of
proton-proton collisions.
4 / 10
Goal: Obtain estimate for polarization systematic uncertainty at CMS.
Brandon McKinzieOctober 2014
Contradiction in Data!
CDF and DØ Collaborations
5 / 10
We expect the CDF and D0 results to be similar,
and we have no explanation for the observed difference.
- DØ Collaboration
*proton-antiproton collisions
DØ Collaboration and NRQCD Prediction
Brandon McKinzieOctober 2014
Methodology
1) Simulate millions of p-p collisions in PYTHIA.
– Require Υ → μ+
μ-
in each event
2) Upsilon pT
is plotted for each polarization case.
– Polarization modeled by applying α weights (see slide 4).
3) Cuts are applied to each polarization case to model
detector acceptance and online event selection.
4) Systematic Uncertainty is estimated by differences in
acceptance magnitudes for polarized vs. unpolarized cases.
6 / 10
Brandon McKinzieOctober 2014
Polarization at STAR
For the STAR detector at RHIC.
200 GeV of energy per-nucleon pair.
Begin with all dimuons produced in
1 million proton-proton collisions.
And then allow only those dimuons
within region of detector acceptance:
|ημ
| < 1
Begin with dimuons that have
→ pT
(1)
> 4 GeV/c
→ pT
(2)
> 2.5 GeV/c
→ cos(θ) < 0.5
And then allow only dimuons
within detector acceptance region:
|ημ
| < 1
7 / 10
Brandon McKinzieOctober 2014
Polarization at CMS
For the CMS detector at the LHC.
2.76 TeV of energy per-nucleon pair.
Begin with dimuons that have
→ pT
(1)
> 4 GeV/c
→ pT
(2)
> 3.5 GeV/c
and then allow only those within
detector acceptance region:
|ημ
| < 2.4
8 / 10
Begin with all dimuons produced in
3 million proton-proton collisions.
And then allow only those dimuons
within region of detector acceptance:
|ημ
| < 2.4
Brandon McKinzieOctober 2014
Systematic Uncertainty
9 / 10
Brandon McKinzieOctober 2014
Conclusions
The systematic error for Upsilon polarization at CMS is
similar to what has been found at STAR, but with important
differences in momentum crossover values and magnitudes
of acceptance.
Although the experimental data is still inconclusive, this
uncertainty estimate can provide intuition regarding how
results may fluctuate depending on the degree of Upsilon
polarization.
10 / 10
Brandon McKinzieOctober 2014
Acknowledgements
Thanks!
Advisors: Manuel Calderón de la Barca Sánchez and Daniel Cebra:
The UC Davis Nuclear Physics Group:
The American Physical Society, Far West Section:

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APSMeetingPresentation

  • 1. Brandon McKinzieOctober 2014 Analysis of the Upsilon Meson: Polarization Systematic Uncertainty at CMS 1 / 10 Compact Muon Solenoid (CMS) Upsilon Event at CMS
  • 2. Brandon McKinzieOctober 2014 Unknown: Degree of Upsilon Polarization Physics Motivation Early universe was in Quark-Gluon Plasma (QGP) state. Upsilon meson is a temperature probe and indicator of deconfinement in the QGP. Need to understand Upsilon. Time Evolution of Universe Upsilon Event in CMS 2 / 10
  • 3. Brandon McKinzieOctober 2014 The Upsilon Meson ● What is it? – More Specifically: b b * Masses of different energy states: → Υ(1S) : 9.46 GeV/c2 → Υ(2S) : 10.02 GeV/c2 → Υ(3S) : 10.36 GeV/c2 * Discovered in 1977 * First observation of the bottom quark 3 / 10
  • 4. Brandon McKinzieOctober 2014 Upsilon Polarization Using this definition, simulate millions of proton-proton collisions. 4 / 10 Goal: Obtain estimate for polarization systematic uncertainty at CMS.
  • 5. Brandon McKinzieOctober 2014 Contradiction in Data! CDF and DØ Collaborations 5 / 10 We expect the CDF and D0 results to be similar, and we have no explanation for the observed difference. - DØ Collaboration *proton-antiproton collisions DØ Collaboration and NRQCD Prediction
  • 6. Brandon McKinzieOctober 2014 Methodology 1) Simulate millions of p-p collisions in PYTHIA. – Require Υ → μ+ μ- in each event 2) Upsilon pT is plotted for each polarization case. – Polarization modeled by applying α weights (see slide 4). 3) Cuts are applied to each polarization case to model detector acceptance and online event selection. 4) Systematic Uncertainty is estimated by differences in acceptance magnitudes for polarized vs. unpolarized cases. 6 / 10
  • 7. Brandon McKinzieOctober 2014 Polarization at STAR For the STAR detector at RHIC. 200 GeV of energy per-nucleon pair. Begin with all dimuons produced in 1 million proton-proton collisions. And then allow only those dimuons within region of detector acceptance: |ημ | < 1 Begin with dimuons that have → pT (1) > 4 GeV/c → pT (2) > 2.5 GeV/c → cos(θ) < 0.5 And then allow only dimuons within detector acceptance region: |ημ | < 1 7 / 10
  • 8. Brandon McKinzieOctober 2014 Polarization at CMS For the CMS detector at the LHC. 2.76 TeV of energy per-nucleon pair. Begin with dimuons that have → pT (1) > 4 GeV/c → pT (2) > 3.5 GeV/c and then allow only those within detector acceptance region: |ημ | < 2.4 8 / 10 Begin with all dimuons produced in 3 million proton-proton collisions. And then allow only those dimuons within region of detector acceptance: |ημ | < 2.4
  • 10. Brandon McKinzieOctober 2014 Conclusions The systematic error for Upsilon polarization at CMS is similar to what has been found at STAR, but with important differences in momentum crossover values and magnitudes of acceptance. Although the experimental data is still inconclusive, this uncertainty estimate can provide intuition regarding how results may fluctuate depending on the degree of Upsilon polarization. 10 / 10
  • 11. Brandon McKinzieOctober 2014 Acknowledgements Thanks! Advisors: Manuel Calderón de la Barca Sánchez and Daniel Cebra: The UC Davis Nuclear Physics Group: The American Physical Society, Far West Section: